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Cited by 543

The DOI matches its Crossref record; 40 of the 40 references it cites were found in a registry or an index.

Astrophysical signatures of secluded dark matter

Open access
Pospelov, Maxim, Ritz, Adam·2009·Physics Letters B

Abstract

We analyze the indirect astrophysical signatures of secluded models of WIMP dark matter, characterized by a weak-scale rate for annihilation into light MeV-scale mediators which are metastable to decay into Standard Model states. Such scenarios allow a significant enhancement of the annihilation cross section in the galactic halo relative to its value at freeze-out, particularly when the mediator is light enough for this process to proceed through radiative capture to a metastable ‘WIMP-onium’ bound state. For MeV-scale vector mediators charged under a hidden U(1)′ gauge group, the enhanced annihilation rate leads predominantly to a sizable excess positron flux, even in the absence of astrophysical boost factors.

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Crossref · 10.1016/j.physletb.2008.12.012

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Metadata

Authors
Pospelov, M., & Ritz, A.
Venue
Physics Letters B
Publisher
Elsevier BV
Published
2009-01
Volume
671
Issue
3
Pages
391-397
ISSN
0370-2693 (ISSN-L)
OpenAlex
W1988409168
Cited by
543
References
40
FWCI
28.75
Type
journal article
Language
en
Open access
hybrid

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CoChat. (2026). Citation check: Astrophysical signatures of secluded dark matter. https://app.cochat.ai/papers/10.1016/j.physletb.2008.12.012
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Pospelov, M., & Ritz, A. (2009). Astrophysical signatures of secluded dark matter. Physics Letters B. https://doi.org/10.1016/j.physletb.2008.12.012

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

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

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.