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Probing Bosonic Stars with Atomic Clocks

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arxiv 1910.00567 v3 pith:2DEZPL2S submitted 2019-10-01 hep-ph astro-ph.COgr-qchep-thphysics.atom-ph

Probing Bosonic Stars with Atomic Clocks

classification hep-ph astro-ph.COgr-qchep-thphysics.atom-ph
keywords darkstarsatomicmatterasymmetricclocksbosonbosonic
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Dark Matter could potentially manifest itself in the form of asymmetric dark stars. In this paper we entertain the possibility of probing such asymmetric bosonic dark matter stars by the use of atomic clocks. If the dark sector connects to the standard model sector via a Higgs or photon portal, the interior of boson stars that are in a Bose-Einstein condensate state can change the values of physical constants that control the timing of atomic clock devices. Dilute asymmetric dark matter boson stars passing through the Earth can induce frequency shifts that can be observed in separated Earth based atomic clocks. This gives the opportunity to probe a class of dark matter candidates that for the moment cannot be detected with any different conventional method.

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Cited by 1 Pith paper

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  1. Quantum corrections as a Bound for Detecting Self-Interacting Ultralight Dark Matter

    hep-ph 2026-07 conditional novelty 5.0

    Radiative stability of the SIULDM potential under Yukawa couplings to SM fermions yields upper bounds on y that already intersect the projected reach of optical and nuclear clocks.