NAGIOS: RODERIC FUNCIONANDO

Ghost particles in the universe : neutrinos in astrophysics and cosmology

Repositori DSpace/Manakin

dc.contributor.author	Raffelt, Georg	es
dc.date.accessioned	2021-06-15T08:01:39Z
dc.date.available	2021-06-15T08:01:39Z
dc.date.issued	2017	es
dc.identifier.citation	Raffelt, Georg. Ghost particles in the universe : neutrinos in astrophysics and cosmology. En: Mètode Science Studies Journal: Annual Review, 7 2017: 190-199	es
dc.identifier.uri	https://hdl.handle.net/10550/79710
dc.description.abstract	Neutrinos are nearly massless and very difficult to detect because they interact so very weakly. Sixty years after seeing the first of these «ghost particles» we know a lot about their properties. Today, observing them in nuclear reactors, the Sun, the Earth?s crust and atmosphere, and at high energies from distant cosmic sources is almost a routine task ? they have become unique astrophysical messengers. They are important for a number of aspects: neutrinos shape some of the most dramatic astrophysical phenomena in the form of stellar-collapse supernova explosions, they may have created the excess of matter over antimatter in the universe, and neutrino-like «weakly interacting massive particles» may well account for the dark matter of the universe.	es
dc.title	Ghost particles in the universe : neutrinos in astrophysics and cosmology	es
dc.type	journal article	es_ES
dc.subject.unesco		es
dc.identifier.doi		es
dc.type.hasVersion	VoR	es_ES