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arXiv · 2006.08359

Neutrino Cooling of Primordial Hot Regions

K. M. Belotsky·S. G. Rubin·M. M. Elkasemy
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Abstract

The effect of neutrino cooling of possible primary regions filled by the hot matter is discussed. Such regions could contain the primordial density inhomogeneities of different origin and survive up to modern epoch. We show that the final temperature of such region is $\sim 10\, {\rm keV}$ provided that the initial temperature is within the interval $10\, {\rm keV} ... 100\, {\rm MeV}$. The cooling is realized due to the nuclear reactions containing $n-p$ transition. The lower limit $10\, {\rm keV}$ is accounted for by suppression of the reactions rates because of threshold effect and $n$, $e^{\pm}$ density diminishment.

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K. M. Belotsky, S. G. Rubin, M. M. Elkasemy. 2020-06-11. Neutrino Cooling of Primordial Hot Regions. https://doi.org/10.3390/sym12091442

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