BEGIN:VCALENDAR
VERSION:2.0
PRODID:icalendar-ruby
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VTIMEZONE
TZID:Europe/Vienna
BEGIN:DAYLIGHT
DTSTART:20220327T030000
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
RRULE:FREQ=YEARLY;BYDAY=-1SU;BYMONTH=3
TZNAME:CEST
END:DAYLIGHT
BEGIN:STANDARD
DTSTART:20221030T020000
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
RRULE:FREQ=YEARLY;BYDAY=-1SU;BYMONTH=10
TZNAME:CET
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTAMP:20260405T190601Z
UID:1652709600@ist.ac.at
DTSTART:20220516T160000
DTEND:20220516T170000
DESCRIPTION:Speaker: Zoltan Haiman\nhosted by Tamas Hausel\nAbstract: Black
  holes as massive as several billion solar masses appeared within a billi
 on years after the Big Bang.  The origin of these objects remains a myste
 ry.  I will present three competing state-of-the art ideas on how such m
 assive black holes may have formed in the early universe from stellar bla
 ck  hole remnants\, via rapid gas accretion\, or via successive mergers.
   I will then discuss the role ofcircumbinary gas in mergers between blac
 k holes: for facilitating (or not) the early shrinking of their orbit\, p
 roducing unique observational signatures\, and impacting low-frequency gr
 avitational wave emission.  Upcoming observations with the recently laun
 ched James Webb Space Telescope (JWST) and with the space-based Laser In
 terferometer Space Antenna (LISA) will help us understand the origin of 
 massive black holes\, including the details of their mergers.
LOCATION:Raiffeisen Lecture Hall\, ISTA
ORGANIZER:arinya.eller@ist.ac.at
SUMMARY:Zoltan Haiman: The formation and growth of massive black holes
URL:https://talks-calendar.ista.ac.at/events/3457
END:VEVENT
END:VCALENDAR
