Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments

Despite being a well understood phenomenon in the context of current terrestrial experiments, neutrino flavor conversions in dense astrophysical environments probably represent one of the most challenging open problems in neutrino physics. Apart from being theoretically interesting, such a problem h...

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Main Authors: Francesco Capozzi, Ninetta Saviano
Format: Article
Language:English
Published: MDPI AG 2022-02-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/8/2/94
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author Francesco Capozzi
Ninetta Saviano
author_facet Francesco Capozzi
Ninetta Saviano
author_sort Francesco Capozzi
collection DOAJ
description Despite being a well understood phenomenon in the context of current terrestrial experiments, neutrino flavor conversions in dense astrophysical environments probably represent one of the most challenging open problems in neutrino physics. Apart from being theoretically interesting, such a problem has several phenomenological implications in cosmology and in astrophysics, including the primordial nucleosynthesis of light elements abundance and other cosmological observables, nucleosynthesis of heavy nuclei, and the explosion of massive stars. In this review, we briefly summarize the state of the art on this topic, focusing on three environments: early Universe, core-collapse supernovae, and compact binary mergers.
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spelling doaj.art-b98368c9e14542ef948c4fac0b94bc592023-11-23T22:23:16ZengMDPI AGUniverse2218-19972022-02-01829410.3390/universe8020094Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological EnvironmentsFrancesco Capozzi0Ninetta Saviano1Instituto de Física Corpuscular, Universidad de Valencia & CSIC, Edificio Institutos de Investigación, Calle Catedrático José Beltrán 2, 46980 Paterna, SpainScuola Superiore Meridionale, Università degli studi di Napoli “Federico II”, Largo San Marcellino 10, 80138 Napoli, ItalyDespite being a well understood phenomenon in the context of current terrestrial experiments, neutrino flavor conversions in dense astrophysical environments probably represent one of the most challenging open problems in neutrino physics. Apart from being theoretically interesting, such a problem has several phenomenological implications in cosmology and in astrophysics, including the primordial nucleosynthesis of light elements abundance and other cosmological observables, nucleosynthesis of heavy nuclei, and the explosion of massive stars. In this review, we briefly summarize the state of the art on this topic, focusing on three environments: early Universe, core-collapse supernovae, and compact binary mergers.https://www.mdpi.com/2218-1997/8/2/94astrophysical neutrinosneutrino oscillationssupernovaeneutron star mergersearly Universesterile neutrinos
spellingShingle Francesco Capozzi
Ninetta Saviano
Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
Universe
astrophysical neutrinos
neutrino oscillations
supernovae
neutron star mergers
early Universe
sterile neutrinos
title Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
title_full Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
title_fullStr Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
title_full_unstemmed Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
title_short Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
title_sort neutrino flavor conversions in high density astrophysical and cosmological environments
topic astrophysical neutrinos
neutrino oscillations
supernovae
neutron star mergers
early Universe
sterile neutrinos
url https://www.mdpi.com/2218-1997/8/2/94
work_keys_str_mv AT francescocapozzi neutrinoflavorconversionsinhighdensityastrophysicalandcosmologicalenvironments
AT ninettasaviano neutrinoflavorconversionsinhighdensityastrophysicalandcosmologicalenvironments