Gravitational clustering of cosmic relic neutrinos in the Milky Way
In order to detect relic neutrinos in the vicinity of the Earth, quantitative knowledge of the gravitational clustering effects on cosmic relic neutrinos in the Milky Way is necessary. Here, the authors develop a computational method capable of yielding neutrino density profiles for different neutri...
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2018-05-01
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Online Access: | https://doi.org/10.1038/s41467-018-04264-y |
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doaj-277db55de1d844df950f03dec8cc57f22021-05-11T09:56:03ZengNature Publishing GroupNature Communications2041-17232018-05-01911710.1038/s41467-018-04264-yGravitational clustering of cosmic relic neutrinos in the Milky WayJue Zhang0Xin Zhang1Center for High Energy Physics, Peking UniversityDepartment of Physics, College of Sciences, Northeastern UniversityIn order to detect relic neutrinos in the vicinity of the Earth, quantitative knowledge of the gravitational clustering effects on cosmic relic neutrinos in the Milky Way is necessary. Here, the authors develop a computational method capable of yielding neutrino density profiles for different neutrino masses and phase space distributions in a single simulation.https://doi.org/10.1038/s41467-018-04264-y |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Jue Zhang Xin Zhang |
spellingShingle |
Jue Zhang Xin Zhang Gravitational clustering of cosmic relic neutrinos in the Milky Way Nature Communications |
author_facet |
Jue Zhang Xin Zhang |
author_sort |
Jue Zhang |
title |
Gravitational clustering of cosmic relic neutrinos in the Milky Way |
title_short |
Gravitational clustering of cosmic relic neutrinos in the Milky Way |
title_full |
Gravitational clustering of cosmic relic neutrinos in the Milky Way |
title_fullStr |
Gravitational clustering of cosmic relic neutrinos in the Milky Way |
title_full_unstemmed |
Gravitational clustering of cosmic relic neutrinos in the Milky Way |
title_sort |
gravitational clustering of cosmic relic neutrinos in the milky way |
publisher |
Nature Publishing Group |
series |
Nature Communications |
issn |
2041-1723 |
publishDate |
2018-05-01 |
description |
In order to detect relic neutrinos in the vicinity of the Earth, quantitative knowledge of the gravitational clustering effects on cosmic relic neutrinos in the Milky Way is necessary. Here, the authors develop a computational method capable of yielding neutrino density profiles for different neutrino masses and phase space distributions in a single simulation. |
url |
https://doi.org/10.1038/s41467-018-04264-y |
work_keys_str_mv |
AT juezhang gravitationalclusteringofcosmicrelicneutrinosinthemilkyway AT xinzhang gravitationalclusteringofcosmicrelicneutrinosinthemilkyway |
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1721448917462155264 |