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Scattering of dark pions in Sp(4) gauge theory
Physical Review D, Volume: 110, Issue: 5
Swansea University Author: Fabian Zierler
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DOI (Published version): 10.1103/physrevd.110.054513
Abstract
Analyses of astrophysical data provide first hints on the self-interactions of dark matter at low energies. Lattice calculations of dark matter theories can be used to investigate them, especially in the case of strongly-interacting dark matter. We consider Sp(4) gauge theory with two fundamental fe...
Published in: | Physical Review D |
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ISSN: | 2470-0010 2470-0029 |
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American Physical Society (APS)
2024
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URI: | https://cronfa.swan.ac.uk/Record/cronfa67451 |
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2024-12-03T13:49:29.1415728 v2 67451 2024-08-22 Scattering of dark pions in Sp(4) gauge theory 7eb526fdce1693fc0b79f33e74cc182d Fabian Zierler Fabian Zierler true false 2024-08-22 BGPS Analyses of astrophysical data provide first hints on the self-interactions of dark matter at low energies. Lattice calculations of dark matter theories can be used to investigate them, especially in the case of strongly-interacting dark matter. We consider Sp(4) gauge theory with two fundamental fermions as a candidate theory. We compute the scattering phase shift for the scattering of two identical dark pions and determine the parameters of the effective range expansion. Our exploratory results in the supposedly most common interaction channel provide a lower limit for the dark matter mass when compared to astrophysical data. We also provide first benchmarks of velocity-weighted cross-sections in the relevant non-relativistic domain. Journal Article Physical Review D 110 5 American Physical Society (APS) 2470-0010 2470-0029 Composite models, dark matter, lattice QCD, Lattice field theory, particle dark matter, phase shift, strong interaction, gravitation, cosmology, astrophysics 23 9 2024 2024-09-23 10.1103/physrevd.110.054513 COLLEGE NANME Biosciences Geography and Physics School COLLEGE CODE BGPS Swansea University SU Library paid the OA fee (TA Institutional Deal) Funded by SCOAP3 2024-12-03T13:49:29.1415728 2024-08-22T16:06:47.7791341 Faculty of Science and Engineering School of Biosciences, Geography and Physics - Physics Yannick Dengler 0000-0002-2305-8868 1 Axel Maas 0000-0002-4621-2151 2 Fabian Zierler 3 67451__31468__a1dde6b5fc0b457a952dcfa9a7082a5c.pdf 67451.vor.pdf 2024-09-26T16:39:17.7964376 Output 1045414 application/pdf Version of Record true Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. true eng https://creativecommons.org/licenses/by/4.0/ 266 Fabian Zierler 0000-0002-8670-4054 fabian.zierler@swansea.ac.uk true https://doi.org/10.5281/zenodo.12920978 false |
title |
Scattering of dark pions in Sp(4) gauge theory |
spellingShingle |
Scattering of dark pions in Sp(4) gauge theory Fabian Zierler |
title_short |
Scattering of dark pions in Sp(4) gauge theory |
title_full |
Scattering of dark pions in Sp(4) gauge theory |
title_fullStr |
Scattering of dark pions in Sp(4) gauge theory |
title_full_unstemmed |
Scattering of dark pions in Sp(4) gauge theory |
title_sort |
Scattering of dark pions in Sp(4) gauge theory |
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7eb526fdce1693fc0b79f33e74cc182d |
author_id_fullname_str_mv |
7eb526fdce1693fc0b79f33e74cc182d_***_Fabian Zierler |
author |
Fabian Zierler |
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Yannick Dengler Axel Maas Fabian Zierler |
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Journal article |
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Physical Review D |
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110 |
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5 |
publishDate |
2024 |
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Swansea University |
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2470-0010 2470-0029 |
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10.1103/physrevd.110.054513 |
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American Physical Society (APS) |
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Faculty of Science and Engineering |
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Faculty of Science and Engineering |
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description |
Analyses of astrophysical data provide first hints on the self-interactions of dark matter at low energies. Lattice calculations of dark matter theories can be used to investigate them, especially in the case of strongly-interacting dark matter. We consider Sp(4) gauge theory with two fundamental fermions as a candidate theory. We compute the scattering phase shift for the scattering of two identical dark pions and determine the parameters of the effective range expansion. Our exploratory results in the supposedly most common interaction channel provide a lower limit for the dark matter mass when compared to astrophysical data. We also provide first benchmarks of velocity-weighted cross-sections in the relevant non-relativistic domain. |
published_date |
2024-09-23T09:28:20Z |
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11.055693 |