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Thermal squeezeout of dark matter

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PhysRevD.104.095013.pdf

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sword-2022-05-02T13:04:35.original.xml (130 B)
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Author(s)
Asadi, Pouya
•
Kramer, Eric David
•
Kuflik, Eric
•
Ridgway, Gregory W
•
Slatyer, Tracy R
•
Smirnov, Juri
Date Issued
2021
Journal
Physical Review D
Publisher
American Physical Society (APS)
Citation
Asadi, Pouya, Kramer, Eric David, Kuflik, Eric, Ridgway, Gregory W, Slatyer, Tracy R et al. 2021. "Thermal squeezeout of dark matter." Physical Review D, 104 (9).
Version
Final published version
Abstract
We carry out a detailed study of the confinement phase transition in a dark sector with a $SU(N)$ gauge group and a single generation of dark heavy quark. We focus on heavy enough quarks such that their abundance freezes out before the phase transition and the phase transition is of first-order. We find that during this phase transition the quarks are trapped inside contracting pockets of the deconfined phase and are compressed enough to interact at a significant rate, giving rise to a second stage of annihilation that can dramatically change the resulting dark matter abundance. As a result, the dark matter can be heavier than the often-quoted unitarity bound of $\sim100~$TeV. Our findings are almost completely independent of the details of the portal between the dark sector and the Standard Model. We comment briefly on possible signals of such a sector. Our main findings are summarized in a companion letter, while here we provide further details on different parts of the calculation.
MIT Department
Massachusetts Institute of Technology. Center for Theoretical Physics
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Creative Commons Attribution 4.0 International License
https://creativecommons.org/licenses/by/4.0
Persistent DSpace Link
https://hdl.handle.net/1721.1/142224
DOI of Published Version
https://doi.org/10.1103/PHYSREVD.104.095013
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