We consider the mixing of muon and tau neutrinos with sterile fermion fields propagating in extra dimensions in the context of core collapse supernova physics, extending the analysis of the electron neutrino case done in a previous work. We show that the potentially dramatic modifications to the supernova evolution are prevented by a mechanism of feedback, so that no severe bounds on the parameters of the extra dimensions need to be imposed. Nevertheless, the supernova core evolution is significantly modified. We discuss the consequences on the delayed explosion mechanism and the compatibility with the SN 1987A signal. Then, for the cases of both nu(mu,tau) and nu(e) mixing with bulk fermions, we analyze the distinctive features of the sign...
In very dense environments, neutrinos can undergo fast flavor conversions on scales as short as a fe...
Core-collapse supernovae (CCSNe) are driven by neutrino emission and are the most prodigious sources...
We carry out a detailed analysis of the supernova (SN) neutrino flavor evolution during the accretio...
16 pages, 7 figures; v2: minor changes, matches published versionInternational audienceWe consider t...
We consider the mixing of muon and tau neutrinos with sterile fermion fields propagating in extra di...
Models with extra space dimensions naturally provide for the existence of fermions that propagate in...
We discuss the phenomenology of neutrino mixing with bulk fermions in the context of supernova physi...
After a brief review of our current understanding of neutrino flavor conversions inside a core colla...
Assuming that right-handed neutrinos exist and propagate in some large extra dimensions, we attempt ...
I shall review some of the recent results concerning the astrophysics of a core collapse supernova (...
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall d...
Ever since a collection of 19 flickers of Cherenkov radiation in neutrino detectors around the world...
Ever since a collection of 19 flickers of Cherenkov radiation in neutrino detectors around the world...
We investigate the nuclear abundances uniquely produced from the neutrino neutrino-process in super-...
We consider for the first time flavor changing neutral currents (FCNC's) in the infall stage of stel...
In very dense environments, neutrinos can undergo fast flavor conversions on scales as short as a fe...
Core-collapse supernovae (CCSNe) are driven by neutrino emission and are the most prodigious sources...
We carry out a detailed analysis of the supernova (SN) neutrino flavor evolution during the accretio...
16 pages, 7 figures; v2: minor changes, matches published versionInternational audienceWe consider t...
We consider the mixing of muon and tau neutrinos with sterile fermion fields propagating in extra di...
Models with extra space dimensions naturally provide for the existence of fermions that propagate in...
We discuss the phenomenology of neutrino mixing with bulk fermions in the context of supernova physi...
After a brief review of our current understanding of neutrino flavor conversions inside a core colla...
Assuming that right-handed neutrinos exist and propagate in some large extra dimensions, we attempt ...
I shall review some of the recent results concerning the astrophysics of a core collapse supernova (...
Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the infall d...
Ever since a collection of 19 flickers of Cherenkov radiation in neutrino detectors around the world...
Ever since a collection of 19 flickers of Cherenkov radiation in neutrino detectors around the world...
We investigate the nuclear abundances uniquely produced from the neutrino neutrino-process in super-...
We consider for the first time flavor changing neutral currents (FCNC's) in the infall stage of stel...
In very dense environments, neutrinos can undergo fast flavor conversions on scales as short as a fe...
Core-collapse supernovae (CCSNe) are driven by neutrino emission and are the most prodigious sources...
We carry out a detailed analysis of the supernova (SN) neutrino flavor evolution during the accretio...