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Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Spectral shaping of cascade emissions from multiplexed cold atomic ensembles</style></title><secondary-title><style face="normal" font="default" size="100%"> Physical Review A</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2016</style></year></dates><volume><style face="normal" font="default" size="100%">93 </style></volume><pages><style face="normal" font="default" size="100%">013811 </style></pages></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Hsiao, Ya-Fen</style></author><author><style face="normal" font="default" size="100%">Pin-Ju Tsai</style></author><author><style face="normal" font="default" size="100%">Chi-Ching Lin</style></author><author><style face="normal" font="default" size="100%">Yong-Fan Chen</style></author><author><style face="normal" font="default" size="100%">Ite A. Yu</style></author><author><style face="normal" font="default" size="100%">Ying-Cheng Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Coherence properties of amplified slow light by four-wave mixing</style></title><secondary-title><style face="normal" font="default" size="100%">Optics Letters</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2014</style></year></dates><volume><style face="normal" font="default" size="100%">39</style></volume><pages><style face="normal" font="default" size="100%">3394-3397</style></pages><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We present an experimental study of the coherence properties of amplified slow light by four-wave mixing (FWM) in a three-level electromagnetically induced transparency (EIT) system driven by one additional pump field. High energy gain (up to 19) is obtained with a weak pump field (a few mW∕cm2) using optically dense cold atomic gases. A large fraction of the amplified light is found to be phase incoherent to the input signal field. The dependence of the incoherent fraction on pump field intensity and detuning and the control field intensity is systematically studied. With the classical input pulses, our results support a recent theoretical study by Lauk et al. [Phys. Rev. A 88, 013823 (2013)], showing that the noise resulting from the atomic dipole fluctuations associated with spontaneous decay is significant in the high gain regime. This effect has to be taken into consideration in EIT-based applications in the presence of FWM.&lt;/p&gt;
</style></abstract><issue><style face="normal" font="default" size="100%">12</style></issue></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Hsiao, Ya-Fen</style></author><author><style face="normal" font="default" size="100%">Hung-Shiue Chen</style></author><author><style face="normal" font="default" size="100%">Pin-Ju Tsai</style></author><author><style face="normal" font="default" size="100%">Ying-Cheng Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Cold atomic media with ultrahigh optical depths</style></title><secondary-title><style face="normal" font="default" size="100%">Phys. Rev. A</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2014</style></year></dates><volume><style face="normal" font="default" size="100%">90</style></volume><pages><style face="normal" font="default" size="100%">054401</style></pages><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We present an experimental study to achieve ultrahigh optical depths for cold atomic media with a two dimensional magneto-optical trap (MOT) of cesium. By combining large atom number, a temporally dark and compressed MOT, and Zeeman-state optical pumping, we achieve an optical depth of up to 1306 for the open transition of the cesium D1 line. Our work demonstrates that it is feasible to push the optical depth up to the 1000 level with a convenient MOT setup. This development paves the way to many important proposals in quantum optics and many-body physics. &lt;/p&gt;
</style></abstract></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Yi-Hsin Chen</style></author><author><style face="normal" font="default" size="100%">Meng-Jung Lee</style></author><author><style face="normal" font="default" size="100%">Hung, Weilun</style></author><author><style face="normal" font="default" size="100%">Ying-Cheng Chen</style></author><author><style face="normal" font="default" size="100%">Yong-Fan Chen</style></author><author><style face="normal" font="default" size="100%">Ite A. Yu</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Interaction between two stopped light pulses</style></title><secondary-title><style face="normal" font="default" size="100%">AIP Conference Proceedings </style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2014</style></year></dates><volume><style face="normal" font="default" size="100%">1588</style></volume><pages><style face="normal" font="default" size="100%">17-26</style></pages><abstract><style face="normal" font="default" size="100%">&lt;p&gt;The efficiency of a nonlinear optical process is proportional to the interaction time. We report a scheme of all-optical switching based on two motionless light pulses via the effect of electromagnetically induced transparency. One pulse was stopped as the stationary light pulse (SLP) and the other was stopped as stored light. The time of their interaction via the medium can be prolonged and, hence, the optical nonlinearity is greatly enhanced. Using a large optical density (OD) of 190, we achieved a very long interaction time of 6.9 μs. This can be analogous to the scheme of trapping light pulses by an optical cavity with a Q factor of 8×109. With the approach of using moving light pulses in the best situation, a switch can only be activated at 2 photons per atomic absorption cross section. With the approach of employing a SLP and a stored light pulse, a switch at only 0.56 photons was achieved and the efficiency is significantly improved. Moreover, the simulation results are in good agreement with the experimental data and show that the efficiency can be further improved by increasing the OD of the medium. Our work advances the technology in quantum information manipulation utilizing photons.&lt;/p&gt;
</style></abstract></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Chang-Kai Chiu</style></author><author><style face="normal" font="default" size="100%">Yi-Hsin Chen</style></author><author><style face="normal" font="default" size="100%">Chen, Yen-Chun</style></author><author><style face="normal" font="default" size="100%">Ite A. Yu</style></author><author><style face="normal" font="default" size="100%">Ying-Cheng Chen</style></author><author><style face="normal" font="default" size="100%">Yong-Fan Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Low-light-level four-wave mixing by quantum interference</style></title><secondary-title><style face="normal" font="default" size="100%">Phys. Rev. A</style></secondary-title></titles><dates><year><style  face="normal" font="default" size="100%">2014</style></year></dates><volume><style face="normal" font="default" size="100%">89</style></volume><pages><style face="normal" font="default" size="100%">5</style></pages><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We observed electromagnetically induced transparency-based four-wave mixing (FWM) in the pulsed regime at low light levels. The FWM conversion efficiency of 3.8(9)% was observed in a four-level system of cold 87Rb atoms using a driving laser pulse with a peak intensity of ≈80 μW/cm2, corresponding to an energy of ≈60 photons per atomic cross section. Comparison between the experimental data and the theoretical predictions proposed by Harris and Hau [Phys. Rev. Lett. 82, 4611 (1999)] showed good agreement. Additionally, a high conversion efficiency of 46(2)% was demonstrated when applying this scheme using a driving laser intensity of ≈1.8 mW/cm2. According to our theoretical predictions, this FWM scheme can achieve a conversion efficiency of nearly 100% when using a dense medium with an optical depth of 500.&lt;/p&gt;
</style></abstract></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Chen, Y. H.</style></author><author><style face="normal" font="default" size="100%">Lee, M. J.</style></author><author><style face="normal" font="default" size="100%">Wang, I. C.</style></author><author><style face="normal" font="default" size="100%">Du, S. W.</style></author><author><style face="normal" font="default" size="100%">Y.F. Chen</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Coherent Optical Memory with High Storage Efficiency and Large Fractional Delay</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review Letters</style></secondary-title><short-title><style face="normal" font="default" size="100%">Coherent Optical Memory with High Storage Efficiency and Large Fractional Delay</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2013</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Feb</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000315141600009</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">8</style></number><volume><style face="normal" font="default" size="100%">110</style></volume><pages><style face="normal" font="default" size="100%">5</style></pages><isbn><style face="normal" font="default" size="100%">0031-9007</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;A high-storage efficiency and long-lived quantum memory for photons is an essential component in long-distance quantum communication and optical quantum computation. Here, we report a 78% storage efficiency of light pulses in a cold atomic medium based on the effect of electromagnetically induced transparency. At 50% storage efficiency, we obtain a fractional delay of 74, which is the best up-to-date record. The classical fidelity of the recalled pulse is better than 90% and nearly independent of the storage time, as confirmed by the direct measurement of phase evolution of the output light pulse with a beat-note interferometer. Such excellent phase coherence between the stored and recalled light pulses suggests that the current result may be readily applied to single photon wave packets. Our work significantly advances the technology of electromagnetically induced transparency-based optical memory and may find practical applications in long-distance quantum communication and optical quantum computation. DOI: 10.1103/PhysRevLett.110.083601&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000315141600009</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 092SF Times Cited: 0 Cited Reference Count: 33 Chen, Yi-Hsin Lee, Meng-Jung Wang, I-Chung Du, Shengwang Chen, Yong-Fan Chen, Ying-Cheng Yu, Ite A. National Science Council of Taiwan [100-2628-M-007-001, 101-2923-M-007-002]; National Tsing Hua University [101N2713E1]; Hong Kong Research Grants Council [600710]; EU [PIRSES-GA-2009-247475] This work was supported by the National Science Council of Taiwan under Grants No. 100-2628-M-007-001 and No. 101-2923-M-007-002 and by National Tsing Hua University under Grant No. 101N2713E1. S. D. was supported by the Hong Kong Research Grants Council (Project No. 600710). The Hsinchu team is the partner in EU FP7 IRSES project COLIMA (Contract No. PIRSES-GA-2009-247475). The authors thank Professor P. K. Lam for valuable comments on the manuscript. 0 Amer physical soc College pk&lt;/p&gt;
