AbstractWe consider sterile neutrinos with rest masses ∼0.2 GeV and with vacuum flavor mixing angles θ2>10−8 for mixing with τ-neutrinos, or 10−8<θ2<10−7 for mixing with muon neutrinos. Such sterile neutrinos could augment core collapse supernova shock energies by enhancing energy transport from the core to the vicinity of the shock front. The decay of these neutrinos could produce a flux of very energetic active neutrinos, detectable by future neutrino observations from galactic supernova. The relevant range of sterile neutrino masses and mixing angles can be probed in future laboratory experiments
International audienceSterile neutrinos with masses up to $\mathcal{O} (100)$ MeV can be copiously p...
We investigate the enhancement of lepton number, energy, and entropy transport resulting from active...
A neutrino mass-mixing scheme which successfully avoids the "alpha effect," allowing r-process nucle...
AbstractWe consider sterile neutrinos with rest masses ∼0.2 GeV and with vacuum flavor mixing angles...
We consider sterile neutrinos with rest masses ∼ 0.2 GeV and with vacuum flavor mixing angles θ2 >...
The role of the sterile neutrinos to the r-process nucleosynthesis in supernova explosions is studie...
We investigate matter-enhanced Mikheyev-Smirnov-Wolfenstein (MSW) active-sterile neutrino conversion...
Taken at face value, current experimental data indicate the existence of anew particle, the sterile ...
[EN] We discuss the production of a class of heavy sterile neutrinos nu(h) in proto-neutron stars. T...
We discuss the effects of resonant $\nu_e \to\nu_s$ and the dense medium of a supernova. In particul...
Heavy sterile neutrinos with masses &calO;(100) MeV mixing with active neutrinos can be produced...
We discuss the effects of resonant νe→νs and ν¯e→ν¯s (νs is a sterile neutrino) conversions in the d...
International audienceHeavy sterile neutrinos with masses &calO;(100) MeV mixing with active neutrin...
We discuss the production of a class of heavy sterile neutrinos nu(h) in proto-neutron stars. The ne...
We employ state-of-the art cosmological observables including supernova surveys and BAO information ...
International audienceSterile neutrinos with masses up to $\mathcal{O} (100)$ MeV can be copiously p...
We investigate the enhancement of lepton number, energy, and entropy transport resulting from active...
A neutrino mass-mixing scheme which successfully avoids the "alpha effect," allowing r-process nucle...
AbstractWe consider sterile neutrinos with rest masses ∼0.2 GeV and with vacuum flavor mixing angles...
We consider sterile neutrinos with rest masses ∼ 0.2 GeV and with vacuum flavor mixing angles θ2 >...
The role of the sterile neutrinos to the r-process nucleosynthesis in supernova explosions is studie...
We investigate matter-enhanced Mikheyev-Smirnov-Wolfenstein (MSW) active-sterile neutrino conversion...
Taken at face value, current experimental data indicate the existence of anew particle, the sterile ...
[EN] We discuss the production of a class of heavy sterile neutrinos nu(h) in proto-neutron stars. T...
We discuss the effects of resonant $\nu_e \to\nu_s$ and the dense medium of a supernova. In particul...
Heavy sterile neutrinos with masses &calO;(100) MeV mixing with active neutrinos can be produced...
We discuss the effects of resonant νe→νs and ν¯e→ν¯s (νs is a sterile neutrino) conversions in the d...
International audienceHeavy sterile neutrinos with masses &calO;(100) MeV mixing with active neutrin...
We discuss the production of a class of heavy sterile neutrinos nu(h) in proto-neutron stars. The ne...
We employ state-of-the art cosmological observables including supernova surveys and BAO information ...
International audienceSterile neutrinos with masses up to $\mathcal{O} (100)$ MeV can be copiously p...
We investigate the enhancement of lepton number, energy, and entropy transport resulting from active...
A neutrino mass-mixing scheme which successfully avoids the "alpha effect," allowing r-process nucle...