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Cited by 221

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Opening the window on strongly interacting dark matter

Starkman, Glenn D., Gould, Andrew, Esmailzadeh, Rahim, Dimopoulos, Savas·1990·Physical Review D

Abstract

We discuss the possibility that the dark matter consists of strongly interacting massive particles (SIMP's) which have cross sections with ordinary matter which are larger than characteristic weak-interaction cross sections. We show that, while results from $\ensuremath{\beta}\ensuremath{\beta}$ decay, cosmic-ray detectors, galactic-halo stability, the cooling of molecular clouds, proton-decay detectors, and the existence of old neutron stars and the Earth constrain the interactions of the missing matter with ordinary matter over a broad range of parameter space, there still exist several windows for SIMP's. It is noteworthy that there are two regions of less than geometric cross sections: one with masses of ${10}^{5}$-${10}^{7}$ GeV and another with masses above ${10}^{10}$ GeV.

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Crossref · 10.1103/physrevd.41.3594

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Metadata

Authors
Starkman, G. D., Gould, A., Esmailzadeh, R., & Dimopoulos, S.
Venue
Physical Review D
Published
1990-06-15
Volume
41
Issue
12
Pages
3594-3603
ISSN
0556-2821 (ISSN-L)
OpenAlex
W2051180132
Cited by
221
References
1
FWCI
1.78
Type
journal article
Language
en
Open access
closed

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