</style></notes><custom7><style face="normal" font="default" size="100%">083601</style></custom7><auth-address><style face="normal" font="default" size="100%">Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan. Natl Tsing Hua Univ, Frontier Res Ctr Fundamental &amp; Appl Sci Matters, Hsinchu 30013, Taiwan. Hong Kong Univ Sci &amp; Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China. Natl Cheng Kung Univ, Dept Phys, Tainan 70101, Taiwan. Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 10617, Taiwan. Chen, YH (reprint author), Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan. yu@phys.nthu.edu.tw</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Huang, S. J.</style></author><author><style face="normal" font="default" size="100%">Hsu, Y. T.</style></author><author><style face="normal" font="default" size="100%">Lee, H.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Volosniev, A. G.</style></author><author><style face="normal" font="default" size="100%">Zinner, N. T.</style></author><author><style face="normal" font="default" size="100%">Wang, D. W.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Field-induced long-lived supermolecules</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review A</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Phys Rev A</style></alt-title><short-title><style face="normal" font="default" size="100%">Field-induced long-lived supermolecules</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2012</style></year><pub-dates><date><style  face="normal" font="default" size="100%">May 7</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://000303651200012</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">85</style></volume><isbn><style face="normal" font="default" size="100%">1050-2947</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We demonstrate that the long-lived bound states (supermolecules) can exist in the dilute limit when we tune the shape of the effective potential between polar molecules by an external microwave field. Binding energies, average sizes, and phase diagrams for both s-orbital (bosons) and p-orbital (fermions) dimers are studied, together with bosonic trimer states. We explicitly show that the nonadiabatic transition rate can be easily tuned small for such ground-state supermolecules, so that the system can be stable from collapse even near the associated potential resonance. Our results, therefore, suggest a feasible cold molecule system to investigate novel few-body and many-body physics (for example, the p-wave BCS-Bose-Einstein-condensate crossover for fermions and the paired condensate for bosons) that cannot be easily accessed in single species atomic gases.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">ISI:000303651200012</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;937IC Times Cited:0 Cited References Count:39&lt;/p&gt;
</style></notes><custom7><style face="normal" font="default" size="100%">055601</style></custom7><auth-address><style face="normal" font="default" size="100%">Huang, SJ Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan Natl Tsing Hua Univ, Frontier Res Ctr Fundamental &amp; Appl Sci Matters, Hsinchu 30013, Taiwan Natl Ctr Theoret Sci, Div Phys, Hsinchu 30099, Taiwan Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 115, Taiwan Aarhus Univ, Dept Phys &amp; Astron, DK-8000 Aarhus C, Denmark</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Chi-Ching Lin</style></author><author><style face="normal" font="default" size="100%">Meng-Chang Wu</style></author><author><style face="normal" font="default" size="100%">Bor-Wen Shiau</style></author><author><style face="normal" font="default" size="100%">Yi-Hsin Chen</style></author><author><style face="normal" font="default" size="100%">Ite A. Yu</style></author><author><style face="normal" font="default" size="100%">Yong-Fan Chen</style></author><author><style face="normal" font="default" size="100%">Ying-Cheng Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Enhanced all-optical switching with double slow light pulses</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review A</style></secondary-title><short-title><style face="normal" font="default" size="100%">Enhanced all-optical switching with double slow light pulses</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2012</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Dec 28</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000312830200008</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">86</style></volume><isbn><style face="normal" font="default" size="100%">1050-2947</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">n/a</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000312830200008</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 0&lt;/p&gt;
</style></notes><custom7><style face="normal" font="default" size="100%">063836</style></custom7></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Yi-Hsin Chen</style></author><author><style face="normal" font="default" size="100%">Meng-Jung Lee</style></author><author><style face="normal" font="default" size="100%">Hung, Weilun</style></author><author><style face="normal" font="default" size="100%">Ying-Cheng Chen</style></author><author><style face="normal" font="default" size="100%">Yong-Fan Chen</style></author><author><style face="normal" font="default" size="100%">Ite A. Yu</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Demonstration of the Interaction between Two Stopped Light Pulses</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review Letters</style></secondary-title><short-title><style face="normal" font="default" size="100%">Demonstration of the Interaction between Two Stopped Light Pulses</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2012</style></year></dates><urls><web-urls><url><style face="normal" font="default" size="100%">http://link.aps.org/doi/10.1103/PhysRevLett.108.173603</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">108</style></volume><pages><style face="normal" font="default" size="100%">173603</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">n/a</style></abstract><notes><style face="normal" font="default" size="100%">&lt;p&gt;PRL&lt;/p&gt;
</style></notes></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Shiau, B. W.</style></author><author><style face="normal" font="default" size="100%">Wu, M. C.</style></author><author><style face="normal" font="default" size="100%">C.C. Lin</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Low-Light-Level Cross-Phase Modulation with Double Slow Light Pulses</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review Letters</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Phys. Rev. Lett.</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">ATOM</style></keyword><keyword><style  face="normal" font="default" size="100%">electromagnetically induced transparency</style></keyword><keyword><style  face="normal" font="default" size="100%">NONLINEAR OPTICS</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2011</style></year><pub-dates><date><style  face="normal" font="default" size="100%">May</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000290474100009</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">19</style></number><volume><style face="normal" font="default" size="100%">106</style></volume><pages><style face="normal" font="default" size="100%">4</style></pages><isbn><style face="normal" font="default" size="100%">0031-9007</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We report on the first experimental demonstration of low-light-level cross-phase modulation (XPM) with double slow light pulses based on the double electromagnetically induced transparency (EIT) in cold cesium atoms. The double EIT is implemented with two control fields and two weak fields that drive populations prepared in the two doubly spin-polarized states. Group velocity matching can be obtained by tuning the intensity of either of the control fields. The XPM is based on the asymmetric M-type five-level system formed by the two sets of EIT. Enhancement in the XPM by group velocity matching is observed. Our work advances studies of low-light-level nonlinear optics based on double slow light pulses.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000290474100009</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 762KCTimes Cited: 0Cited Reference Count: 20Cited References:      Anton MA, 2008, OPT COMMUN, V281, P6040, DOI 10.1016/j.optcom.2008.09.014     MacRae A, 2008, OPT LETT, V33, P2659, DOI 10.1364/OL.33.002659     Li SJ, 2008, PHYS REV LETT, V101     Lin YW, 2008, OPT EXPRESS, V16, P3753, DOI 10.1364/OE.16.003753     Chen YF, 2006, PHYS REV A, V74, DOI 10.1103/PhysRevA.74.063807     Ottaviani C, 2006, EUR PHYS J D, V40, P281, DOI 10.1140/epjd/e2006-00164-5     Wang ZB, 2006, PHYS REV LETT, V97, DOI 10.1103/PhysRevLett.97.063901     Chen YF, 2006, PHYS REV LETT, V96, DOI 10.1103/PhysRevLett.96.043603     Chen YF, 2005, PHYS REV A, V72, DOI 10.1103/PhysRevA.72.033812     Fleischhauer M, 2005, REV MOD PHYS, V77, P633, DOI 10.1103/RevModPhys.77.633     Rebic S, 2004, PHYS REV A, V70, DOI 10.1103/PhysRevA.70.032317     Petrosyan D, 2004, PHYS REV A, V70, DOI 10.1103/PhysRevA.70.023822     Kang HS, 2003, PHYS REV LETT, V91, DOI 10.1103/PhysRevLett.91.093601     Ottaviani C, 2003, PHYS REV LETT, V90, DOI 10.1103/PhysRevLett.90.197902     Matsko AB, 2003, OPT LETT, V28, P96, DOI 10.1364/OL.28.000096     Petrosyan D, 2002, PHYS REV A, V65, DOI 10.1103/PhysRevA.65.033833     Lukin MD, 2000, PHYS REV LETT, V84, P1419, DOI 10.1103/PhysRevLett.84.1419     Harris SE, 1999, PHYS REV LETT, V82, P4611, DOI 10.1103/PhysRevLett.82.4611     Hau LV, 1999, NATURE, V397, P594, DOI 10.1038/17561     Schmidt H, 1996, OPT LETT, V21, P1936, DOI 10.1364/OL.21.001936Shiau, Bor-Wen Wu, Meng-Chang Lin, Chi-Ching Chen, Ying-ChengNational Science Council of Taiwan under NSC[97-2112-M-028-MY3, 98-2628-M-001-003, 99-2628-M-001-021]We acknowledge fruitful discussions with Ite A. Yu and Yong-Fong Chen. This work was supported by the National Science Council of Taiwan under NSC Grants No. 97-2112-M-028-MY3, No. 98-2628-M-001-003, and No. 99-2628-M-001-021.AMER PHYSICAL SOCCOLLEGE PK&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">[Shiau, BW|Wu, MC|Lin, CC|Chen, YC] Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 10617, Taiwan.Shiau, BW (reprint author), Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 10617, Taiwan, Taiwanchenyc@pub.iams.sinica.edu.tw</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Lin, P. Y.</style></author><author><style face="normal" font="default" size="100%">Shiau, B. W.</style></author><author><style face="normal" font="default" size="100%">Hsiao, Y. F.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Creation of arbitrary spectra with an acousto-optic modulator and an injection-locked diode laser</style></title><secondary-title><style face="normal" font="default" size="100%">Review of Scientific Instruments</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Rev. Sci. Instrum.</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">BAND</style></keyword><keyword><style  face="normal" font="default" size="100%">FREQUENCY</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2011</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Aug</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000294486600009</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">8</style></number><volume><style face="normal" font="default" size="100%">82</style></volume><pages><style face="normal" font="default" size="100%">6</style></pages><isbn><style face="normal" font="default" size="100%">0034-6748</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We use a double-passed acousto-optic modulator (AOM), driven by an arbitrary waveform generator to produce multiple frequency components for a laser with arbitrary frequency spacings. A programmed sequence containing various sections of radio-frequency sinusoidal signal at different frequency is applied to drive the AOM. The diffracted light is used to injection-lock a diode laser. The combined techniques allow us to generate the multi-line spectra for the diode laser with arbitrary frequency spacings in the range of 100 MHz at a relatively high output power of 80 mW and a small power variation of 2%. Such a light source can be used in the application for laser cooling of molecules. (C) 2011 American Institute of Physics. [doi:10.1063/1.3626903]&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000294486600009</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 814VZTimes Cited: 0Cited Reference Count: 11Cited References:      ROGERS CE, 2011, REV SCI INSTRUM, V82     Shuman ES, 2010, NATURE, V467, P820     Johnson DMS, 2010, OPT LETT, V35, P745     Shuman ES, 2009, PHYS REV LETT, V103     Houtz R, 2009, OPT EXPRESS, V17, P19235     Tomita I, 2003, IEEE PHOTONIC TECH L, V15, P1204, DOI 10.1109/LPT.2003.816125     Buchkremer FBJ, 2000, REV SCI INSTRUM, V71, P3306, DOI 10.1063/1.1287633     Ferrari G, 1999, OPT LETT, V24, P151, DOI 10.1364/OL.24.000151     SINCLAIR AG, 1994, J OPT SOC AM B, V11, P2333, DOI 10.1364/JOSAB.11.002333     JOHNSON RV, 1979, APPL OPTICS, V18, P903, DOI 10.1364/AO.18.000903     DAGDIGIA.PJ, 1974, J CHEM PHYS, V60, P2330, DOI 10.1063/1.1681366Lin, Pei-Ying Shiau, Bor-Wen Hsiao, Ya-Fen Chen, Ying-ChengNational Science Council of Taiwan[98-2628-M-001-003, 99-2628-M-001-021]This work was supported by the National Science Council of Taiwan under NSC (Grant Nos. 98-2628-M-001-003 and 99-2628-M-001-021).AMER INST PHYSICSMELVILLE&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">[Lin, PY|Shiau, BW|Hsiao, YF|Chen, YC] Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 10617, Taiwan.Lin, PY (reprint author), Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 10617, Taiwanchenyc@pub.iams.sinica.edu.tw</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Lo, H. Y.