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The Sommerfeld enhancement for dark matter with an excited state

Open access
Slatyer, Tracy R·2010·Journal of Cosmology and Astroparticle Physics

Abstract

We present an analysis of the Sommerfeld enhancement to dark matter annihilation in the presence of an excited state, where the interaction inducing the enhancement is purely off-diagonal, such as in models of exciting or inelastic dark matter. We derive a simple and accurate semi-analytic approximation for the s -wave enhancement, which is valid provided the mass splitting between the ground and excited states is not too large, and discuss the cutoff of the enhancement for large mass splittings. We reproduce previously derived results in the appropriate limits, and demonstrate excellent agreement with numerical calculations of the enhancement. We show that the presence of an excited state leads to generically larger values of the Sommerfeld enhancement, larger resonances, and shifting of the resonances to lower mediator masses. Furthermore, in the presence of a mass splitting the enhancement is no longer a monotonic function of velocity: the enhancement where the kinetic energy is close to that required to excite the higher state can be up to twice as large as the enhancement at zero velocity.

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Metadata

Authors
Slatyer, T. R.
Venue
Journal of Cosmology and Astroparticle Physics
Published
2010-02-22
Volume
2010
Issue
02
Pages
028-028
ISSN
  • 1475-7508 (ISSN-L)
  • 1475-7516
OpenAlex
W2157379494
Cited by
165
References
3
FWCI
5.80
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The Sommerfeld enhancement for dark matter with an excited state. https://app.cochat.ai/papers/10.1088/1475-7516/2010/02/028
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Slatyer, T. R. (2010). The Sommerfeld enhancement for dark matter with an excited state. Journal of Cosmology and Astroparticle Physics. https://doi.org/10.1088/1475-7516/2010/02/028

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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