Spontaneous dark-matter mass generation along cosmological attractors in string theory
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Coudarchet2019_Article_Spontan ...
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Affiliation
Univ Arizona, Dept PhysIssue Date
2019-03-20Keywords
Cosmology of Theories beyond the SMSuperstrings and Heterotic Strings
Supersymmetry Breaking
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SPRINGERCitation
Coudarchet, T., Heurtier, L. & Partouche, H. J. High Energ. Phys. (2019) 2019: 117. https://doi.org/10.1007/JHEP03(2019)117Journal
JOURNAL OF HIGH ENERGY PHYSICSRights
© The Author(s) 2019.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
We propose a new scenario for generating a relic density of non-relativistic dark matter in the context of heterotic string theory. Contrary to standard thermal freeze-out scenarios, dark-matter particles are abundantly produced while still relativistic, and then decouple from the thermal bath due to the sudden increase of their mass above the universe temperature. This mass variation is sourced by the condensation of an order-parameter modulus, which is triggered when the temperature T (t) drops below the supersymmetry breaking scale M (t), which are both time-dependent. A cosmological attractor mechanism forces this phase transition to take place, in an explicit class of heterotic string models with spontaneously broken supersymmetry, and at finite temperature.Note
Open access journalISSN
1029-8479Version
Final published versionSponsors
Department of Energy [DE-FG02-13ER41976/DE-SC0009913]; CNRS; Royal Society International Cost Share AwardAdditional Links
https://link.springer.com/article/10.1007/JHEP03(2019)117ae974a485f413a2113503eed53cd6c53
10.1007/jhep03(2019)117