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Su, P. C.</style></author><author><style face="normal" font="default" size="100%">Chen, H. C.</style></author><author><style face="normal" font="default" size="100%">Chen, J. X.</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author><author><style face="normal" font="default" size="100%">Y.F. Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Electromagnetically-induced-transparency-based cross-phase-modulation at attojoule levels</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review A</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Phys. Rev. A</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">ATOMS</style></keyword><keyword><style  face="normal" font="default" size="100%">CAVITY</style></keyword><keyword><style  face="normal" font="default" size="100%">KERR NONLINEARITIES</style></keyword><keyword><style  face="normal" font="default" size="100%">light</style></keyword><keyword><style  face="normal" font="default" size="100%">optics</style></keyword><keyword><style  face="normal" font="default" size="100%">PULSES</style></keyword><keyword><style  face="normal" font="default" size="100%">SHIFTS</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2011</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Apr</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000290105800004</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">4</style></number><volume><style face="normal" font="default" size="100%">83</style></volume><pages><style face="normal" font="default" size="100%">4</style></pages><isbn><style face="normal" font="default" size="100%">1050-2947</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We report the experimental demonstration of electromagnetically-induced-transparency-based cross-phase-modulation at attojoule or, equivalently, few-hundred-photon levels. A phase shift of 0.005 rad of a probe pulse modulated by a signal pulse with an energy of similar to 100 aJ, equivalent to similar to 400 photons, was observed in a four-level system of cold (87)Rb atoms.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000290105800004</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 757RQTimes Cited: 1Cited Reference Count: 24Cited References:      Pritchard JD, 2010, PHYS REV LETT, V105     Lo HY, 2010, OPT EXPRESS, V18, P18498     Mucke M, 2010, NATURE, V465, P755     Lo HY, 2010, PHYS REV A, V81     Gea-Banacloche J, 2010, PHYS REV A, V81     Zhu YF, 2010, OPT LETT, V35, P303     Lin YW, 2009, PHYS REV LETT, V102     Bajcsy M, 2009, PHYS REV LETT, V102     Siddons P, 2009, NAT PHOTONICS, V3, P225     Matsuda N, 2009, NAT PHOTONICS, V3, P95     Fushman I, 2008, SCIENCE, V320, P769, DOI 10.1126/science.1154643     Chen YF, 2006, PHYS REV LETT, V96, DOI 10.1103/PhysRevLett.96.043603     Chen YF, 2005, OPT LETT, V30, P3207, DOI 10.1364/OL.30.003207     Friedler I, 2005, PHYS REV A, V72, DOI 10.1103/PhysRevA.72.043803     Fleischhauer M, 2005, REV MOD PHYS, V77, P633, DOI 10.1103/RevModPhys.77.633     Bajcsy M, 2003, NATURE, V426, P638, DOI 10.1038/nature02176     Kang HS, 2003, PHYS REV LETT, V91, DOI 10.1103/PhysRevLett.91.093601     Lukin MD, 2000, PHYS REV LETT, V84, P1419, DOI 10.1103/PhysRevLett.84.1419     Harris SE, 1999, PHYS REV LETT, V82, P4611, DOI 10.1103/PhysRevLett.82.4611     Hau LV, 1999, NATURE, V397, P594, DOI 10.1038/17561     Harris SE, 1997, PHYS TODAY, V50, P36, DOI 10.1063/1.881806     Schmidt H, 1996, OPT LETT, V21, P1936, DOI 10.1364/OL.21.001936     TURCHETTE QA, 1995, PHYS REV LETT, V75, P4710, DOI 10.1103/PhysRevLett.75.4710     KETTERLE W, 1993, PHYS REV LETT, V70, P2253, DOI 10.1103/PhysRevLett.70.2253Lo, Hsiang-Yu Chen, Yen-Chun Su, Po-Ching Chen, Hao-Chung Chen, Jun-Xian Chen, Ying-Cheng Yu, Ite A. Chen, Yong-FanNational Science Council of Taiwan[98-2628-M-006-002]We acknowledge Bing He for helpful discussions. This work was supported by the National Science Council of Taiwan under Grant No. 98-2628-M-006-002.AMER PHYSICAL SOCCOLLEGE PK&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">[Lo, HY|Chen, YC|Su, PC|Chen, HC|Chen, JX|Chen, YF] Natl Cheng Kung Univ, Dept Phys, Tainan 701, Taiwan. [Chen, YC] Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 106, Taiwan. [Yu, IA] Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan.Lo, HY (reprint author), Natl Cheng Kung Univ, Dept Phys, Tainan 701, Taiwanyfchen@mail.ncku.edu.tw</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Tu, M. F.</style></author><author><style face="normal" font="default" size="100%">Ho, J. J.</style></author><author><style face="normal" font="default" size="100%">Hsieh, C. C.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Intense SrF radical beam for molecular cooling experiments</style></title><secondary-title><style face="normal" font="default" size="100%">Review of Scientific Instruments</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Rev. Sci. Instrum.</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">BAND</style></keyword><keyword><style  face="normal" font="default" size="100%">LASER</style></keyword><keyword><style  face="normal" font="default" size="100%">OPTICAL DOUBLE-RESONANCE</style></keyword><keyword><style  face="normal" font="default" size="100%">SPECTRUM</style></keyword><keyword><style  face="normal" font="default" size="100%">STATE</style></keyword><keyword><style  face="normal" font="default" size="100%">SYSTEM</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2009</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Nov</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000273061100012</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">11</style></number><volume><style face="normal" font="default" size="100%">80</style></volume><pages><style face="normal" font="default" size="100%">5</style></pages><isbn><style face="normal" font="default" size="100%">0034-6748</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We have developed a continuous SrF radical beam for the loading of helium buffer gas cooling. The SrF molecules are efficiently generated by high-temperature chemical reaction of the solid precursor SrF(2) with boron in a graphite oven. The beam properties are characterized with laser-induced fluorescence spectroscopic method. We obtain a molecular flux of up to 2.1 x 10(15) sr(-1) s(-1) at the detection region for all rotational states. The dependence of the flux on oven temperature suggests that even higher flux is possible if a higher temperature in the oven is achieved. (C) 2009 American Institute of Physics. [doi:10.1063/1.3262631]&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000273061100012</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 536RITimes Cited: 0Cited Reference Count: 35Cited References:      Carr LD, 2009, NEW J PHYS, V11     Patterson D, 2009, NEW J PHYS, V11     Wall TE, 2008, PHYS REV A, V78     Narevicius E, 2008, PHYS REV LETT, V100     Hogan SD, 2007, PHYS REV A, V76, DOI 10.1103/PhysRevA.76.023412     Patterson D, 2007, J CHEM PHYS, V126     Kohler T, 2006, REV MOD PHYS, V78, P1311, DOI 10.1103/RevModPhys.78.1311     Rabl P, 2006, PHYS REV LETT, V97, DOI 10.1103/PhysRevLett.97.033003     Fulton R, 2006, NAT PHYS, V2, P465, DOI 10.1038/nphys339     Chen L, 2006, J CHEM PHYS, V124, DOI 10.1063/1.2139092     Maxwell SE, 2005, PHYS REV LETT, V95, DOI 10.1103/PhysRevLett.95.173201     Hornkohl JO, 2005, APPL OPTICS, V44, P3686, DOI 10.1364/AO.44.003686     Di Rosa MD, 2004, EUR PHYS J D, V31, P395     Egorov D, 2004, EUR PHYS J D, V31, P307, DOI 10.1140/epjd/e2004-00140-1     Blinov BB, 2004, NATURE, V428, P153, DOI 10.1038/nature02377     KERMAN J, 2004, PHYS REV LETT, V92     Elioff MS, 2003, SCIENCE, V302, P1940, DOI 10.1126/science.1090679     Rangwala SA, 2003, PHYS REV A, V67, DOI 10.1103/PhysRevA.67.043406     BROWN J, 2003, ROTATIONAL SPECTROSC     Gupta M, 2001, J PHYS CHEM A, V105, P1626, DOI 10.1021/jp002640u     Rugamas F, 2000, MEAS SCI TECHNOL, V11, P1750, DOI 10.1088/0957-0233/11/12/315     Bethlem HL, 1999, PHYS REV LETT, V83, P1558, DOI 10.1103/PhysRevLett.83.1558     Teule JM, 1998, J PHYS CHEM A, V102, P9482, DOI 10.1021/jp981993e     Weinstein JD, 1998, NATURE, V395, P148     Colarusso P, 1996, J MOL SPECTROSC, V175, P158, DOI 10.1006/jmsp.1996.0019     KEIJZER F, 1995, J MOL SPECTROSC, V169, P511, DOI 10.1006/jmsp.1995.1043     STEIMLE TC, 1993, J MOL SPECTROSC, V158, P487, DOI 10.1006/jmsp.1993.1094     KANDLER J, 1989, CHEM PHYS LETT, V155, P470, DOI 10.1016/0009-2614(89)87188-X     ERNST WE, 1985, CHEM PHYS LETT, V113, P351, DOI 10.1016/0009-2614(85)80379-1     CHILDS WJ, 1981, J MOL SPECTROSC, V87, P522, DOI 10.1016/0022-2852(81)90422-7     DOMAILLE PJ, 1977, J MOL SPECTROSC, V68, P146, DOI 10.1016/0022-2852(77)90430-1     STEIMLE TC, 1977, J MOL SPECTROSC, V68, P134, DOI 10.1016/0022-2852(77)90429-5     DAGDIGIA.PJ, 1974, J CHEM PHYS, V60, P2330, DOI 10.1063/1.1681366     HILDENBR.DL, 1968, J CHEM PHYS, V48, P3657, DOI 10.1063/1.1669666     TU MF, UNPUBTu, Ming-Feng Ho, Jia-Jung Hsieh, Chih-Chiang Chen, Ying-ChengNSC[96-2112-M-001-006, 97-2628-M-001-028]This work is supported by the National Science Council of Taiwan under NSC Grant Nos. 96-2112-M-001-006 and 97-2628-M-001-028.AMER INST PHYSICSMELVILLE&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">[Tu, MF|Ho, JJ|Hsieh, CC|Chen, YC] Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 10617, Taiwan.Tu, MF (reprint author), Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 10617, Taiwanchenyc@pub.iams.sinica.edu.tw</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Lin, Y. W.</style></author><author><style face="normal" font="default" size="100%">Chou, H. C.</style></author><author><style face="normal" font="default" size="100%">Dwivedi, P. P.