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Matter asymmetry sourced dark matter

Alonso, Rodrigo; Scholtz, Jakub

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Authors

Jakub Scholtz



Abstract

We investigate the possibility that the dark matter abundance is sourced by the baryon/lepton asymmetry of the early Universe. It turns out that a Goldstone field of a global classically preserved symmetry in the Standard Model experiences a kick during a period of baryon/lepton number generation. This mechanism can be regarded as dynamical generation of initial conditions for misalignment yet the prediction for relic abundance presents an inverse dependence on the coupling in parallel with freeze-in vs freeze-out. We explore two realizations of this mechanism and show that in conjunction with leptogenesis, it is possible to identify a viable promising region of parameter space for dark matter production with mass 10 MeV–1 GeV and decay constant f in the range of 10 10 – 10 12     GeV

Citation

Alonso, R., & Scholtz, J. (2021). Matter asymmetry sourced dark matter. Physical Review D, 104(2), Article 023513. https://doi.org/10.1103/physrevd.104.023513

Journal Article Type Article
Acceptance Date Jun 12, 2021
Online Publication Date Jul 12, 2021
Publication Date Jul 15, 2021
Deposit Date Oct 25, 2021
Publicly Available Date Oct 26, 2021
Journal Physical Review D
Print ISSN 2470-0010
Electronic ISSN 2470-0029
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 104
Issue 2
Article Number 023513
DOI https://doi.org/10.1103/physrevd.104.023513
Public URL https://durham-repository.worktribe.com/output/1225615

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Published Journal Article (692 Kb)
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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
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.





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