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SUMMARY:Black hole superradiance
DTSTART;VALUE=DATE-TIME:20250320T020000Z
DTEND;VALUE=DATE-TIME:20250320T040000Z
DTSTAMP;VALUE=DATE-TIME:20260618T044600Z
UID:indico-event-25526@indico.ihep.ac.cn
DESCRIPTION:Speakers: Hong Zhang (Shandong University - Qingdao)\n点击
 链接入会，或添加至会议列表：\nhttps://meeting.tencent.com/dm
 /sDmKVbOO5Y9Y\n\n#腾讯会议：628-408-999\n\nAbstract: \nUltralight sc
 alars and vectors are popular dark matter candidates.They could extract en
 ergy and angular momentum from a Kerr black hole (BH) if the wave length i
 s comparable to the size of BH horizon\, forming a sizeable condensate aro
 und the host BH. The growth of the condensate\, together with its gravitat
 ional wave radiation\, provides a model-independent strategy to search for
  these new particles. In this talk\, I will introduce the evolution of the
  BH-condensate system and its gravitational wave emission. The effect of a
 ccretion will also be discussed.\n\nSelf-introduction:\nHong Zhang receive
 d his bachelor’s degree in Physics from USTC in 2008. Then he moved to t
 he United States and received his Ph.D. at Stony Brook University in New Y
 ork in 2014. Later\, he worked as a postdoc\, first at Ohio State Universi
 ty and then at Munich Technical University. In 2019\, he joined Shandong U
 niversity\, Qingdao campus. He is interested in effective field theories a
 nd their applications on heavy quarkonium and axions.\nhttps://indico.ihep
 .ac.cn/event/25526/
URL:https://indico.ihep.ac.cn/event/25526/
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