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Using a pair of rectangular coils in the MOT for the production of cold atom clouds with large optical density</style></title><secondary-title><style face="normal" font="default" size="100%">Optics Express</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Opt. Express</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">2-DIMENSIONAL MAGNETOOPTICAL TRAP</style></keyword><keyword><style  face="normal" font="default" size="100%">ATOMS</style></keyword><keyword><style  face="normal" font="default" size="100%">BOSE-EINSTEIN CONDENSATION</style></keyword><keyword><style  face="normal" font="default" size="100%">CESIUM</style></keyword><keyword><style  face="normal" font="default" size="100%">CONTINUOUS BEAM</style></keyword><keyword><style  face="normal" font="default" size="100%">GAS</style></keyword><keyword><style  face="normal" font="default" size="100%">light</style></keyword><keyword><style  face="normal" font="default" size="100%">SLOW</style></keyword><keyword><style  face="normal" font="default" size="100%">SODIUM ATOMS</style></keyword><keyword><style  face="normal" font="default" size="100%">STORAGE</style></keyword><keyword><style  face="normal" font="default" size="100%">vapor</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2008</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Mar</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000254121400030</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">6</style></number><volume><style face="normal" font="default" size="100%">16</style></volume><pages><style face="normal" font="default" size="100%">3753-3761</style></pages><isbn><style face="normal" font="default" size="100%">1094-4087</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We demonstrate a simple method to increase the optical density (OD) of cold atom clouds produced by a magneto-optical trap (MOT). A pair of rectangular anti-Helmholtz coils is used in the MOT to generate the magnetic field that produces the cigar-shaped atom cloud. With 7.2 x 10(8) Rb-87 atoms in the cigar-type MOT, we achieve an OD of 32 as determined by the slow light measurement and this OD is large enough such that the atom cloud can almost contain the entire Gaussian light pulse. Compared to the conventional MOT under the same trapping conditions, the OD is increased by about 2.7 folds by this simple method. In another MOT setup of the cigar-shaped Cs atom cloud, we achieve an OD of 105 as determined by the absorption spectrum of the |6S(1/2), F = 4 &amp;gt; -&amp;gt;| 6P(3/2), F ' = 5 &amp;gt; transition. (C) 2008 Optical Society of America&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000254121400030</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 276DLTimes Cited: 11Cited Reference Count: 39Cited References:      Cho HW, 2007, OPT EXPRESS, V15, P12114, DOI 10.1364/OE.15.012114     Guan PC, 2007, PHYS REV A, V76, DOI 10.1103/PhysRevA.76.033817     Gomez E, 2007, PHYS REV A, V75, DOI 10.1103/PhysRevA.75.033418     Chen YF, 2006, PHYS REV A, V74, DOI 10.1103/PhysRevA.74.063807     Chaudhuri S, 2006, PHYS REV A, V74, DOI 10.1103/PhysRevA.74.023406     Castagna N, 2006, EUR PHYS J-APPL PHYS, V34, P21, DOI 10.1051/epjap:2006037     Ramirez-Serrano J, 2006, OPT LETT, V31, P682, DOI 10.1364/OL.31.000682     Chen YF, 2006, PHYS REV LETT, V96, DOI 10.1103/PhysRevLett.96.043603     Chen YF, 2005, OPT LETT, V30, P3207, DOI 10.1364/OL.30.003207     Overstreet KR, 2005, OPT EXPRESS, V13, P9672, DOI 10.1364/OPEX.13.009672     Chen YF, 2005, PHYS REV A, V72, DOI 10.1103/PhysRevA.72.053803     Bartenstein M, 2005, PHYS REV LETT, V94, DOI 10.1103/PhysRevLett.94.103201     Oates CW, 2005, PHYS REV A, V71     Braje DA, 2004, PHYS REV LETT, V93, DOI 10.1103/PhysRevLett.93.183601     Kang HS, 2004, PHYS REV LETT, V93, DOI 10.1103/PhysRevLett.93.073601     Vengalattore M, 2004, PHYS REV LETT, V92     Sanguinetti S, 2003, EUR PHYS J D, V25, P3, DOI 10.1140/epjd/e2003-00215-5     Schoser J, 2002, PHYS REV A, V66     Cren P, 2002, EUR PHYS J D, V20, P107, DOI 10.1140/epjd/e2002-00106-3     Chen YC, 2001, PHYS REV A, V64     Phillips DF, 2001, PHYS REV LETT, V86, P783, DOI 10.1103/PhysRevLett.86.783     Liu C, 2001, NATURE, V409, P490, DOI 10.1038/35054017     Sortais Y, 2000, PHYS REV LETT, V85, P3117, DOI 10.1103/PhysRevLett.85.3117     Fleischhauer M, 2000, PHYS REV LETT, V84, P5094, DOI 10.1103/PhysRevLett.84.5094     Hau LV, 1999, NATURE, V397, P594, DOI 10.1038/17561     METCALF HJ, 1999, LASER COOLING TRAPPI     Dieckmann K, 1998, PHYS REV A, V58, P3891, DOI 10.1103/PhysRevA.58.3891     Berthoud P, 1998, EUROPHYS LETT, V41, P141, DOI 10.1209/epl/i1998-00122-9     Weyers S, 1997, OPT COMMUN, V143, P30, DOI 10.1016/S0030-4018(97)00312-X     DAVIS KB, 1995, PHYS REV LETT, V75, P3969, DOI 10.1103/PhysRevLett.75.3969     ANDERSON MH, 1995, SCIENCE, V269, P198, DOI 10.1126/science.269.5221.198     ADAMS CS, 1994, PHYS REP, V240, P143, DOI 10.1016/0370-1573(94)90066-3     KASEVICH M, 1992, APPL PHYS B-PHOTO, V54, P321, DOI 10.1007/BF00325375     MONROE C, 1990, PHYS REV LETT, V65, P1571, DOI 10.1103/PhysRevLett.65.1571     RIIS E, 1990, PHYS REV LETT, V64, P1658, DOI 10.1103/PhysRevLett.64.1658     WALKER T, 1990, PHYS REV LETT, V64, P408, DOI 10.1103/PhysRevLett.64.408     RAAB EL, 1987, PHYS REV LETT, V59, P2631, DOI 10.1103/PhysRevLett.59.2631     STECK DA, CESIUM D LINE DATA     STECK DA, RUBIDIUM 87 D LINE DLin, Yen-Wei Chou, Hung-Chih Dwivedi, Prashant P. Chen, Ying-Cheng Yu, Ite A.OPTICAL SOC AMERWASHINGTON&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">[Lin, YW|Chou, HC|Yu, IA] Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan. [Dwivedi, PP|Chen, YC] Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 106, Taiwan.Lin, YW (reprint author), Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwanyu@phys.nthu.edu.tw</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Laha, S.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Gupta, P.</style></author><author><style face="normal" font="default" size="100%">Simien, C. E.</style></author><author><style face="normal" font="default" size="100%">Martinez, Y. N.</style></author><author><style face="normal" font="default" size="100%">Mickelson, P. G.</style></author><author><style face="normal" font="default" size="100%">Nagel, S. B.</style></author><author><style face="normal" font="default" size="100%">Killian, T. C.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Kinetic energy oscillations in annular regions of ultracold neutral plasmas</style></title><secondary-title><style face="normal" font="default" size="100%">European Physical Journal D</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Eur. Phys. J. D</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">DYNAMICS</style></keyword><keyword><style  face="normal" font="default" size="100%">EXPANSION</style></keyword><keyword><style  face="normal" font="default" size="100%">ONE-COMPONENT PLASMA</style></keyword><keyword><style  face="normal" font="default" size="100%">relaxation</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2006</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Oct</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000240475100008</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">1</style></number><volume><style face="normal" font="default" size="100%">40</style></volume><pages><style face="normal" font="default" size="100%">51-56</style></pages><isbn><style face="normal" font="default" size="100%">1434-6060</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;A study of ion equilibration in annular regions of ultracold strontium plasmas is reported. Plasmas are formed by photoionizing laser-cooled atoms with a pulsed dye laser. The experimental probe is spatially-resolved absorption spectroscopy using the S-2(1/2)-P-2(1/2) transition of the Sr+ ion. The kinetic energy of the ions is calculated from the Doppler broadening of the spectrum, and it displays clear oscillations during the first microsecond after plasma formation. The oscillations, which are a characteristic of strong coulomb coupling, are fit with a simple phenomenological model incorporating damping and density variation in the plasma.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article; Proceedings Paper</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000240475100008</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 083RETimes Cited: 7Cited Reference Count: 23Cited References:      Cummings EA, 2005, PHYS REV LETT, V95, DOI 10.1103/PhysRevLett.95.235001     Cummings EA, 2005, PHYS PLASMAS, V12, DOI 10.1063/1.2140683     KILLIAN TC, 2005, J PHYS B ATOM MOL PH, V38, P351     LAHA S, 2005, THESIS RICE U     POHL T, 2005, J PHYS CONF SER, V11, P223, DOI 10.1088/1742-6596/11/1/022     Chen YC, 2004, PHYS REV LETT, V93, DOI 10.1103/PhysRevLett.93.265003     Pohl T, 2004, PHYS REV LETT, V92, DOI 10.1103/PhysRevLett.92.155003     Simien CE, 2004, PHYS REV LETT, V92, DOI 10.1103/PhysRevLett.92.143001     POHL T, 2004, J PHYS B ATOM MOL PH, V37, P183     Morozov IV, 2003, J PHYS A-MATH GEN, V36, P6005, DOI 10.1088/0305-4470/36/22/323     Robicheaux F, 2003, PHYS PLASMAS, V10, P2217, DOI 10.1063/1.1573213     NAGEL SB, 2003, PHYS REV A, V67, P11401     Kuzmin SG, 2002, PHYS PLASMAS, V9, P3743, DOI 10.1063/1.1497166     MAZEVET S, 2002, PHYS REV LETT, V88, P55001     Murillo MS, 2001, PHYS REV LETT, V87, part. no., DOI 10.1103/PhysRevLett.87.115003     Kulin S, 2000, PHYS REV LETT, V85, P318, DOI 10.1103/PhysRevLett.85.318     Killian TC, 1999, PHYS REV LETT, V83, P4776, DOI 10.1103/PhysRevLett.83.4776     Zwicknagel G, 1999, CONTRIB PLASM PHYS, V39, P155, DOI 10.1002/ctpp.2150390138     Hamaguchi S, 1997, PHYS REV E, V56, P4671, DOI 10.1103/PhysRevE.56.4671     SIEGMAN AE, 1986, LASERS     JONES WD, 1985, INTRO LINEAR THEORIE, P63501     GOULD H, 1975, PHYS REV LETT, V35, P1455, DOI 10.1103/PhysRevLett.35.1455     HANSEN JP, 1974, PHYS REV LETT, V32, P277, DOI 10.1103/PhysRevLett.32.277Laha, S. Chen, Y. C. Gupta, P. Simien, C. E. Martinez, Y. N. Mickelson, P. G. Nagel, S. B. Killian, T. C.International Workshop on Ultracold Plasma and Rydberg Systems (Ultracold PARYS)FEB 14-MAR 16, 2005Gif sur Yvette, FRANCESPRINGERNEW YORK&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">Rice Univ, Dept Phys &amp; Astron, Houston, TX 77005 USA. Rice Univ, Rice Quantum Inst, Houston, TX 77005 USA. Acad Sinica, Inst Atom &amp; Mol Sci, Taipei 106, Taiwan.Laha, S (reprint author), Rice Univ, Dept Phys &amp; Astron, Houston, TX 77005 USAsampad@rice.edu</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Mickelson, P. G.</style></author><author><style face="normal" font="default" size="100%">Martinez, Y. N.</style></author><author><style face="normal" font="default" size="100%">Saenz, A. D.</style></author><author><style face="normal" font="default" size="100%">Nagel, S. B.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Killian, T. C.</style></author><author><style face="normal" font="default" size="100%">Pellegrini, P.</style></author><author><style face="normal" font="default" size="100%">Cote, R.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Spectroscopic determination of the s-wave scattering lengths of Sr-86 and Sr-88</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review Letters</style></secondary-title><short-title><style face="normal" font="default" size="100%">Spectroscopic determination of the s-wave scattering lengths of Sr-86 and Sr-88</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2005</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Nov 25</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000233458500018</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">95</style></volume><isbn><style face="normal" font="default" size="100%">0031-9007</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We report the use of photoassociative spectroscopy to determine the ground-state s-wave scattering lengths for the main bosonic isotopes of strontium, Sr-86 and Sr-88. Photoassociative transitions are driven with a laser red detuned by up to 1400 GHz from the S-1(0)-P-1(1) atomic resonance at 461 nm. A minimum in the transition amplitude for Sr-86 at -494 +/- 5 GHz allows us to determine the scattering lengths 610a(0)&amp;lt; a(86)&amp;lt; 2300a(0) for Sr-86 and a much smaller value of -1a(0)&amp;lt; a(88)&amp;lt; 13a(0) for Sr-88.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000233458500018</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 30&lt;/p&gt;
