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...

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Main Authors: Matthew Baumgart, Nicholas L. Rodd, Tracy R. Slatyer, Varun Vaidya
Format: Article
Language:English
Published: SpringerOpen 2024-01-01
Series:Journal of High Energy Physics
Subjects:
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).
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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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