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Cited by 470

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Non-perturbative effect on thermal relic abundance of dark matter

Open access
Hisano, Junji, Matsumot, Shigeki, Nagai, Minoru, Saito, Osamu, Senami, Masato·2007·Physics Letters B

Abstract

We point out that thermal relic abundance of dark matter is strongly altered by a non‐perturbative effect called the Sommerfeld enhancement, when constituent particles of the dark matter are SU(2)L non‐singlet and much heavier than the weak gauge bosons. Typical candidates are the heavy wino and higgsino. We investigate the non‐perturbative effect on the relic abundance of dark matter for the wino as an example. We show that its thermal abundance is reduced by 50% compared to the perturbative result. The wino mass consistent with the observed dark matter abundance turns out to be 2.7 TeV

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Metadata

Authors
Hisano, J., Matsumot, S., Nagai, M., Saito, O., & Senami, M.
Venue
Physics Letters B
Publisher
Elsevier BV
Published
2007-03
Volume
646
Issue
1
Pages
34-38
ISSN
0370-2693 (ISSN-L)
OpenAlex
W2010273876
Cited by
470
References
4
FWCI
13.37
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Non-perturbative effect on thermal relic abundance of dark matter. https://app.cochat.ai/papers/10.1016/j.physletb.2007.01.012
The paper
Hisano, J., Matsumot, S., Nagai, M., Saito, O., & Senami, M. (2007). Non-perturbative effect on thermal relic abundance of dark matter. Physics Letters B. https://doi.org/10.1016/j.physletb.2007.01.012

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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.