</style></notes><custom7><style face="normal" font="default" size="100%">223002</style></custom7></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Killian, T. C.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Gupta, P.</style></author><author><style face="normal" font="default" size="100%">Laha, S.</style></author><author><style face="normal" font="default" size="100%">Martinez, Y. N.</style></author><author><style face="normal" font="default" size="100%">Mickelson, P. G.</style></author><author><style face="normal" font="default" size="100%">Nagel, S. B.</style></author><author><style face="normal" font="default" size="100%">Saenz, A. D.</style></author><author><style face="normal" font="default" size="100%">Simien, C. E.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Ultracold neutral plasmas</style></title><secondary-title><style face="normal" font="default" size="100%">Plasma Physics and Controlled Fusion</style></secondary-title><short-title><style face="normal" font="default" size="100%">Ultracold neutral plasmas</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2005</style></year><pub-dates><date><style  face="normal" font="default" size="100%">May</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000229591100022</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">47</style></volume><pages><style face="normal" font="default" size="100%">A297-A306</style></pages><isbn><style face="normal" font="default" size="100%">0741-3335</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;Ultracold neutral plasmas are formed by photo-ionizing laser-cooled atoms near the ionization threshold. Through the application of atomic physics techniques and diagnostics, these experiments stretch the boundaries of traditional neutral plasma physics. The electron temperature in these plasmas ranges from 1 to 1000 K and the ion temperature is around 1 K. The density can approach 10(11) cm(-3). Fundamental interest stems from the possibility of creating strongly coupled plasmas, but recombination, collective modes, and thermalization in these systems have also been studied. Optical absorption images of a strontium plasma, using the Sr+ S-2(1/2) -&amp;gt; P-2(1/2) transition at 422 mn, depict the density profile of the plasma, and probe kinetics on a 50 ns time-scale. The Doppler-broadened ion absorption spectrum measures the ion velocity distribution, which gives an accurate measure of the ion dynamics in the first microsecond after photo-ionization.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000229591100022</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 2 Si 5a 12th International Congress on Plasma Physics (ICPP2004) Oct 25-29, 2004 Nice, FRANCE Int Advisory Comm&lt;/p&gt;
</style></notes></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Nagel, S. B.</style></author><author><style face="normal" font="default" size="100%">Mickelson, P. G.</style></author><author><style face="normal" font="default" size="100%">Saenz, A. D.</style></author><author><style face="normal" font="default" size="100%">Martinez, Y. N.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Killian, T. C.</style></author><author><style face="normal" font="default" size="100%">Pellegrini, P.</style></author><author><style face="normal" font="default" size="100%">Cote, R.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Photoassociative spectroscopy at long range in ultracold strontium</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review Letters</style></secondary-title><short-title><style face="normal" font="default" size="100%">Photoassociative spectroscopy at long range in ultracold strontium</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2005</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Mar 4</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000227386000023</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">94</style></volume><isbn><style face="normal" font="default" size="100%">0031-9007</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We report photoassociative spectroscopy of Sr-88(2) in a magneto-optical trap operating on the S-1(0)--&amp;gt;P-3(1) intercombination line at 689 nm. Photoassociative transitions are driven with a laser red detuned by 600-2400 MHz from the S-1(0)--&amp;gt;P-1(1) atomic resonance at 461 nm. Photoassociation takes place at extremely large internuclear separation, and the photoassociative spectrum is strongly affected by relativistic retardation. A fit of the transition frequencies determines the P-1(1) atomic lifetime (tau=5.22+/-0.03 ns) and resolves a discrepancy between experiment and recent theoretical calculations.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000227386000023</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 30&lt;/p&gt;
</style></notes><custom7><style face="normal" font="default" size="100%">083004</style></custom7></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Killian, T. C.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Gupta, P.</style></author><author><style face="normal" font="default" size="100%">Laha, S.</style></author><author><style face="normal" font="default" size="100%">Martinez, Y. N.</style></author><author><style face="normal" font="default" size="100%">Mickelson, P. G.</style></author><author><style face="normal" font="default" size="100%">Nagel, S. B.</style></author><author><style face="normal" font="default" size="100%">Saenz, A. D.</style></author><author><style face="normal" font="default" size="100%">Simien, C. E.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Absorption imaging and spectroscopy of ultracold neutral plasmas</style></title><secondary-title><style face="normal" font="default" size="100%">Journal of Physics B-Atomic Molecular and Optical Physics</style></secondary-title><short-title><style face="normal" font="default" size="100%">Absorption imaging and spectroscopy of ultracold neutral plasmas</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2005</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Jan 28</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000227154000027</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">38</style></volume><pages><style face="normal" font="default" size="100%">S351-S362</style></pages><isbn><style face="normal" font="default" size="100%">0953-4075</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;Absorption imaging and spectroscopy can probe the dynamics of an ultracold neutral plasma during the first few microseconds after its creation. Quantitative analysis of the data, however, is complicated by the inhomogeneous density distribution, expansion of the plasma and possible lack of global thermal equilibrium for the ions. In this paper, we describe methods for addressing these issues. Using simple assumptions about the underlying temperature distribution and ion motion, the Doppler-broadened absorption spectrum obtained from plasma images can be related to the average temperature in the plasma.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000227154000027</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 2 Si International Workshop and Seminar on Rydberg Physics Apr 19-may 14, 2004 Max Planck Inst Physik Komplexer Sys, Dresden, GERMANY&lt;/p&gt;
</style></notes></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Simien, C. E.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Gupta, P.</style></author><author><style face="normal" font="default" size="100%">Laha, S.</style></author><author><style face="normal" font="default" size="100%">Martinez, Y. N.</style></author><author><style face="normal" font="default" size="100%">Mickelson, P. G.</style></author><author><style face="normal" font="default" size="100%">Nagel, S. B.</style></author><author><style face="normal" font="default" size="100%">Killian, T. C.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Absorption imaging of ultracold neutral plasmas</style></title><secondary-title><style face="normal" font="default" size="100%">Ieee Transactions on Plasma Science</style></secondary-title><short-title><style face="normal" font="default" size="100%">Absorption imaging of ultracold neutral plasmas</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2005</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Apr</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000228407100159</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">33</style></volume><pages><style face="normal" font="default" size="100%">540-541</style></pages><isbn><style face="normal" font="default" size="100%">0093-3813</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We report optical absorption imaging of ultracold neutral plasmas. Imaging allows direct observation of the ion density profile and expansion of the plasma. The frequency dependence of the plasma's optical depth gives the ion absorption spectrum, which is broadened by the ion motion. We use the spectral width to monitor ion equilibration in the first 250 ns after plasma formation. On a microsecond time scale, we observe the radial acceleration of ions resulting from pressure exerted by the trapped electron gas.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000228407100159</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 0 Part 1&lt;/p&gt;
</style></notes></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Simien, C. E.</style></author><author><style face="normal" font="default" size="100%">Laha, S.</style></author><author><style face="normal" font="default" size="100%">Gupta, P.</style></author><author><style face="normal" font="default" size="100%">Martinez, Y. N.</style></author><author><style face="normal" font="default" size="100%">Mickelson, P. G.</style></author><author><style face="normal" font="default" size="100%">Nagel, S. B.</style></author><author><style face="normal" font="default" size="100%">Killian, T. C.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Electron screening and kinetic-energy oscillations in a strongly coupled plasma</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review Letters</style></secondary-title><short-title><style face="normal" font="default" size="100%">Electron screening and kinetic-energy oscillations in a strongly coupled plasma</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2004</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Dec 31</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000226054600032</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">93</style></volume><isbn><style face="normal" font="default" size="100%">0031-9007</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We study equilibration of strongly coupled ions in an ultracold neutral plasma produced by photoionizing laser-cooled and trapped atoms. By varying the electron temperature, we show that electron screening modifies the equilibrium ion temperature. Even with few electrons in a Debye sphere, the screening is well described by a model using a Yukawa ion-ion potential. We also observe damped oscillations of the ion kinetic energy that are a unique feature of equilibration of a strongly coupled plasma.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000226054600032</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 51&lt;/p&gt;
