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Primordial stellar-mass black holes, which may contribute to dark matter and to the observed LIGO binary black hole coalescences, are expected to be born with very low spins.
1901
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1903
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T. Nakamura, M. Sasaki, T. Tanaka and K. S. Thorne, Gravitational Waves from Coalescing Black Hole MACHO Binaries , ApJL 487
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K. Ioka, T. Chiba, T. Tanaka and T. Nakamura, Black hole binary formation in the expanding universe: Three body problem approximation , Physical Review D 58
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2016
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B. Carr, F. Kühnel and M. Sandstad, Primordial black holes as dark matter , Physical Review D 94
2016
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