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The binary black hole merger events observed by the Advanced LIGO (aLIGO) and VIRGO collaboration can shed light on the origins of black holes.
1927
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N. Smirnov, Table for estimating the goodness of fit of empirical distributions
1948
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L. S. Finn and D. F. Chernoff, Observing binary inspiral in gravitational radiation: One interferometer
1993
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C. M. Will and A. G. Wiseman, Gravitational radiation from compact binary systems: Gravitational wave forms and energy loss to second postNewtonian order
1996
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T. Nakamura, M. Sasaki, T. Tanaka, and K. S. Thorne, Gravitational waves from coalescing black hole MACHO binaries
1997
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E. E. Flanagan and S. A. Hughes, Measuring gravitational waves from binary black hole coalescences: 1. Signal-to-noise for inspiral, merger, and ringdown
1998
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P. Kroupa, On the variation of the initial mass function
2001
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A. Heger and S. E. Woosley, The nucleosynthetic signature of population III
2002
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S. E. Woosley, A. Heger, and T. A. Weaver, The evolution and explosion of massive stars
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2011
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S. E. Woosley, Pulsational Pair-Instability Supernovae
2017
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M. Fishbach and D. E. Holz, Where Are LIGO’s Big Black Holes?
2017
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