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DTSTART;TZID=Atlantic/Canary:20210316T123000
DTEND;TZID=Atlantic/Canary:20210316T133000
UID:iactalks-1453
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1453
CREATED:2021-03-16T12:30:00+00:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Light in the dark: GW190521 as a boson star merger 
DESCRIPTION:Light in the dark: GW190521 as a boson star merger \nDr. NicolÃ
 ¡s Sanchis-Gual\n\nThe detections of gravitational waves are opening a new
  window to the&nbsp;Universe. The nature of black holes and neutron stars 
 may now be unveiled, but gravitational radiation may also lead to exciting
 &nbsp;discoveries of new exotic compact objects, oblivious to electromagne
 tic&nbsp;waves. In particular, Advanced LIGO-Virgo recently reported a sho
 rt&nbsp;gravitational-wave signal (GW190521) interpreted as a quasi-circul
 ar&nbsp;merger of black holes, one at least populating the pair-instabilit
 y&nbsp;supernova gap. We found that GW190521 is also consistent with&nbsp;
 numerically simulated signals from head-on collisions of two (equal mass&n
 bsp;and spin) horizonless vector boson stars (aka Proca stars). This&nbsp;
 provides the first demonstration of close degeneracy between these two&nbs
 p;theoretical models, for a real gravitational-wave event.&nbsp;
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