</style></notes><custom7><style face="normal" font="default" size="100%">265003</style></custom7></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Simien, C. E.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Gupta, P.</style></author><author><style face="normal" font="default" size="100%">Laha, S.</style></author><author><style face="normal" font="default" size="100%">Martinez, Y. N.</style></author><author><style face="normal" font="default" size="100%">Mickelson, P. G.</style></author><author><style face="normal" font="default" size="100%">Nagel, S. B.</style></author><author><style face="normal" font="default" size="100%">Killian, T. C.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Using absorption imaging to study ion dynamics in an ultracold neutral plasma</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review Letters</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Phys. Rev. Lett.</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">COLD</style></keyword><keyword><style  face="normal" font="default" size="100%">EXPANSION</style></keyword><keyword><style  face="normal" font="default" size="100%">LIQUIDS</style></keyword><keyword><style  face="normal" font="default" size="100%">RYDBERG ATOMS</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2004</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Apr</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000221037500015</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">14</style></number><volume><style face="normal" font="default" size="100%">92</style></volume><pages><style face="normal" font="default" size="100%">4</style></pages><isbn><style face="normal" font="default" size="100%">0031-9007</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We report optical absorption imaging of ultracold neutral strontium plasmas. The ion absorption spectrum determined from the images is Doppler broadened and thus provides a quantitative measure of the ion kinetic energy. For the particular plasma conditions studied, ions heat rapidly as they equilibrate during the first 250 ns after plasma formation. Equilibration leaves ions on the border between the weakly coupled gaseous and strongly coupled liquid states. On a longer time scale of microseconds, pressure exerted by the trapped electron gas accelerates the ions radially.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000221037500015</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 815JBTimes Cited: 63Cited Reference Count: 22Cited References:      Killian TC, 2003, J PHYS A-MATH GEN, V36, P6077, DOI 10.1088/0305-4470/36/22/333     Robicheaux F, 2003, PHYS PLASMAS, V10, P2217, DOI 10.1063/1.1573213     Nagel SB, 2003, PHYS REV A, V67, DOI 10.1103/PhysRevA.67.011401     Gabrielse G, 2002, PHYS REV LETT, V89     Amoretti M, 2002, NATURE, V419, P456, DOI 10.1038/nature01096     Mazevet S, 2002, PHYS REV LETT, V88, DOI 10.1103/PhysRevLett.88.055001     KLUZMIN SG, 2002, PHYS PLASMAS, V9, P3743     Murillo MS, 2001, PHYS REV LETT, V87, part. no., DOI 10.1103/PhysRevLett.87.115003     Killian TC, 2001, PHYS REV LETT, V86, P3759, DOI 10.1103/PhysRevLett.86.3759     Levinton FM, 2001, REV SCI INSTRUM, V72, P898, DOI 10.1063/1.1321005     Tkachev AN, 2000, QUANTUM ELECTRON+, V30, P1077, DOI 10.1070/QE2000v030n12ABEH001869     Robinson MP, 2000, PHYS REV LETT, V85, P4466, DOI 10.1103/PhysRevLett.85.4466     Murillo MS, 2000, PHYS REV LETT, V85, P2514, DOI 10.1103/PhysRevLett.85.2514     Kulin S, 2000, PHYS REV LETT, V85, P318, DOI 10.1103/PhysRevLett.85.318     Killian TC, 1999, PHYS REV LETT, V83, P4776, DOI 10.1103/PhysRevLett.83.4776     Mitchell TB, 1999, PHYS PLASMAS, V6, P1751, DOI 10.1063/1.873433     Dubin DHE, 1999, REV MOD PHYS, V71, P87, DOI 10.1103/RevModPhys.71.87     METCALF HJ, 1999, LASER COOLING TRAPPI     FAROUKI RT, 1994, J CHEM PHYS, V101, P9885, DOI 10.1063/1.467955     ICHIMARU S, 1982, REV MOD PHYS, V54, P1017, DOI 10.1103/RevModPhys.54.1017     GRIEM HR, 1974, SPECTRAL LINE BROADE     GREENE C, COMMUNICATIONSimien, CE Chen, YC Gupta, P Laha, S Martinez, YN Mickelson, PG Nagel, SB Killian, TCAMERICAN PHYSICAL SOCCOLLEGE PK&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">Rice Univ, Dept Phys &amp; Astron, Houston, TX 77251 USA. Rice Univ, Rice Quantum Inst, Houston, TX 77251 USA.Simien, CE (reprint author), Rice Univ, Dept Phys &amp; Astron, Houston, TX 77251 USA</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Y.W. Chen</style></author><author><style face="normal" font="default" size="100%">Lin, C. W.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Quantization axes in coherent two-field spectroscopy</style></title><secondary-title><style face="normal" font="default" size="100%">Journal of the Optical Society of America B-Optical Physics</style></secondary-title><alt-title><style face="normal" font="default" size="100%">J. Opt. Soc. Am. B-Opt. Phys.</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">ATOMS</style></keyword><keyword><style  face="normal" font="default" size="100%">CESIUM</style></keyword><keyword><style  face="normal" font="default" size="100%">electromagnetically induced transparency</style></keyword><keyword><style  face="normal" font="default" size="100%">INTERACTING DARK RESONANCES</style></keyword><keyword><style  face="normal" font="default" size="100%">INTERFERENCE</style></keyword><keyword><style  face="normal" font="default" size="100%">LASER</style></keyword><keyword><style  face="normal" font="default" size="100%">POPULATION-INVERSION</style></keyword><keyword><style  face="normal" font="default" size="100%">STATES</style></keyword><keyword><style  face="normal" font="default" size="100%">STORAGE</style></keyword><keyword><style  face="normal" font="default" size="100%">vapor</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2002</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Aug</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000177430100024</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">8</style></number><volume><style face="normal" font="default" size="100%">19</style></volume><pages><style face="normal" font="default" size="100%">1917-1921</style></pages><isbn><style face="normal" font="default" size="100%">0740-3224</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;Coherent two-field spectroscopy calculations with different choices of the quantization (z) axis are compared. In a system driven by a strong coupling field and a weak probe field, alignment of the z axis along either the polarization direction of a linearly polarized coupling field or the propagation direction of a circularly polarized coupling field is shown to simplify the calculations and facilitate interpretation of the results. The advantages of a suitable choice of the z axis are highlighted with an example of a degenerate three-level system of electromagnetically induced transparency. (C) 2002 Optical Society of America.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000177430100024</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 583VBTimes Cited: 0Cited Reference Count: 22Cited References:      Chen YC, 2001, PHYS REV A, V64, DOI 10.1103/PhysRevA.64.053806     Chen YC, 2001, PHYS REV A, V63     Phillips DF, 2001, PHYS REV LETT, V86, P783, DOI 10.1103/PhysRevLett.86.783     Liu C, 2001, NATURE, V409, P490, DOI 10.1038/35054017     McGloin D, 2000, PHYS REV A, V62, part. no., DOI 10.1103/PhysRevA.62.053802     Chen YC, 2000, PHYS REV A, V61, DOI 10.1103/PhysRevA.61.053805     Wang S, 2000, PHYS REV A, V61     Akulshin AM, 1999, PHYS REV LETT, V83, P4277, DOI 10.1103/PhysRevLett.83.4277     Lukin MD, 1999, PHYS REV A, V60, P3225, DOI 10.1103/PhysRevA.60.3225     Taichenachev AV, 1999, JETP LETT+, V69, P819, DOI 10.1134/1.568096     Durrant AV, 1998, OPT COMMUN, V151, P136, DOI 10.1016/S0030-4018(98)00052-2     Marangos JP, 1998, J MOD OPTIC, V45, P471, DOI 10.1080/09500349808231909     Padmabandu GG, 1996, PHYS REV LETT, V76, P2053, DOI 10.1103/PhysRevLett.76.2053     Arimondo E, 1996, PROG OPTICS, V35, P257, DOI 10.1016/S0079-6638(08)70531-6     LI YQ, 1995, PHYS REV A, V51, pR2703     COURTOIS JY, 1994, PHYS REV LETT, V72, P3017, DOI 10.1103/PhysRevLett.72.3017     BOLLER KJ, 1991, PHYS REV LETT, V66, P2593, DOI 10.1103/PhysRevLett.66.2593     GRISON D, 1991, EUROPHYS LETT, V15, P149, DOI 10.1209/0295-5075/15/2/007     IMAMOGLU A, 1989, OPT LETT, V14, P1344, DOI 10.1364/OL.14.001344     KOCHAROVSKAYA OA, 1988, JETP LETT+, V48, P630     ASPECT A, 1988, PHYS REV LETT, V61, P826, DOI 10.1103/PhysRevLett.61.826     GRAY HR, 1978, OPT LETT, V3, P218, DOI 10.1364/OL.3.000218Chen, YW Lin, CW Chen, YC Yu, IAOPTICAL SOC AMERWASHINGTON&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan.Chen, YW (reprint author), Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Liao, Y. A.</style></author><author><style face="normal" font="default" size="100%">Hsu, L.</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Simple technique for directly and accurately measuring the number of atoms in a magneto-optical trap</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review A</style></secondary-title><short-title><style face="normal" font="default" size="100%">Simple technique for directly and accurately measuring the number of atoms in a magneto-optical trap</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">2001</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Sep</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000170978600005</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">64</style></volume><isbn><style face="normal" font="default" size="100%">1050-2947</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We have systematically studied a simple technique that accurately determines number of atoms in a magneto-optical trap, Absorption energy of a laser field that interacts with cold atoms is a direct measurement of atom number. The measured energy neither depends on the detuning, intensity, and polarization of the laser field nor is affected by other system parameters. Our work also demonstrates that such technique can be applied to study the phenomenon of coherent population trapping.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:000170978600005</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 12&lt;/p&gt;
</style></notes><custom7><style face="normal" font="default" size="100%">031401</style></custom7></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Liao, Y. A.</style></author><author><style face="normal" font="default" size="100%">Chiu, H. Y.</style></author><author><style face="normal" font="default" size="100%">Su, J. J.</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Observation of the quantum interference phenomenon induced by interacting dark resonances</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review A</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Phys. Rev. A</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">ATOMS</style></keyword><keyword><style  face="normal" font="default" size="100%">INVERSION</style></keyword><keyword><style  face="normal" font="default" size="100%">light</style></keyword><keyword><style  face="normal" font="default" size="100%">vapor</style></keyword><keyword><style  face="normal" font="default" size="100%">VELOCITY</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2001</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Nov</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000172074200090</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">5</style></number><volume><style face="normal" font="default" size="100%">64</style></volume><pages><style face="normal" font="default" size="100%">5</style></pages><isbn><style face="normal" font="default" size="100%">1050-2947</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We report an experimental observation of narrow and high-contrast spectra. which are induced by interacting dark resonances and have been predicted in Phys. Rev. A 60, 3225 (1999). Spectra are measured with cold (87)Rb atoms produced by a magneto-optical trap. In this experimental system, a coupling laser and a weak probe laser form a three-level Lambda -type configuration of electromagnetically induced transparency (EIT); a microwave drives a magnetic-dipole transition between the fourth level and the ground state that is coupled with the excited state by the coupling laser. The observed spectral profile of probe absorption exhibits a very sharp peak emerging inside a narrow EIT dip. Such spectral feature provides more opportunities in manipulating atomic-optical response.