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Bounds on very low reheating scenarios after Planck

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de Salas, P. F., Lattanzi, M., Mangano, G., Miele, G., Pastor, S., Pisanti, O.·2015·Physical Review D

Abstract

We consider the case of very low reheating scenarios [${T}_{\mathrm{RH}}\ensuremath{\sim}\mathcal{O}(\mathrm{MeV})$] with a better calculation of the production of the relic neutrino background (with three-flavor oscillations). At 95% confidence level, a lower bound on the reheating temperature ${T}_{\mathrm{RH}}>4.1\text{ }\text{ }\mathrm{MeV}$ is obtained from big bang nucleosynthesis, while ${T}_{\mathrm{RH}}>4.7\text{ }\text{ }\mathrm{MeV}$ from Planck data (allowing neutrino masses to vary), the most stringent bound on the reheating temperature to date. Neutrino masses as large as 1 eV are possible for very low reheating temperatures.

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Metadata

Authors
de Salas, P. F., Lattanzi, M., Mangano, G., Miele, G., Pastor, S., & Pisanti, O.
Venue
Physical Review D
Published
2015-12-23
Volume
92
Issue
12
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W1947481790
Cited by
321
References
31
FWCI
6.56
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Bounds on very low reheating scenarios after Planck. https://app.cochat.ai/papers/10.1103/physrevd.92.123534
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de Salas, P. F., Lattanzi, M., Mangano, G., Miele, G., Pastor, S., & Pisanti, O. (2015). Bounds on very low reheating scenarios after Planck. Physical Review D. https://doi.org/10.1103/physrevd.92.123534

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