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.
| Original language | English |
|---|---|
| Article number | 063014 |
| Journal | Physical Review D |
| Volume | 102 |
| Issue number | 6 |
| Number of pages | 15 |
| ISSN | 2470-0010 |
| DOIs | |
| Publication status | Published - 15. Sept 2020 |
Funding
We thank Professor Kelin Gao for the numerous discussions we had on atomic clocks and the vital information he provided to us on the setup and precision of the atomic clocks of his lab. We are grateful to Joshua Eby, Jared Evans, and Peter Suranyi for many valuable discussions. L. S. and L. C. R. W. thank the University of Cincinnati Office of Research Faculty Bridge Program for funding through the Faculty Bridge Grant. L. C. R. W. thanks the Aspen Center for Physics, which is supported by National Science Foundation Grant No. PHY-1607611, where some of the research was conducted. C. K. is partially funded by the Danish National Research Foundation, Grant No. DNRF90, and by the Danish Council for Independent Research, Grant No. DFF 4181-00055.
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