Thermal squeezeout of dark matter

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....

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Main Authors: Asadi, Pouya, Kramer, Eric David, Kuflik, Eric, Ridgway, Gregory W, Slatyer, Tracy R, Smirnov, Juri
Other Authors: Massachusetts Institute of Technology. Center for Theoretical Physics
Format: Article
Language:English
Published: American Physical Society (APS) 2022
Online Access:https://hdl.handle.net/1721.1/142224
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author Asadi, Pouya
Kramer, Eric David
Kuflik, Eric
Ridgway, Gregory W
Slatyer, Tracy R
Smirnov, Juri
author2 Massachusetts Institute of Technology. Center for Theoretical Physics
author_facet Massachusetts Institute of Technology. Center for Theoretical Physics
Asadi, Pouya
Kramer, Eric David
Kuflik, Eric
Ridgway, Gregory W
Slatyer, Tracy R
Smirnov, Juri
author_sort Asadi, Pouya
collection MIT
description 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.
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spelling mit-1721.1/1422242023-12-07T14:37:52Z Thermal squeezeout of dark matter Asadi, Pouya Kramer, Eric David Kuflik, Eric Ridgway, Gregory W Slatyer, Tracy R Smirnov, Juri Massachusetts Institute of Technology. Center for Theoretical Physics 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. 2022-05-02T13:56:07Z 2022-05-02T13:56:07Z 2021 2022-05-02T13:04:35Z Article http://purl.org/eprint/type/JournalArticle https://hdl.handle.net/1721.1/142224 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). en 10.1103/PHYSREVD.104.095013 Physical Review D Creative Commons Attribution 4.0 International License https://creativecommons.org/licenses/by/4.0 application/pdf American Physical Society (APS) APS
spellingShingle Asadi, Pouya
Kramer, Eric David
Kuflik, Eric
Ridgway, Gregory W
Slatyer, Tracy R
Smirnov, Juri
Thermal squeezeout of dark matter
title Thermal squeezeout of dark matter
title_full Thermal squeezeout of dark matter
title_fullStr Thermal squeezeout of dark matter
title_full_unstemmed Thermal squeezeout of dark matter
title_short Thermal squeezeout of dark matter
title_sort thermal squeezeout of dark matter
url https://hdl.handle.net/1721.1/142224
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