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Merger rate distribution of primordial black hole binaries with electric charges

Published 9 Jan 2020 in astro-ph.CO, gr-qc, and hep-ph | (2001.02984v3)

Abstract: We consider gravitational radiation and electromagnetic radiation from point mass binary with electric charges in a Keplerian orbit, and calculate the merger rate distribution of primordial black hole binaries with charges and a general mass function by taking into account gravitational torque and electromagnetic torque by the nearest primordial black hole. We apply the formalism to the extremal charged case and find that $\alpha=-(m_i+m_j)2\partial2 \ln {\cal R}(m_i,m_j)/\partial m_i \partial m_j=12/11$, which is independent of the mass function.

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