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000172074200090</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 490VJTimes Cited: 53Cited Reference Count: 21Cited References:      Yan M, 2001, PHYS REV A, V64, DOI 10.1103/PhysRevA.64.013412     Chen YC, 2001, PHYS REV A, V63     Phillips DF, 2001, PHYS REV LETT, V86, P783, DOI 10.1103/PhysRevLett.86.783     Liu C, 2001, NATURE, V409, P490, DOI 10.1038/35054017     Lukin MD, 1999, PHYS REV A, V60, P3225, DOI 10.1103/PhysRevA.60.3225     Budker D, 1999, PHYS REV LETT, V83, P1767, DOI 10.1103/PhysRevLett.83.1767     Hau LV, 1999, NATURE, V397, P594, DOI 10.1038/17561     Harris SE, 1998, PHYS REV LETT, V81, P3611, DOI 10.1103/PhysRevLett.81.3611     KOCHAROVSKAYA OA, 1998, PISMA ESKP TEOR FIZ, V48, P581     Harris SE, 1997, PHYS TODAY, V50, P36, DOI 10.1063/1.881806     Padmabandu GG, 1996, PHYS REV LETT, V76, P2053, DOI 10.1103/PhysRevLett.76.2053     ARIMONDO E, 1996, PROGR OPTICS, V35, P258     BOLLER KJ, 1991, PHYS REV LETT, V66, P2539     MONROE C, 1990, PHYS REV LETT, V65, P1571, DOI 10.1103/PhysRevLett.65.1571     IMAMOGLU A, 1989, OPT LETT, V14, P1344, DOI 10.1364/OL.14.001344     ASPECT A, 1988, PHYS REV LETT, V61, P826, DOI 10.1103/PhysRevLett.61.826     RAAB EL, 1987, PHYS REV LETT, V59, P2631, DOI 10.1103/PhysRevLett.59.2631     DALTON BJ, 1982, J PHYS B-AT MOL OPT, V15, P3997, DOI 10.1088/0022-3700/15/21/019     GRAY HR, 1978, OPT LETT, V3, P218, DOI 10.1364/OL.3.000218     ALZETTA G, 1976, NUOVO CIMENTO B, V36, P5, DOI 10.1007/BF02749417     ARIMONDO E, 1976, LETT NUOVO CIMENTO, V17, P333, DOI 10.1007/BF02746514Chen, YC Liao, YA Chiu, HY Su, JJ Yu, IAAMER PHYSICAL SOCCOLLEGE PK&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan.Chen, YC (reprint author), Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Y.W. Chen</style></author><author><style face="normal" font="default" size="100%">Su, J. J.</style></author><author><style face="normal" font="default" size="100%">Huang, J. Y.</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Pump-probe spectroscopy of cold Rb-87 atoms in various polarization configurations</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review A</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Phys. Rev. A</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">2-PHOTON SPECTROSCOPY</style></keyword><keyword><style  face="normal" font="default" size="100%">ATOMS</style></keyword><keyword><style  face="normal" font="default" size="100%">BEAMS</style></keyword><keyword><style  face="normal" font="default" size="100%">CESIUM ATOMS</style></keyword><keyword><style  face="normal" font="default" size="100%">DIMENSIONAL OPTICAL MOLASSES</style></keyword><keyword><style  face="normal" font="default" size="100%">LASER</style></keyword><keyword><style  face="normal" font="default" size="100%">MAGNETOOPTICAL</style></keyword><keyword><style  face="normal" font="default" size="100%">NONLINEAR SPECTROSCOPY</style></keyword><keyword><style  face="normal" font="default" size="100%">RB</style></keyword><keyword><style  face="normal" font="default" size="100%">RECOIL-INDUCED RESONANCES</style></keyword><keyword><style  face="normal" font="default" size="100%">sodium</style></keyword><keyword><style  face="normal" font="default" size="100%">TRAP</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2001</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Apr</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000168095300114</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">4</style></number><volume><style face="normal" font="default" size="100%">63</style></volume><pages><style face="normal" font="default" size="100%">11</style></pages><isbn><style face="normal" font="default" size="100%">1050-2947</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We investigate systematically pump-probe spectroscopy of cold Rb-87 atoms produced by a magneto-optical trap. The pump-probe spectra are measured without the presence of the trapping beams or any optical molasses. Various polarization configurations of the probe and pump fields result in very different spectra of probe absorption. The observed spectra exhibit a dispersive profile, a dispersionlike profile, a Lorentzian profile, or a dispersive profile plus a Lorentzian profile. The widths of all the spectral profiles are narrower than the natural linewidth of the excited state. Our work clarifies the mechanisms behind these different spectral profiles and provides essential information for the pump-probe spectroscopy of cold atoms.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000168095300114</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 422AGTimes Cited: 21Cited Reference Count: 31Cited References:      Chen YC, 2000, PHYS REV A, V61, DOI 10.1103/PhysRevA.61.053805     di Stefano A, 1999, APPL PHYS B-LASERS O, V69, P263, DOI 10.1007/s003400050806     Lezama A, 1999, PHYS REV A, V59, P4732, DOI 10.1103/PhysRevA.59.4732     Sorensen JL, 1998, OPT LETT, V23, P25, DOI 10.1364/OL.23.000025     Snadden MJ, 1997, J OPT SOC AM B, V14, P544, DOI 10.1364/JOSAB.14.000544     Mitsunaga M, 1996, J OPT SOC AM B, V13, P2696, DOI 10.1364/JOSAB.13.002696     Guibal S, 1996, OPT COMMUN, V131, P61, DOI 10.1016/0030-4018(96)00268-4     Ye J, 1996, OPT LETT, V21, P1280, DOI 10.1364/OL.21.001280     Snadden MJ, 1996, OPT COMMUN, V125, P70, DOI 10.1016/0030-4018(95)00711-3     KUNZE S, 1996, LASER SPECTROSCOPY, P138     BERMAN PR, 1995, PHYS REV A, V51, P3947, DOI 10.1103/PhysRevA.51.3947     GEORGIADES NP, 1994, OPT LETT, V19, P1474, DOI 10.1364/OL.19.001474     MEACHER DR, 1994, PHYS REV A, V50, pR1992     COURTOIS JY, 1994, PHYS REV LETT, V72, P3017, DOI 10.1103/PhysRevLett.72.3017     GUO J, 1994, PHYS REV A, V49, P3934, DOI 10.1103/PhysRevA.49.3934     SINCLAIR AG, 1994, OPT COMMUN, V106, P207, DOI 10.1016/0030-4018(94)90323-9     FOX RW, 1993, OPT LETT, V18, P1456, DOI 10.1364/OL.18.001456     GUO J, 1993, PHYS REV A, V47, P4128, DOI 10.1103/PhysRevA.47.4128     COURTOIS JY, 1992, PHYS REV A, V46, P7060, DOI 10.1103/PhysRevA.46.7060     LOUNIS B, 1992, PHYS REV LETT, V69, P3029, DOI 10.1103/PhysRevLett.69.3029     GUO J, 1992, PHYS REV A, V46, P1426, DOI 10.1103/PhysRevA.46.1426     JESSEN PS, 1992, PHYS REV LETT, V69, P49, DOI 10.1103/PhysRevLett.69.49     VERKERK P, 1992, PHYS REV LETT, V68, P3861, DOI 10.1103/PhysRevLett.68.3861     VALLET M, 1992, OPT COMMUN, V87, P340, DOI 10.1016/0030-4018(92)90481-6     TABOSA JWR, 1991, PHYS REV LETT, V66, P3245, DOI 10.1103/PhysRevLett.66.3245     GRISON D, 1991, EUROPHYS LETT, V15, P149, DOI 10.1209/0295-5075/15/2/007     MONROE C, 1990, PHYS REV LETT, V65, P1571, DOI 10.1103/PhysRevLett.65.1571     GRYNBERG G, 1990, PHYS REV LETT, V65, P701, DOI 10.1103/PhysRevLett.65.701     RAAB EL, 1987, PHYS REV LETT, V59, P2631, DOI 10.1103/PhysRevLett.59.2631     DALTON BJ, 1982, J PHYS B-AT MOL OPT, V15, P3997, DOI 10.1088/0022-3700/15/21/019     COHENTANNOUDJI C, 1977, FRONTIER LASER SPECT, V1, P28Chen, YC Chen, YW Su, JJ Huang, JY Yu, IAAMERICAN PHYSICAL SOCCOLLEGE PK&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan.Chen, YC (reprint author), Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Lin, W. B.</style></author><author><style face="normal" font="default" size="100%">Hsue, H. C.</style></author><author><style face="normal" font="default" size="100%">Hsu, L.</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Effect of the trapping laser linewidth on the atom number in a magneto-optical trap</style></title><secondary-title><style face="normal" font="default" size="100%">Chinese Journal of Physics</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Chin. J. Phys.</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">VAPOR-CELL</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2000</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Oct</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000089864100004</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">5</style></number><volume><style face="normal" font="default" size="100%">38</style></volume><pages><style face="normal" font="default" size="100%">920-926</style></pages><isbn><style face="normal" font="default" size="100%">0577-9073</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We have experimentally studied the effect of the trapping laser linewidth on the number of capped atoms in a magneto-optical trap (MOT). Our data show that a significant number of the atoms can still be trapped in the MOT, even when the trapping laser linewidth is larger than the natural linewidth of the excited state of the driving transition.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000089864100004</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 363XZTimes Cited: 1Cited Reference Count: 10Cited References:      Chen YC, 2000, PHYS REV A, V61, DOI 10.1103/PhysRevA.61.053805     TUNG SK, 2000, J PHYS TAIPEI, V38, P395     Snadden MJ, 1997, OPT LETT, V22, P892, DOI 10.1364/OL.22.000892     Gabbanini C, 1997, EUROPHYS LETT, V37, P251, DOI 10.1209/epl/i1997-00139-0     Ye J, 1996, OPT LETT, V21, P1280, DOI 10.1364/OL.21.001280     TOWNSEND CG, 1995, PHYS REV A, V52, P1423, DOI 10.1103/PhysRevA.52.1423     LINDQUIST K, 1992, PHYS REV A, V46, P4082, DOI 10.1103/PhysRevA.46.4082     MONROE C, 1991, OPT LETT, V16, P50, DOI 10.1364/OL.16.000050     RAAB EL, 1987, PHYS REV LETT, V59, P2631, DOI 10.1103/PhysRevLett.59.2631     GOLDBERG L, 1983, ELECTRON LETT, V19, P491, DOI 10.1049/el:19830333Chen, YC Lin, WB Hsue, HC Hsu, L Yu, IAPHYSICAL SOC REPUBLIC CHINATAIPEI&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan. Natl Chiao Tung Univ, Dept Electrophys, Hsinchu 300, Taiwan.Chen, YC (reprint author), Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Lin, C. W.</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Role of degenerate Zeeman levels in electromagnetically induced transparency</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review A</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Phys. Rev. A</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">ABSORPTION</style></keyword><keyword><style  face="normal" font="default" size="100%">ATOMS</style></keyword><keyword><style  face="normal" font="default" size="100%">COLD</style></keyword><keyword><style  face="normal" font="default" size="100%">DISPERSION</style></keyword><keyword><style  face="normal" font="default" size="100%">INTERFERENCE</style></keyword><keyword><style  face="normal" font="default" size="100%">LASER-COOLED RUBIDIUM</style></keyword><keyword><style  face="normal" font="default" size="100%">POPULATION-INVERSION</style></keyword><keyword><style  face="normal" font="default" size="100%">RB VAPOR</style></keyword><keyword><style  face="normal" font="default" size="100%">sodium</style></keyword><keyword><style  face="normal" font="default" size="100%">SPECTROSCOPY</style></keyword><keyword><style  face="normal" font="default" size="100%">TRAPPED ATOMS</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2000</style></year><pub-dates><date><style  face="normal" font="default" size="100%">May</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000086953200103</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">5</style></number><volume><style face="normal" font="default" size="100%">61</style></volume><pages><style face="normal" font="default" size="100%">6</style></pages><isbn><style face="normal" font="default" size="100%">1050-2947</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We have observed various Lambda-type electromagnetically induced transparency (EIT) spectra in laser-cooled Rb-87 atoms of different laser polarization configurations. Unexpected profiles occur in the EIT spectra. We have found the degenerate Zeeman sublevels are responsible for these profiles. The experimental data are in good agreement with the results from the theoretical calculation which takes into account all the 13 Zeeman levels in the Lambda system. Our study demonstrates that Zeeman sublevels play important roles in quantum interference phenomena such as EIT and amplification without population inversion (AWI), and should be taken into account in the analysis of these phenomena.