Deciphering the archaeological record: Cosmological imprints of nonminimal dark sectors
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PhysRevD.101.123511.pdf
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AMER PHYSICAL SOCCitation
Dienes, K., Huang, F., Kost, J., Su, S., & Thomas, B. (2020). Deciphering the archaeological record: Cosmological imprints of nonminimal dark sectors. Physical Review D, 101(12). doi: 10.1103/physrevd.101.123511Journal
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Copyright © 2020 American Physical Society.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
Many proposals for physics beyond the Standard Model give rise to a dark sector containing many degrees of freedom. In this work, we exploit the cosmological implications of the nontrivial dynamics which may arise within such dark sectors, focusing on decay processes which take place entirely among the dark constituents. First, we demonstrate that such decays can leave dramatic imprints on the resulting dark-matter phase-space distribution. In particular, this distribution need not be thermal-it can even be multimodal, exhibiting a nontrivial pattern of peaks and troughs as a function of momentum. We then proceed to show how these features can induce modifications to the matter power spectrum. Finally, we assess the extent to which one can approach the archaeological "inverse" problem of deciphering the properties of an underlying dark sector from the matter power spectrum. Indeed, one of the main results of this paper is a remarkably simple conjectured analytic expression which permits the reconstruction of many of the important features of the dark-matter phase-space distribution directly from the matter power spectrum. Our results therefore provide an interesting toolbox of methods for learning about, and potentially constraining, the features of nonminimal dark sectors and their dynamics in the early universe.ISSN
1550-7998Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1103/physrevd.101.123511
