TY  - JOUR
AU  - Capozzi, F.
AU  - Saviano, N.
PY  - 2022
DA  - 2022//
TI  - Neutrino Flavor Conversions in High-Density Astrophysical and Cosmological Environments
T2  - Universe
JO  - Universe
SP  - 94 - 23pp
VL  - 8
IS  - 2
PB  - Mdpi
KW  - astrophysical neutrinos
KW  - neutrino oscillations
KW  - supernovae
KW  - neutron star mergers
KW  - early Universe
KW  - sterile neutrinos
AB  - 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.
UR  - https://arxiv.org/abs/2202.02494
UR  - https://doi.org/10.3390/universe8020094
DO  - 10.3390/universe8020094
LA  - English
N1  - WOS:000762069300001
ID  - Capozzi+Saviano2022
ER  -