BEGIN:VCALENDAR
VERSION:2.0
PRODID:researchseminars.org
CALSCALE:GREGORIAN
X-WR-CALNAME:researchseminars.org
BEGIN:VEVENT
SUMMARY:Alejandro Torres-Orjuela (Peking U.\, Beijing and Peking U.\, Beij
 ing\, KIAA)
DTSTART:20200722T100000Z
DTEND:20200722T110000Z
DTSTAMP:20260423T035755Z
UID:CENTRA/9
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/CENTRA/9/">P
 hase Shift of Gravitational Waves induced by Aberration</a>\nby Alejandro 
 Torres-Orjuela (Peking U.\, Beijing and Peking U.\, Beijing\, KIAA) as par
 t of CENTRA Seminar\n\n\nAbstract\nThe velocity of a gravitational wave (G
 W) source provides crucial information about its formation and evolution p
 rocesses. Previous studies considered the Doppler effect on the phase of G
 Ws as a potential signature of a time-dependent velocity of the source. Ho
 wever\, the Doppler shift only accounts for the time component of the wave
  vector\, and in principle motion also affects the spatial components. In 
 my talk I discuss the latter effect\, known as “aberration” for light\
 , for GWs and how it affects the waveform modelling of an accelerating sou
 rce. I show that the additional aberrational phase shift could be detectab
 le in two astrophysical scenarios\, namely\, a recoiling binary black hole
  (BBH) due to GW radiation and a BBH in a triple system. Further\, I discu
 ss how adding the aberrational phase shift in the waveform templates could
  significantly enhance the detectability of moving sources.\n
LOCATION:https://researchseminars.org/talk/CENTRA/9/
END:VEVENT
END:VCALENDAR
