Szczegóły seminarium
Data: 12.03.2024
Aleksandra Olejak (MPIA, Garching)
Fingerprints of binary star interactions in the parameters of binary black hole mergers
Streszczenie:
The growing database of gravitational wave (GW) detections with inferred
parameters of merging black holes (BH-BH) contains non-obvious insights
into their formation scenarios. Interactions in massive star binaries in
the form of stable or unstable mass transfer are expected to accompany
the formation of GW sources. Those interactions could leave
characteristic fingerprints in the parameters (masses and spins) of
detected BH-BH systems. Therefore, their identification would help in
constraining poorly understood parts of stellar evolution. Restricted
criteria for common envelope development (i.e. unstable mass transfer)
combined with efficient tidal spin-up of stripped helium core may result
in a characteristic pattern in effective spin vs mass ratio
distributions of merging BH-BH, consistent with GW detections. In
particular, the progenitors of unequal BH-BH systems in the stable mass
transfer formation scenario experience more efficient orbital
contraction during the second Roche Lobe Overflow than nearly equal mass
component systems. That makes it easier for unequal-mass progenitors to
enter the tidal spin-up regime and later merge due to GW emission. Our
result is, however, sensitive to highly uncertain assumptions on angular
momentum loss. We conclude that a significant fraction of unequal-mass
BH-BH mergers among the future GW detections could indicate the
contribution of a stable mass transfer formation channel. Such a
population would be consistent with the mass ratio reversal scenario
during the first, relatively conservative mass transfer, and low angular
momentum loss during the second, highly non-conservative mass transfer
phase.
Bio:
- engineer at the Faculty of Physics, Warsaw University of Technology
(2017)
- Master's degree at Astronomical Observatory, UW (2019)
- PhD at CAMK PAN (2023)
- currently a postdoc fellow at the Max Planck Institute for Astrophysics
in Garching
Main scientific interests:
evolution of massive stars in isolated binary systems,formation scenarios of binary black hole mergers,
gravitational wave sources and their origin (mainly under LIGO/Virgo and LISA