Results 81 to 90 of about 23,101 (234)
Future Long-Baseline Neutrino Facilities and Detectors
We review the ongoing effort in the US, Japan, and Europe of the scientific community to study the location and the detector performance of the next-generation long-baseline neutrino facility. For many decades, research on the properties of neutrinos and
Milind Diwan +5 more
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Non-standard neutrino interactions with a massive boson can produce the bosons in the core of core-collapse supernovae (SNe). After the emission of the bosons from the SN core, their subsequent decays into neutrinos can modify the SN neutrino flux.
Kensuke Akita, Sang Hui Im, Mehedi Masud
doaj +1 more source
Dirac-Neutrino Magnetic Moment and the Dynamics of a Supernova Explosion
The double conversion of the neutrino helicity $\nu_L \to \nu_R \to \nu_L$ has been analyzed for supernova conditions, where the first stage is due to the interaction of the neutrino magnetic moment with plasma electrons and protons in the supernova core,
A. A. Okrugin +23 more
core +1 more source
Neutrino Emission from Supernovae [PDF]
Author version of chapter for 'Handbook of Supernovae,' edited by A. Alsabti and P. Murdin, Springer.
openaire +3 more sources
Neutrino forces in neutrino backgrounds
The Standard Model predicts a long-range force, proportional to G F 2 / r 5 $$ {G}_F^2/{r}^5 $$ , between fermions due to the exchange of a pair of neutrinos. This quantum force is feeble and has not been observed yet.
Mitrajyoti Ghosh +4 more
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Invited talk at the X International Workshop on Neutrino Telescopes, Venice, Italy, March 11-14 ...
openaire +2 more sources
Limits on heavy neutral leptons, Z ′ bosons and majorons from high-energy supernova neutrinos
Light hypothetical particles with masses up to O 100 $$ \mathcal{O}(100) $$ MeV can be produced in the core of supernovae. Their subsequent decays to neutrinos can produce a flux component with higher energies than the standard flux.
Kensuke Akita +3 more
doaj +1 more source
Supernova Relic Electron Neutrinos and anti-Neutrinos in future Large-scale Observatories
We investigate the signal from supernova relic neutrinos in future large scale observatories, such as MEMPHYS (UNO, Hyper-K), LENA and GLACIER, at present under study.
Volpe, C., Welzel, J.
core +1 more source
Understanding Supernova Neutrino Physics using Low-Energy Beta-Beams
We show that fitting linear combinations of low-energy beta-beam spectra to supernova-neutrino energy-distributions reconstructs the response of a nuclear target to a supernova flux in a very accurate way. This allows one to make direct predictions about
Jachowicz, N., McLaughlin, G. C.
core +1 more source

