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High Energy Physics - Phenomenology

Title: Asymmetric Reheating via Inverse Symmetry Breaking

Abstract: Asymmetric reheating is a generic requirement for models of dark sectors with light species, but its implementation is usually in tension with unique phenomenologies otherwise possible in compelling theories containing dark copies of the Standard Model. We present a simple module to implement asymmetric reheating during a $\mathbb{Z}_2$-breaking phase above some critical temperature. This reinvigorates the possibility of an exactly degenerate mirror sector and the striking phenomenology of composite particles oscillating into their mirror counterparts.
Comments: 8 pages, 4 figures; v3: accepted for publication in PRD
Subjects: High Energy Physics - Phenomenology (hep-ph); Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Cite as: arXiv:2211.13212 [hep-ph]
  (or arXiv:2211.13212v3 [hep-ph] for this version)

Submission history

From: Aurora Ireland [view email]
[v1] Wed, 23 Nov 2022 18:54:07 GMT (2932kb,D)
[v2] Wed, 6 Sep 2023 00:11:55 GMT (2942kb,D)
[v3] Wed, 24 Apr 2024 04:23:33 GMT (3039kb,D)

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