The quintuplet annihilation spectrum
Abstract We extend the Effective Field Theory of Heavy Dark Matter to arbitrary odd representations of SU(2) and incorporate the effects of bound states. This formalism is then deployed to compute the gamma-ray spectrum for a 5 of SU(2): quintuplet dark matter. Except at isolated values of the quint...
Main Authors: | , , , |
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Format: | Article |
Language: | English |
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SpringerOpen
2024-01-01
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Series: | Journal of High Energy Physics |
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Online Access: | https://doi.org/10.1007/JHEP01(2024)158 |
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author | Matthew Baumgart Nicholas L. Rodd Tracy R. Slatyer Varun Vaidya |
author_facet | Matthew Baumgart Nicholas L. Rodd Tracy R. Slatyer Varun Vaidya |
author_sort | Matthew Baumgart |
collection | DOAJ |
description | Abstract We extend the Effective Field Theory of Heavy Dark Matter to arbitrary odd representations of SU(2) and incorporate the effects of bound states. This formalism is then deployed to compute the gamma-ray spectrum for a 5 of SU(2): quintuplet dark matter. Except at isolated values of the quintuplet mass, the bound state contribution to hard photons with energy near the dark-matter mass is at the level of a few percent compared to that from direct annihilation. Further, compared to smaller representations, such as the triplet wino, the quintuplet can exhibit a strong variation in the shape of the spectrum as a function of mass. Using our results, we forecast the fate of the thermal quintuplet, which has a mass of ~13.6 TeV. We find that existing H.E.S.S. data should be able to significantly test the scenario, however, the final word on this canonical model of minimal dark matter will likely be left to the Cherenkov Telescope Array (CTA). |
first_indexed | 2024-03-07T15:24:00Z |
format | Article |
id | doaj.art-8aefd77ebefa4b4c9688c2603335eba3 |
institution | Directory Open Access Journal |
issn | 1029-8479 |
language | English |
last_indexed | 2024-03-07T15:24:00Z |
publishDate | 2024-01-01 |
publisher | SpringerOpen |
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series | Journal of High Energy Physics |
spelling | doaj.art-8aefd77ebefa4b4c9688c2603335eba32024-03-05T17:26:50ZengSpringerOpenJournal of High Energy Physics1029-84792024-01-012024118010.1007/JHEP01(2024)158The quintuplet annihilation spectrumMatthew Baumgart0Nicholas L. Rodd1Tracy R. Slatyer2Varun Vaidya3Department of Physics, Arizona State UniversityTheoretical Physics Department, CERNCenter for Theoretical Physics, Massachusetts Institute of TechnologyDepartment of Physics, University of South DakotaAbstract We extend the Effective Field Theory of Heavy Dark Matter to arbitrary odd representations of SU(2) and incorporate the effects of bound states. This formalism is then deployed to compute the gamma-ray spectrum for a 5 of SU(2): quintuplet dark matter. Except at isolated values of the quintuplet mass, the bound state contribution to hard photons with energy near the dark-matter mass is at the level of a few percent compared to that from direct annihilation. Further, compared to smaller representations, such as the triplet wino, the quintuplet can exhibit a strong variation in the shape of the spectrum as a function of mass. Using our results, we forecast the fate of the thermal quintuplet, which has a mass of ~13.6 TeV. We find that existing H.E.S.S. data should be able to significantly test the scenario, however, the final word on this canonical model of minimal dark matter will likely be left to the Cherenkov Telescope Array (CTA).https://doi.org/10.1007/JHEP01(2024)158Models for Dark MatterParticle Nature of Dark Matter |
spellingShingle | Matthew Baumgart Nicholas L. Rodd Tracy R. Slatyer Varun Vaidya The quintuplet annihilation spectrum Journal of High Energy Physics Models for Dark Matter Particle Nature of Dark Matter |
title | The quintuplet annihilation spectrum |
title_full | The quintuplet annihilation spectrum |
title_fullStr | The quintuplet annihilation spectrum |
title_full_unstemmed | The quintuplet annihilation spectrum |
title_short | The quintuplet annihilation spectrum |
title_sort | quintuplet annihilation spectrum |
topic | Models for Dark Matter Particle Nature of Dark Matter |
url | https://doi.org/10.1007/JHEP01(2024)158 |
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