Dynamical versus isolated formation channels of gravitational wave sources
201820 pages
Published in:
- IAU Symp. (2018) 397-416
Contribution to:
- IAU Symposium 346, 397-416
- Published: Dec 30, 2019
Citations per year
Abstract: (Cambridge University Press)
What are the formation channels of merging black holes and neutron stars? The first two observing runs of Advanced LIGO and Virgo give us invaluable insights to address this question, but a new approach to theoretical models is required, in order to match the challenges posed by the new data. In this review, I discuss the impact of stellar winds, core-collapse and pair instability supernovae on the formation of compact remnants in both isolated and dynamically formed binaries. Finally, I show that dynamical processes, such as the runaway collision scenario and the Kozai-Lidov mechanism, leave a clear imprint on the demography of merging systems.- black hole physics
- gravitational waves
- (stars:) binaries: general
- stellar dynamics
- stars: winds
- galaxies: star clusters
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