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Bound on induced gravitational wave background from primordial black holes

  • Gravity, Astrophysics
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Abstract

The today’s energy density of the induced (second order) gravitational wave background in the frequency region ∼10−3–103 Hz is constrained using the existing limits on primordial black hole production in the early Universe. It is shown, in particular, that at frequencies near ∼40 Hz (which is the region explored by LIGO detector), the value of the induced part of ΩGW cannot exceed (1−3) × 10−7. The spread of values of the bound is caused by the uncertainty in parameters of the gravitational collapse of black holes.

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Authors and Affiliations

  1. Institute for Nuclear Research, Russian Academy of Sciences, Moscow, 117312, Russia

    E. V. Bugaev & P. A. Klimai

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  1. E. V. Bugaev
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  2. P. A. Klimai
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Correspondence to P. A. Klimai.

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Bugaev, E.V., Klimai, P.A. Bound on induced gravitational wave background from primordial black holes. Jetp Lett. 91, 1–5 (2010). https://doi.org/10.1134/S0021364010010017

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