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arxiv: 1802.08259 · v1 · pith:ML3B4CJJnew · submitted 2018-02-22 · ✦ hep-ph · astro-ph.CO

Gravitational Radiation Background from Boson Star Binaries

classification ✦ hep-ph astro-ph.CO
keywords binariesbosongravitationalstarbackgroundformationradiationrate
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We calculate the gravitational radiation background generated from boson star binaries formed in locally dense clusters with formation rate tracked by the regular star formation rate. We compute how the the frequency window in gravitational waves is affected by the boson field mass and repulsive self-coupling, anticipating constraints from EPTA and LISA. We also comment on the possible detectability of these binaries.

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Cited by 1 Pith paper

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

  1. Dynamical Boson Stars

    gr-qc 2012-02 unverdicted novelty 2.0

    Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.