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- durée total des cours : 10 h
- 5 matinées (10h-12h30) les 14-15 et 17-18 mai 2018 au laboratoire APC, salle a venir.
The course will focus on forefront aspects of neutrino physics and astrophysics. They will comprise lectures of 2h30 each, covering four main chapters.
General framework : Recent developments in neutrino physics, status and open questions. Neutrino oscillations in vacuum and in matter - the Mikheev-Smirnov-Wolfenstein effect and applications to the Sun, to the Earth and core-collapse supernovae
Neutrino flavor conversion phenomena : density matrix and effective spins formalisms, evolution equations describing neutrino propagation in astrophysical and cosmological environments, mean-field approximation, link to many body systems such as condensed matter and atomic nuclei
Neutrinos in dense media - core-collapse supernovae and accretion disks around compact systems (black holes or binary neutron star mergers): neutrino self-interaction and novel collective conversion phenomena, link to the supernova dynamics and to r-process nucleosynthesis, interplay with unknown neutrino properties, sterile neutrinos and/or non-standard interactions
Future observations : neutrinos from core-collapse supernovae and the diffuse supernova neutrino background, aspects of low-energy neutrino-nucleus cross sections, general conclusions
