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Cited by 182

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Low Reheating Temperature and the Visible Sterile Neutrino

Open access
Gelmini, Graciela, Palomares-Ruiz, Sergio, Pascoli, Silvia·2004·Physical Review Letters

Abstract

We present here a scenario, based on a low reheating temperature T(R)<<100 MeV at the end of (the last episode of) inflation, in which the coupling of sterile neutrinos to active neutrinos can be as large as experimental bounds permit (thus making this neutrino "visible" in future experiments). In previous models this coupling was forced to be very small to prevent a cosmological overabundance of sterile neutrinos. Here the abundance depends on how low the reheating temperature is. For example, the sterile neutrino required by the Liquid Scintillator Neutrino Detector result may not have any cosmological problem within our scenario.

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Metadata

Authors
Gelmini, G., Palomares-Ruiz, S., & Pascoli, S.
Venue
Physical Review Letters
Published
2004-08-20
Volume
93
Issue
8
Pages
081302-081302
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2009626955
Cited by
182
References
2
FWCI
8.91
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Low Reheating Temperature and the Visible Sterile Neutrino. https://app.cochat.ai/papers/10.1103/physrevlett.93.081302
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Gelmini, G., Palomares-Ruiz, S., & Pascoli, S. (2004). Low Reheating Temperature and the Visible Sterile Neutrino. Physical Review Letters. https://doi.org/10.1103/physrevlett.93.081302

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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.