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SUMMARY:Fundamental oscillation modes of self-interacting bosonic dark sta
 rs
DTSTART;VALUE=DATE-TIME:20190629T030000Z
DTEND;VALUE=DATE-TIME:20190629T033000Z
DTSTAMP;VALUE=DATE-TIME:20260517T093752Z
UID:indico-contribution-5@indico.itp.ac.cn
DESCRIPTION:Speakers: 陳 樫旭 (淡江大學)\nWe perform a detailed ana
 lysis of the fundamental f-mode frequencies and damping times of nonrotati
 ng stellar-mass boson stars in general relativity by solving the nonradial
  perturbation equations. Two parameters which govern the microscopic prope
 rties of the bosonic condensates\, namely the self-coupling strength and t
 he mass of the scalar particle\, are explored. These two quantities charac
 terize oscillations of boson stars. Specifically\, we reexamine some empir
 ical relations that describe the f-mode parameters in terms of the mass an
 d radius of boson stars.\n\nhttps://indico.itp.ac.cn/event/1/contributions
 /5/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/5/
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