Signature of relic heavy stable neutrinos in underground experiments

Fuente: arXiv
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Main Authors: Fargion, D., Khlopov, M. Yu., Konoplich, R. V., Mignani, R.
Format: Preprint
Published: 1998
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_version_ 1866914342465699840
author Fargion, D.
Khlopov, M. Yu.
Konoplich, R. V.
Mignani, R.
author_facet Fargion, D.
Khlopov, M. Yu.
Konoplich, R. V.
Mignani, R.
contents Considering heavy stable neutrinos of 4th generation we calculate the relic density of such neutrinos in the Universe. Taking into account the condensation of heavy neutrinos in the Galaxy and applying the results of calculations to experimental data from underground experiments on search for WIMPs in elastic neutral current scattering on nuclei we found an exclusion region of neutrino mass 60 GeV < m < 290 GeV. The bounds obtained from present underground experiments while confirming the previous bounds derived from analysis of cosmic ray spectra are more relible ones. We discuss also the first indication of elastic scattering induced by WIMP in DAMA experiment finding a very narrow window of neutrino mass 45 GeV < m < 50 GeV compatible with the possible signal rate in the detector.
format Preprint
id arxiv_https___arxiv_org_abs_astro_ph_9810048
institution arXiv
publishDate 1998
record_format arxiv
spellingShingle Signature of relic heavy stable neutrinos in underground experiments
Fargion, D.
Khlopov, M. Yu.
Konoplich, R. V.
Mignani, R.
Astrophysics
High Energy Physics - Phenomenology
Considering heavy stable neutrinos of 4th generation we calculate the relic density of such neutrinos in the Universe. Taking into account the condensation of heavy neutrinos in the Galaxy and applying the results of calculations to experimental data from underground experiments on search for WIMPs in elastic neutral current scattering on nuclei we found an exclusion region of neutrino mass 60 GeV < m < 290 GeV. The bounds obtained from present underground experiments while confirming the previous bounds derived from analysis of cosmic ray spectra are more relible ones. We discuss also the first indication of elastic scattering induced by WIMP in DAMA experiment finding a very narrow window of neutrino mass 45 GeV < m < 50 GeV compatible with the possible signal rate in the detector.
title Signature of relic heavy stable neutrinos in underground experiments
topic Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/astro-ph/9810048