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000086953200103</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 312QDTimes Cited: 24Cited Reference Count: 27Cited References:      Akulshin AM, 1999, PHYS REV LETT, V83, P4277, DOI 10.1103/PhysRevLett.83.4277     Kitching J, 1999, PHYS REV A, V59, P4685, DOI 10.1103/PhysRevA.59.4685     Lezama A, 1999, PHYS REV A, V59, P4732, DOI 10.1103/PhysRevA.59.4732     Mitsunaga M, 1999, PHYS REV A, V59, P4773, DOI 10.1103/PhysRevA.59.4773     Hau LV, 1999, NATURE, V397, P594, DOI 10.1038/17561     Chen HX, 1998, PHYS REV A, V58, P1545, DOI 10.1103/PhysRevA.58.1545     Durrant AV, 1998, OPT COMMUN, V151, P136, DOI 10.1016/S0030-4018(98)00052-2     Akulshin AM, 1998, PHYS REV A, V57, P2996, DOI 10.1103/PhysRevA.57.2996     Marangos JP, 1998, J MOD OPTIC, V45, P471, DOI 10.1080/09500349808231909     Cataliotti FS, 1997, PHYS REV A, V56, P2221, DOI 10.1103/PhysRevA.56.2221     Hopkins SA, 1997, OPT COMMUN, V138, P185, DOI 10.1016/S0030-4018(97)00030-8     vanderVeldt T, 1997, OPT COMMUN, V137, P420, DOI 10.1016/S0030-4018(96)00797-3     Mitsunaga M, 1996, J OPT SOC AM B, V13, P2696, DOI 10.1364/JOSAB.13.002696     Li YQ, 1996, OPT LETT, V21, P1064, DOI 10.1364/OL.21.001064     Grynberg G, 1996, PHYS REV A, V54, P776, DOI 10.1103/PhysRevA.54.776     Padmabandu GG, 1996, PHYS REV LETT, V76, P2053, DOI 10.1103/PhysRevLett.76.2053     Ling HY, 1996, PHYS REV A, V53, P1014, DOI 10.1103/PhysRevA.53.1014     ARIMONDO E, 1996, PROGR OPTICS, V35, P258     GEABANACLOCHE J, 1995, PHYS REV A, V51, P576, DOI 10.1103/PhysRevA.51.576     XIAO M, 1995, PHYS REV LETT, V74, P66     HARRIS SE, 1992, PHYS REV A, V46, P29     GRISON D, 1991, EUROPHYS LETT, V15, P149, DOI 10.1209/0295-5075/15/2/007     BOLLER KJ, 1991, PHYS REV LETT, V66, P2539     MONROE C, 1990, PHYS REV LETT, V65, P1571, DOI 10.1103/PhysRevLett.65.1571     HARRIS SE, 1990, PHYS REV LETT, V64, P1107, DOI 10.1103/PhysRevLett.64.1107     IMAMOGLU A, 1989, OPT LETT, V14, P1344, DOI 10.1364/OL.14.001344     RAAB EL, 1987, PHYS REV LETT, V59, P2631, DOI 10.1103/PhysRevLett.59.2631Chen, YC Lin, CW Yu, IAAMERICAN PHYSICAL SOCCOLLEGE PK&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan.Chen, YC (reprint author), Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Tung, S. K.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Lin, C. W.</style></author><author><style face="normal" font="default" size="100%">Hsu, L.</style></author><author><style face="normal" font="default" size="100%">Yu, I. A.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Cooling atoms below 100 mu K</style></title><secondary-title><style face="normal" font="default" size="100%">Chinese Journal of Physics</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Chin. J. Phys.</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">LASER</style></keyword><keyword><style  face="normal" font="default" size="100%">LIMIT</style></keyword><keyword><style  face="normal" font="default" size="100%">RADIATION PRESSURE</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">2000</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Apr</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:000086700400030</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">2</style></number><volume><style face="normal" font="default" size="100%">38</style></volume><pages><style face="normal" font="default" size="100%">395-399</style></pages><isbn><style face="normal" font="default" size="100%">0577-9073</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We capture Rb-87 atoms from room-temperature background vapor with a magneto-optical trap (MOT). The temperature of the atoms in the MOT is 320 mu K as the result of Doppler cooling. We further employ polarization gradient cooling to lower atom temperature. The factors that can affect the performance of polarization gradient cooling have been systematically studied. An atom temperature of 75 mu K has been reached with the optimized conditions. Temperatures are measured by the release and recapture method and the time of flight method. Such cold atoms are ready for the evaporative cooling which will finally realize the Bose-Einstein condensation.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article; Proceedings Paper</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:000086700400030</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: 308FTTimes Cited: 0Cited Reference Count: 9Cited References:      Snadden MJ, 1997, OPT LETT, V22, P892, DOI 10.1364/OL.22.000892     Ye J, 1996, OPT LETT, V21, P1280, DOI 10.1364/OL.21.001280     ANDERSEN ML, 1995, GENDER SOC, V9, P269, DOI 10.1177/089124395009003001     MONROE C, 1990, PHYS REV LETT, V65, P1571, DOI 10.1103/PhysRevLett.65.1571     CASTIN Y, 1989, J OPT SOC AM B, V6, P2046, DOI 10.1364/JOSAB.6.002046     DALIBARD J, 1989, J OPT SOC AM B, V6, P2023, DOI 10.1364/JOSAB.6.002023     UNGAR PJ, 1989, J OPT SOC AM B, V6, P2058, DOI 10.1364/JOSAB.6.002058     RAAB EL, 1987, PHYS REV LETT, V59, P2631, DOI 10.1103/PhysRevLett.59.2631     CHU S, 1985, PHYS REV LETT, V55, P48, DOI 10.1103/PhysRevLett.55.48Tung, SK Chen, YC Lin, CW Hsu, L Yu, IATaiwan International Conference on Superconductivity (TICS 99)/6th Workshop on Low Temperature Physics (WLTP6)AUG 17-20, 1999KENTING, TAIWANNatl Sun Yat Sen Univ, Kaohsiung, Dept PhysPHYSICAL SOC REPUBLIC CHINATAIPEIPart 2&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan. Natl Chiao Tung Univ, Dept Electrophys, Hsinchu 300, Taiwan.Tung, SK (reprint author), Natl Tsing Hua Univ, Dept Phys, Hsinchu 300, Taiwan</style></auth-address></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Guan, W. Y.</style></author><author><style face="normal" font="default" size="100%">Xu, Y. H.</style></author><author><style face="normal" font="default" size="100%">Sheen, S. R.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Wei, J. Y. T.</style></author><author><style face="normal" font="default" size="100%">Lai, HF</style></author><author><style face="normal" font="default" size="100%">Wu, M. K.</style></author><author><style face="normal" font="default" size="100%">Ho, J. C.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">ION-SIZE EFFECT ON TN IN (R1-XPRX)BA2CU3O7-Y SYSTEMS (R=LU, YB, TM, ER, Y, HO, DY, GD, EU, SM, AND ND)</style></title><secondary-title><style face="normal" font="default" size="100%">Physical Review B</style></secondary-title><short-title><style face="normal" font="default" size="100%">ION-SIZE EFFECT ON TN IN (R1-XPRX)BA2CU3O7-Y SYSTEMS (R=LU, YB, TM, ER, Y, HO, DY, GD, EU, SM, AND ND)</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">1994</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Jun 1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:A1994NR70100063</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">49</style></volume><pages><style face="normal" font="default" size="100%">15993-15999</style></pages><isbn><style face="normal" font="default" size="100%">0163-1829</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;We conducted a detailed study of the structure and magnetic properties of (R1-xPrx)Ba2Cu3O7 sintered samples, where R = Lu, Yb, Tm, Er, Y, Ho, Dy, Gd, Eu, Sm, and Nd for x = 0.5-1.0. We found that the temperature dependence of the dc susceptibility follows the Curie-Weiss law in the temperature range 20-300 K and the paramagnetism of the Pr and R sublattices exist independently of one another. The antiferromagnetic ordering temperature T(N) of Pr ions decreases monotonically with increasing R concentration (1-x). At a given x, T(N) is R-ion-size dependent. The slope in the T(N) vs x curve is steeper for ions with smaller ionic radii. The observed results are interpreted in terms of the hybridization between the local states of the Pr ion and the valence-band states of the CuO2 planes.&lt;/p&gt;
</style></abstract><accession-num><style face="normal" font="default" size="100%">WOS:A1994NR70100063</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;Times Cited: 52&lt;/p&gt;
</style></notes></record><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Guan, W. Y.</style></author><author><style face="normal" font="default" size="100%">Y. C. Chen</style></author><author><style face="normal" font="default" size="100%">Wei, J. Y. T.</style></author><author><style face="normal" font="default" size="100%">Xu, Y. H.</style></author><author><style face="normal" font="default" size="100%">Wu, M. K.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">ION-SIZE EFFECT ON T(M) AND T(C) IN (R1-XPR(X))BA2CU3O7 SYSTEMS (R = YB, TM, ER, HO, DY, GD, EU, SM, ND AND Y)</style></title><secondary-title><style face="normal" font="default" size="100%">Physica C-Superconductivity and Its Applications</style></secondary-title><alt-title><style face="normal" font="default" size="100%">Physica C</style></alt-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">MAGNETIC ORDER</style></keyword><keyword><style  face="normal" font="default" size="100%">PR</style></keyword><keyword><style  face="normal" font="default" size="100%">SUPERCONDUCTIVITY</style></keyword><keyword><style  face="normal" font="default" size="100%">YBA2CU3O7-DELTA</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">1993</style></year><pub-dates><date><style  face="normal" font="default" size="100%">Apr</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">&lt;Go to ISI&gt;://WOS:A1993KZ52100007</style></url></web-urls></urls><number><style face="normal" font="default" size="100%">1-3</style></number><volume><style face="normal" font="default" size="100%">209</style></volume><pages><style face="normal" font="default" size="100%">19-22</style></pages><isbn><style face="normal" font="default" size="100%">0921-4534</style></isbn><language><style face="normal" font="default" size="100%">English</style></language><abstract><style face="normal" font="default" size="100%">&lt;p&gt;The magnetic ordering temperatures T(m) of Pr ions in (R1-xPrx)Ba2Cu3O7 systems (R = Yb, Tm, Er, Ho, Dy, Gd, Eu, Sm, Nd and Y) with x = 0.5 - 1.0 were measured. We observe that T(m) decreases monotonically with increasing R concentration. At constant x, T(m) is R ion-size dependent. The slope in the T(m) vs. x is steeper for ion with smaller ionic radius. In comparison with the ion-size effect on the superconducting transition temperatures T(c) in these systems, the observed results can be qualitatively interpreted in terms of the hybridization between the local states of Pr ion and the conduction band states of the CuO2 planes.&lt;/p&gt;
</style></abstract><work-type><style face="normal" font="default" size="100%">Article; Proceedings Paper</style></work-type><accession-num><style face="normal" font="default" size="100%">WOS:A1993KZ52100007</style></accession-num><notes><style face="normal" font="default" size="100%">&lt;p&gt;ISI Document Delivery No.: KZ521Times Cited: 25Cited Reference Count: 14Cited References:      XU YH, 1992, PHYS REV B, V45, P3176, DOI 10.1103/PhysRevB.45.3176     NIEVA G, 1991, PHYS REV B, V44, P6999, DOI 10.1103/PhysRevB.44.6999     XU YH, 1991, SOLID STATE COMMUN, V80, P105, DOI 10.1016/0038-1098(91)90296-8     GHAMATY S, 1991, PHYS REV B, V43, P5430, DOI 10.1103/PhysRevB.43.5430     DAS I, 1991, PHYSICA C, V173, P331, DOI 10.1016/0921-4534(91)90732-E     YANG HD, 1990, PHYSICA B, V165, P1193     FELNER I, 1989, PHYS REV B, V40, P6739, DOI 10.1103/PhysRevB.40.6739     KEBEDE A, 1989, PHYS REV B, V40, P4453, DOI 10.1103/PhysRevB.40.4453     LI WH, 1989, PHYS REV B, V40, P5300, DOI 10.1103/PhysRevB.40.5300     XU YH, 1988, APPL PHYS LETT, V53, P334, DOI 10.1063/1.100600     SODERHOLM L, 1987, NATURE, V328, P604, DOI 10.1038/328604a0     HO JC, 1987, SOLID STATE COMMUN, V63, P711, DOI 10.1016/0038-1098(87)90115-3     YU J, 1987, PHYS LETT A, V122, P203, DOI 10.1016/0375-9601(87)90807-3     NAKAMARA F, SOLID STATE COMMUN, V65, P1339GUAN, WY CHEN, YC WEI, JYT XU, YH WU, MK2ND ISRAELI INTERNATIONAL CONF ON HIGH-TEMPERATURE SUPERCONDUCTIVITYJAN 04-08, 1992EILAT, ISRAELCNRS, ITALIAN NATL RES COUNCIL, BRIT COUNCIL, USA, EUROPEAN OFF AEROSP RES &amp;amp; DEV, ISRAELI MINIST FOREIGN AFFAIRS, TEL AVIV UNIV, OREN FAMILY CHAIR EXPTL SOLID STATE PHYSELSEVIER SCIENCE BVAMSTERDAM&lt;/p&gt;
</style></notes><auth-address><style face="normal" font="default" size="100%">NATL TSING HUA UNIV,DEPT PHYS,HSINCHU 30043,TAIWAN.GUAN, WY (reprint author), NATL TSING HUA UNIV,CTR MAT SCI,HSINCHU 30043,TAIWAN</style></auth-address></record></records></xml>