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Accuracy of inference on the physics of binary evolution from gravitational-wave observations
Jim W. Barrett, Sebastian M. Gaebel, Coenraad J. Neijssel +5
The properties of the population of merging binary black holes encode some of the uncertain physics of the evolution of massive stars in binaries. The binary black hole merger rate…
Predicting the Presence of Companions for Stripped-Envelope Supernovae: The Case of the Broad-Lined Type Ic SN 2002ap
E. Zapartas, S. E. de Mink, S. D. Van Dyk +10
Many young, massive stars are found in close binaries. Using population synthesis simulations we predict the likelihood of a companion star being present when these massive stars e…
Exploring the Parameter Space of Compact Binary Population Synthesis
Jim W. Barrett, Ilya Mandel, Coenraad J. Neijssel +2
As we enter the era of gravitational wave astronomy, we are beginning to collect observations which will enable us to explore aspects of astrophysics of massive stellar binaries wh…
Formation of the first three gravitational-wave observations through isolated binary evolution
Simon Stevenson, Alejandro Vigna-Gómez, Ilya Mandel +4
During its first 4 months of taking data, Advanced LIGO has detected gravitational waves from two binary black hole mergers, GW150914 and GW151226, along with the statistically les…
Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction
E. Zapartas, S. E. de Mink, R. G. Izzard +8
Most massive stars, the progenitors of core-collapse supernovae, are in close binary systems and may interact with their companion through mass transfer or merging. We undertake a…