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SUMMARY:Continuous gravitational-wave searches for dark matter in O4 LIGO 
 data
DTSTART;VALUE=DATE-TIME:20260705T083000Z
DTEND;VALUE=DATE-TIME:20260705T090000Z
DTSTAMP;VALUE=DATE-TIME:20261027T060753Z
UID:indico-contribution-808@indico.narit.or.th
DESCRIPTION:Speakers: Andrew Miller (ICTP - AP / University Chinese Academ
 y of Sciences)\nDark matter could compose ~80% of all matter in the univer
 se\, and yet it is completely invisible to us. Despite decades of experime
 nts designed to detect dark matter\, and numerous models for potential dar
 k matter particles\, no concrete evidence has been put forward to support 
 the existence of beyond standard-model physics. Because of this\, it is wo
 rth asking whether approaching the detection of dark matter from a differe
 nt point of view\, that is\, via gravitational-wave interferometers\, coul
 d provide some insight into explaining the origin of dark matter. In this 
 talk\, I will discuss searches for dark matter in two forms: ultralight pa
 rticle dark matter and sub-solar mass primordial black holes. While not de
 signed to search for dark matter\, gravitational-wave detectors can robust
 ly probe a variety of dark-matter models simultaneously\, without affectin
 g their sensitivity to canonical gravitational-wave sources\, and put comp
 etitive and sometimes even stronger constraints than those from other expe
 riments designed to search for dark matter.\n\nhttps://indico.narit.or.th/
 event/236/contributions/808/
LOCATION:National Astronomical Research Institute of Thailand (NARIT) Andr
 omeda Meeting Room
URL:https://indico.narit.or.th/event/236/contributions/808/
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