• Open Access

Probing bosonic stars with atomic clocks

Chris Kouvaris, Eleftherios Papantonopoulos, Lauren Street, and L. C. R. Wijewardhana
Phys. Rev. D 102, 063014 – Published 14 September 2020

Abstract

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 interiors 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.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
4 More
  • Received 2 April 2020
  • Accepted 18 August 2020

DOI:https://doi.org/10.1103/PhysRevD.102.063014

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & FieldsAtomic, Molecular & Optical

Authors & Affiliations

Chris Kouvaris*

  • CP3-Origins, Centre for Cosmology and Particle Physics Phenomenology, University of Southern Denmark, Campusvej 55, 5230 Odense M, Denmark, and Theoretical Physics Department, CERN, 1211 Geneva, Switzerland

Eleftherios Papantonopoulos

  • National Technical University of Athens, Zografou Campus 9, Heroon Polytechneiou Street 157 80 Athens, Greece

Lauren Street and L. C. R. Wijewardhana§

  • University of Cincinnati, Department of Physics, Cincinnati, Ohio 45221, USA

  • *kouvaris@cp3.sdu.dk
  • lpapa@central.ntua.gr
  • streetlg@mail.uc.edu
  • §rohana.wijewardhana@gmail.com

Article Text

Click to Expand

References

Click to Expand
Issue

Vol. 102, Iss. 6 — 15 September 2020

Reuse & Permissions
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

×

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×