Enhanced n-body annihilation of dark matter and its indirect signatures

Abstract We examine the possible indirect signatures of dark matter annihilation processes with a non-standard scaling with the dark matter density, and in particular the case where more than two dark matter particles participate in the annihilation process. We point out that such processes can be s...

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Main Authors: Mohammad Hossein Namjoo, Tracy R. Slatyer, Chih-Liang Wu
Format: Article
Language:English
Published: SpringerOpen 2019-03-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP03(2019)077
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spelling doaj-5682094106ca4c3197745dfc40c1f9c32020-11-25T02:51:12ZengSpringerOpenJournal of High Energy Physics1029-84792019-03-012019316610.1007/JHEP03(2019)077Enhanced n-body annihilation of dark matter and its indirect signaturesMohammad Hossein Namjoo0Tracy R. Slatyer1Chih-Liang Wu2Center for Theoretical Physics, Massachusetts Institute of TechnologyCenter for Theoretical Physics, Massachusetts Institute of TechnologyCenter for Theoretical Physics, Massachusetts Institute of TechnologyAbstract We examine the possible indirect signatures of dark matter annihilation processes with a non-standard scaling with the dark matter density, and in particular the case where more than two dark matter particles participate in the annihilation process. We point out that such processes can be strongly enhanced at low velocities without violating unitarity, similar to Sommerfeld enhancement in the standard case of two-body annihilation, potentially leading to visible signals in indirect searches. We study in detail the impact of such multi-body annihilations on the ionization history of the universe and consequently the cosmic microwave background, and find that unlike in the two-body case, the dominant signal can naturally arise from the end of the cosmic dark ages, after the onset of structure formation. We examine the complementary constraints from the Galactic Center, Galactic halo, and galaxy clusters, and outline the circumstances under which each search would give rise to the strongest constraints. We also show that if there is a population of ultra-compact dense dark matter clumps present in the Milky Way with sufficiently steep density profile, then it might be possible to detect point sources illuminated by multi-body annihilation, even if there is no large low-velocity enhancement. Finally, we provide a case study of a model where 3-body annihilation dominates the freezeout process, and in particular the resonant regime where a large low-velocity enhancement is naturally generated.http://link.springer.com/article/10.1007/JHEP03(2019)077Beyond Standard ModelCosmology of Theories beyond the SM
collection DOAJ
language English
format Article
sources DOAJ
author Mohammad Hossein Namjoo
Tracy R. Slatyer
Chih-Liang Wu
spellingShingle Mohammad Hossein Namjoo
Tracy R. Slatyer
Chih-Liang Wu
Enhanced n-body annihilation of dark matter and its indirect signatures
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
author_facet Mohammad Hossein Namjoo
Tracy R. Slatyer
Chih-Liang Wu
author_sort Mohammad Hossein Namjoo
title Enhanced n-body annihilation of dark matter and its indirect signatures
title_short Enhanced n-body annihilation of dark matter and its indirect signatures
title_full Enhanced n-body annihilation of dark matter and its indirect signatures
title_fullStr Enhanced n-body annihilation of dark matter and its indirect signatures
title_full_unstemmed Enhanced n-body annihilation of dark matter and its indirect signatures
title_sort enhanced n-body annihilation of dark matter and its indirect signatures
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2019-03-01
description Abstract We examine the possible indirect signatures of dark matter annihilation processes with a non-standard scaling with the dark matter density, and in particular the case where more than two dark matter particles participate in the annihilation process. We point out that such processes can be strongly enhanced at low velocities without violating unitarity, similar to Sommerfeld enhancement in the standard case of two-body annihilation, potentially leading to visible signals in indirect searches. We study in detail the impact of such multi-body annihilations on the ionization history of the universe and consequently the cosmic microwave background, and find that unlike in the two-body case, the dominant signal can naturally arise from the end of the cosmic dark ages, after the onset of structure formation. We examine the complementary constraints from the Galactic Center, Galactic halo, and galaxy clusters, and outline the circumstances under which each search would give rise to the strongest constraints. We also show that if there is a population of ultra-compact dense dark matter clumps present in the Milky Way with sufficiently steep density profile, then it might be possible to detect point sources illuminated by multi-body annihilation, even if there is no large low-velocity enhancement. Finally, we provide a case study of a model where 3-body annihilation dominates the freezeout process, and in particular the resonant regime where a large low-velocity enhancement is naturally generated.
topic Beyond Standard Model
Cosmology of Theories beyond the SM
url http://link.springer.com/article/10.1007/JHEP03(2019)077
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