Hitoshi Murayama
(University of California Berkeley (US))
2/1/21, 9:30 AM
Jihn E. Kim
(Kyung Hee University)
2/1/21, 11:10 AM
I show a possibility that a quintessential axion (with its breaking by the weak SU(2) gauge anomaly) can be the source of dark energy. However, I cannot show why the minimum of the potential is at the zero value for the cosmological constant.
Hai-Bo Yu
(University of California, Riverside)
2/1/21, 2:00 PM
Deog Ki Hong
(Pusan National University (KR))
2/1/21, 2:40 PM
The standard cooling scenario in the presence of nucleon superfluidity fits rather well to the observation of the neutron stars. It implies that the stellar cooling arguments could place a stringent constraint on the properties of novel particles. We study in particular the cooling rate induced by dark gauge bosons for very young neutron stars: remnants of Cassiopeia A and SN1987A. The cooling...
Eung Jin Chun
(Korea Institute for Advanced Study)
2/1/21, 4:40 PM
Sin Kyu Kang
(Seoul-Tech)
2/1/21, 5:10 PM
Chang Sub Shin
(Institute for Basic Science )
2/2/21, 10:10 AM
Sunghoon Jung
(Seoul National University)
2/2/21, 11:40 AM
Yuhsin Tsai
(Fermilab/Cornell)
2/3/21, 11:00 AM
Pyungwon Ko
(Korea Inst. for Advanced Study (KIAS))
2/3/21, 2:00 PM
Jong-Chul Park
2/3/21, 2:40 PM
Chang Hyon Ha
(Chung-Ang University)
2/3/21, 3:10 PM
Dumitru Ghilencea
(IFIN-HH (RO))
2/3/21, 4:00 PM
Gungwon Kang
(KISTI)
2/3/21, 4:40 PM