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Superfluid dark stars

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arxiv 2403.03833 v3 pith:CLFGGVMB submitted 2024-03-06 astro-ph.CO gr-qchep-ph

Lorenzo Cipriani , Massimo Mannarelli , Fabrizio Nesti , Silvia Trabucco This is my paper · ORCID
classification astro-ph.COgr-qchep-ph
keywords darksuperfluidamplitudebinarybosonbosonsconsistingdeformability
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We present a superfluid dark star model consisting of relativistic dark bosons with two-body self-interaction. The obtained masses, radii, and tidal deformability depend in a simple way on the boson mass and interaction strength. We report first results on binary mergers: the distinctive amplitude and frequency of the emitted gravitational waves are well within reach of terrestrial interferometers.

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  1. One Membrane to Love them all: Tidal deformations of compact objects from the membrane paradigm

    gr-qc 2025-06 conditional novelty 7.0 of 10

    The tidal deformability of any compact object in vacuum general relativity can be encoded in the bulk and shear viscosity of a fictitious membrane, with explicit formulas for the electric and magnetic Love numbers.

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