-
Dan Hooper07/02/2022, 09:30
-
Pyungwon Ko07/02/2022, 10:20
-
Jong Chul Park07/02/2022, 11:20
-
Chang Hyon Ha (Chung-Ang University)07/02/2022, 11:50
-
Koichi Hamaguchi (University of Tokyo)07/02/2022, 13:40
-
Eung Jin Chun07/02/2022, 14:30
-
Kyu Jung Bae (Kyungbook National University)07/02/2022, 15:00
-
Michelle Galloway (University of Zürich)07/02/2022, 16:00
-
Francesco D'Eramo (University of Padua)07/02/2022, 16:50
-
Keisuke Harigaya (CERN)07/02/2022, 17:20
-
Yu-Dai Tsai08/02/2022, 09:30
-
Nicolas Bernal08/02/2022, 10:00
-
Hitoshi Murayama08/02/2022, 11:00
-
Youngjoon Kwon08/02/2022, 11:50
-
Masahide Yamaguchi08/02/2022, 13:40
-
Jinn-Ouk Gong08/02/2022, 14:30
-
Ki-Young Choi (Sungkyunkwan University)08/02/2022, 15:00
-
Joachim Kopp08/02/2022, 16:00
-
Eric Kuflik08/02/2022, 16:50
-
Seung J. Lee (Korea University)08/02/2022, 17:20
-
Taehyun Jung09/02/2022, 09:30
-
Po-Yen Tseng (National Tsing Hua University, Department of Physics)09/02/2022, 10:00
-
Chang Sub Shin09/02/2022, 11:00
-
Seong Chan Park (Yonsei University)09/02/2022, 11:30
-
Fuminobu Takahashi09/02/2022, 13:40
-
Wen Yin09/02/2022, 14:30
-
Mathias Pierre (DESY)09/02/2022, 15:00
In this talk I discuss various possibilities of producing dark matter in a state out of thermal equilibrium. I will show that the non-thermal nature of dark matter can leave an imprint on the matter power spectrum, which features a cutoff analogous to that for warm dark matter. I will present a mapping procedure that allows translating the Lyman-alpha forest mass bound to such scenarios and...
Go to contribution page -
Mikhail Shaposhnikov09/02/2022, 16:00
-
Yann Mambrini09/02/2022, 16:50
-
Oleg Lebedev09/02/2022, 17:20
-
Brian Thomas Batell10/02/2022, 09:30
-
Seodong Shin (Jeonbuk National University)10/02/2022, 10:20
-
Deog Ki Hong (Pusan National University (KR))10/02/2022, 11:20
-
Choong Sun Kim (Yonsei University)10/02/2022, 11:50
-
Donghui Jeong (The Pennsylvania State University)10/02/2022, 13:40
-
Ji-hoon Kim10/02/2022, 14:30
-
Gungwon Kang10/02/2022, 15:00
-
Kfir Blum10/02/2022, 16:00
The time delay between the images of gravitationally lensed quasars probes a combination of angular diameter distances and the mass profile of the lens galaxy. Some observational campaigns to measure such systems have reported a determination of the Hubble parameter H0 in tension with determinations based on the cosmic microwave background and large scale structure. I will discuss challenges...
Go to contribution page -
Hyungjin Kim10/02/2022, 16:50
-
Sunghoon Jung (Seoul National University)10/02/2022, 17:20
-
Youngjoon Kwon
-
Jong Chul Park (Chungnam National University)
-
Gungwon Kang
Choose timezone
Your profile timezone: