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Spin of Primordial Black Holes

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arxiv 1901.05963 v3 pith:YS4UFUIO submitted 2019-01-17 astro-ph.CO gr-qchep-phhep-th

Spin of Primordial Black Holes

classification astro-ph.CO gr-qchep-phhep-th
keywords spinblackprimordialzetaholesorderparameteracoustic
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Primordial black holes, formed from rare peaks in the primordial fluctuations $\zeta$, are non-rotating at zeroth order in $\zeta_{\rm rms}$. We show that the spin also vanishes at first order in $\zeta_{\rm rms}$, suggesting the dimensionless spin parameter $a_{\rm rms} \sim \zeta_{\rm rms}^2$. We identify one quadratic contribution to the spin by calculating (and extrapolating to the formation time) the torque on a black hole due to ambient acoustic waves. For a reasonable density of primordial black holes this implies a percent level spin parameter.

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Cited by 11 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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  3. The Gravitational Spectral Radio Forest: A Signature of Primordial Black Holes

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    High-energy neutrino telescopes constrain sub-asteroid mass primordial black holes with extended mass functions as dark matter, yielding limits slightly weaker than but independent of gamma-ray bounds.

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    gr-qc 2021-11 accept novelty 4.0

    GWTC-3 catalogs 90 compact binary coalescence events with p_astro > 0.5 from LIGO and Virgo's first three observing runs, including the first confident neutron star-black hole binaries.

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