Results 51 to 60 of about 1,191,896 (269)
Non-standard interactions of solar neutrinos in dark matter experiments
Physics Letters B, 2017 We show that non-standard neutrino interactions (NSI) can be probed in future direct dark matter detection experiments through both elastic neutrino-electron scattering and coherent neutrino-nucleus scattering. We show NSI can increase the event rate due
Bhaskar Dutta +3 more
doaj +1 more source
CORE-COLLAPSE SUPERNOVAE FROM 9 TO 120 SOLAR MASSES BASED ON NEUTRINO-POWERED EXPLOSIONS [PDF]
, 2015 Nucleosynthesis, light curves, explosion energies, and remnant masses are calculated for a grid of supernovae (SNe) resulting from massive stars with solar metallicity and masses from 9.0 to 120 M ⊙ .
T. Sukhbold +4 more
semanticscholar +1 more source
Combined Effect of NSI and SFP on Solar Electron Neutrino Oscillation
Advances in High Energy Physics, 2016 The combined effect of spin-flavor precession (SFP) and the nonstandard neutrino interaction (NSI) on the survival probability of solar electron neutrinos (assumed to be Dirac particles) is examined for various values of ϵ11, ϵ12, and μB.
Deniz Yilmaz
doaj +1 more source
Journal of High Energy Physics, 2022 The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP).
Evgeny Akhmedov, Pablo Martínez-Miravé
doaj +1 more source
Solar neutrino physics with low-threshold dark matter detectors [PDF]
, 2014 Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent neutrino-nucleus and neutrino-electron elastic scatterings.
J. Billard +8 more
semanticscholar +1 more source
Solar neutrino spectroscopy [PDF]
Physics Reports, 2017 More than forty years after the first detection of neutrinos from the Sun, the spectroscopy of solar neutrinos has proven to be an on-going success story. The long-standing puzzle about the observed solar neutrino deficit has been resolved by the discovery of neutrino flavor oscillations.
openaire +2 more sources
7Be solar neutrino measurement with KamLAND [PDF]
, 2014 We report a measurement of the neutrino-electron elastic scattering rate of 862 keV ^7Be solar neutrinos based on a 165.4 kt d exposure of KamLAND. The observed rate is 582±94(kt d)^(−1), which corresponds to an 862-keV Be7 solar neutrino flux of (3.26±0.
A. Gando +70 more
semanticscholar +1 more source
Shedding light on LMA-dark solar neutrino solution by medium baseline reactor experiments: JUNO and RENO-50 [PDF]
, 2014 A bstractIn the presence of Non-Standard neutral current Interactions (NSI) a new solution to solar neutrino anomaly with cos 2θ12 < 0 appears. We investigate how this solution can be tested by upcoming intermediate baseline reactor experiments, JUNO and
P. Bakhti, Y. Farzan
semanticscholar +1 more source
On Stellar Evolution in a Neutrino Hertzsprung–Russell Diagram
The Astrophysical Journal, 2020 We explore the evolution of a select grid of solar metallicity stellar models from their pre-main-sequence phase to near their final fates in a neutrino Hertzsprung–Russell diagram, where the neutrino luminosity replaces the traditional photon luminosity.
Ebraheem Farag +4 more
doaj +1 more source
Solar neutrinos and neutrino physics [PDF]
, 2015 .Solar neutrino studies triggered and largely motivated the major developments in neutrino physics in the last 50 years. The theory of neutrino propagation in different media with matter and fields has been elaborated.
M. Maltoni, Alexei Yu. Smirnov
semanticscholar +1 more source