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Iwasaki, Sachio*; Jido, Daisuke*; Oka, Makoto; Suzuki, Kei
Physics Letters B, 820, p.136498_1 - 136498_6, 2021/09
Times Cited Count:2 Percentile:18.91(Astronomy & Astrophysics)We investigate time evolution of -wave charmonium populations under a time-dependent homogeneous magnetic field and evaluate survival probabilities of the low-lying charmonia to the goal of estimating the magnetic field strength at heavy-ion collisions. Our approach implements mixing between different spin eigenstates and transitions to radially excited states. We show that the survival probabilities can change even by an extremely short magnetic field. Furthermore, we find that the survival probabilities depend on the initial spin states. We propose the sum of the survival probabilities over spin partners as an observable insensitive to the initial states. We also find that the sum can be approximately given as a function of with a duration time and the maximum strength of the magnetic field .
Iwasaki, Sachio*; Oka, Makoto; Suzuki, Kei
European Physical Journal A, 57(7), p.222_1 - 222_14, 2021/07
Times Cited Count:17 Percentile:70.63(Physics, Nuclear)We review the properties of quarkonia under strong magnetic fields. The main phenomena are (i) mixing between different spin eigenstates, (ii) quark Landau levels and deformation of wave function, (iii) modification of potential, and (iv) the motional Stark effect. For theoretical approaches, we review (i) constituent quark models, (ii) effective Lagrangians, (iii) QCD sum rules, and (iv) holographic approaches.
Acharya, U.*; Hasegawa, Shoichi; Imai, Kenichi*; Nagamiya, Shoji*; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 397 of others*
Physical Review C, 102(6), p.064905_1 - 064905_13, 2020/12
Times Cited Count:5 Percentile:52.72(Physics, Nuclear)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji*; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 666 of others*
Physical Review Letters, 123(2), p.022301_1 - 022301_10, 2019/07
Times Cited Count:30 Percentile:86.91(Physics, Multidisciplinary)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji*; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 451 of others*
Physical Review C, 99(5), p.054903_1 - 054903_29, 2019/05
Times Cited Count:15 Percentile:83.07(Physics, Nuclear)Aidala, C.*; Hasegawa, Shoichi; Imai, Kenichi; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 293 of others*
Physical Review C, 99(4), p.044912_1 - 044912_10, 2019/04
Times Cited Count:5 Percentile:47.88(Physics, Nuclear)Aidala, C.*; Hasegawa, Shoichi; Imai, Kenichi; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 312 of others*
Nature Physics, 15(3), p.214 - 220, 2019/03
Times Cited Count:149 Percentile:99.03(Physics, Multidisciplinary)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 317 of others*
Physical Review C, 99(2), p.024903_1 - 024903_16, 2019/02
Times Cited Count:11 Percentile:74.44(Physics, Nuclear)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 448 of others*
Physical Review C, 98(5), p.054902_1 - 054902_11, 2018/11
Times Cited Count:14 Percentile:75.94(Physics, Nuclear)Aidala, C.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji*; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 397 of others*
Physical Review C, 98(5), p.054903_1 - 054903_11, 2018/11
Times Cited Count:11 Percentile:68.32(Physics, Nuclear)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 362 of others*
Physical Review Letters, 121(22), p.222301_1 - 222301_8, 2018/11
Times Cited Count:34 Percentile:86.03(Physics, Multidisciplinary)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 468 of others*
Physical Review C, 98(1), p.014912_1 - 014912_16, 2018/07
Times Cited Count:7 Percentile:53.6(Physics, Nuclear)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 347 of others*
Physical Review C, 97, p.064904_1 - 064904_11, 2018/06
Times Cited Count:22 Percentile:86.47(Physics, Nuclear)Adare, A.*; Hasegawa, Shoichi; Nagamiya, Shoji; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 448 of others*
Physical Review C, 97(6), p.064911_1 - 064911_22, 2018/06
Times Cited Count:32 Percentile:92.26(Physics, Nuclear)Aidala, C.*; Hasegawa, Shoichi; Imai, Kenichi; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 311 of others*
Physical Review Letters, 120(6), p.062302_1 - 062302_8, 2018/02
Times Cited Count:42 Percentile:89.79(Physics, Multidisciplinary)Aidala, C.*; Hasegawa, Shoichi; Imai, Kenichi; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 456 of others*
Physical Review C, 96(6), p.064901_1 - 064901_18, 2017/12
Times Cited Count:3 Percentile:27.61(Physics, Nuclear)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 497 of others*
Physical Review C, 96(2), p.024907_1 - 024907_19, 2017/08
Times Cited Count:11 Percentile:65.8(Physics, Nuclear)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 462 of others*
Physical Review D, 95(7), p.072002_1 - 072002_19, 2017/04
Times Cited Count:11 Percentile:49.91(Astronomy & Astrophysics)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 545 of others*
Physical Review C, 94(6), p.064901_1 - 064901_14, 2016/12
Times Cited Count:74 Percentile:97.96(Physics, Nuclear)Adare, A.*; Hasegawa, Shoichi; Imai, Kenichi; Nagamiya, Shoji; Sako, Hiroyuki; Sato, Susumu; Tanida, Kiyoshi; PHENIX Collaboration*; 397 of others*
Physical Review C, 94(5), p.054910_1 - 054910_18, 2016/11
Times Cited Count:24 Percentile:84.18(Physics, Nuclear)