Szczegóły seminarium
Data: 17.10.2023
Bryn Haskell (CAMK Warsaw)
Astrophysics with continuous gravitational waves
Streszczenie:
The era of gravitational wave astronomy has begun, and the recent
detection of signals from a binary neutron star coalescence has allowed
to start probing high density physics in neutron star interiors in
unprecedented ways. There is, however, another class of predicted
gravitational wave signals that may allow for even more detailed studies
of the interior of these compact stars, i.e. long lived
quasi-monochromatic signals, or 'continuous' gravitational waves (CWs).
These signals have not yet been detected, but the sensitivity of the
recent observational run of the gravitational wave detectors, O3, has
reached the point where realistic astrophysical scenarios can be probed.
In this talk I will present the theoretical mechanisms for CW emission
and expected sources, and review the results obtained by the
LIGO-Virgo-KAGRA collaboration during O3.
Bio:
Brynmor Haskell obtained his PhD from the University of Southampton in
2006, under the supervision of Nils Andersson. After staying in
Southampton for a postdoc he moved to Amsterdam with a Marie Skłodowska
Curie Fellowship and after a short stay at the Albert Einstein Institute
in Golm, Germany, to Melbourne with a DECRA fellowship from the
Australian Research Council. In 2016 he then obtained a Marie
Skłodowska Curie fellowship to come to CAMK in Warsaw, where he is
currently an Associate Professor.