BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Ultra-high-accuracy computation and gravitational self-force obser
vables in binary black holes
DTSTART;VALUE=DATE-TIME:20141105T134500Z
DTEND;VALUE=DATE-TIME:20141105T144500Z
DTSTAMP;VALUE=DATE-TIME:20201025T055155Z
UID:indico-event-632@indico.math.cnrs.fr
DESCRIPTION:\nThe principal approximation methods used to compute the insp
iral of compact binary systems are the post-Newtonian (pN) expansion\, in
which an orbital angular velocity MΩ serves as the expansion parameter\;
and the self-force or extreme-mass-ratio-inspiral approach\, in which the
small parameter is the mass ratio m/M of the binary’s two components. We
work in an overlapping regime where both approximations are valid and fin
d numerical values of pN coefficients at orders beyond the reach of curren
t analytical work. In this talk we present a novel analytic extraction of
high-order pN parameters that govern quasi-circular binary systems using u
ltra-high accuracy numerical computations.\n\nhttps://indico.math.cnrs.fr/
event/632/
LOCATION:IHES Amphithéâtre Léon Motchane
URL:https://indico.math.cnrs.fr/event/632/
END:VEVENT
END:VCALENDAR