It has been known that neutrinos from supernova (SN) bursts can give rise to nuclear recoil (NR) signals arising from coherent elastic neutrino-nucleus scattering (CE$\nu$NS) interaction, a neutral current (NC) process, of the neutrinos with xenon nuclei in future large (multi-ton scale) liquid xenon (LXe) detectors employed for dark matter search, depending on the SN progenitor mass and distance to the SN. In this paper, we show that the same detectors will also be sensitive to inelastic charged current (CC) interactions of the SN electron neutrinos ($\nu_e$CC) with the xenon nuclei. Such interactions, while creating an electron in the final state, also leave the post-interaction target nucleus in an excited state, the subsequent deexcitat...
We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through th...
Knowledge of the ionization and scintillation responses of liquid xenon (LXe) to nuclear recoils is ...
We propose that neutrino-proton elastic scattering, {nu} + p {yields} {nu} + p, can be used for the ...
For the next galactic supernova, operational neutrino telescopes will measure the neutrino flux seve...
Dark matter detectors that utilize liquid xenon have now achieved tonne-scale targets, giving them s...
The dark matter experiment XENON1T is operational and sensitive to all flavors of neutrinos emitted ...
We propose that neutrino-proton elastic scattering, ν+p→ν+p, can be used for the detection of supern...
Future large liquid-scintillator detectors can be implemented to observe neutrinos from a core-colla...
Neutrinos from core collapse supernovae can excite nuclei of some detector materials beyond their ne...
Core-collapse supernova (CCSN) provides a unique astrophysical site for studying neutrino-matter int...
Detecting neutrinos—elementary particles that barely interact with other matter—usually requires det...
In this letter we point out the possibility to study new physics in the neutrino sector using dark m...
We study the effect of including flavor changing neutral currents (FCNC) in the analysis of the neut...
We study the sensitivity of large-scale xenon detectors to low-energy solar neutrinos, to coherent n...
The sources of the astrophysical neutrino flux discovered by IceCube are for the most part unresolve...
We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through th...
Knowledge of the ionization and scintillation responses of liquid xenon (LXe) to nuclear recoils is ...
We propose that neutrino-proton elastic scattering, {nu} + p {yields} {nu} + p, can be used for the ...
For the next galactic supernova, operational neutrino telescopes will measure the neutrino flux seve...
Dark matter detectors that utilize liquid xenon have now achieved tonne-scale targets, giving them s...
The dark matter experiment XENON1T is operational and sensitive to all flavors of neutrinos emitted ...
We propose that neutrino-proton elastic scattering, ν+p→ν+p, can be used for the detection of supern...
Future large liquid-scintillator detectors can be implemented to observe neutrinos from a core-colla...
Neutrinos from core collapse supernovae can excite nuclei of some detector materials beyond their ne...
Core-collapse supernova (CCSN) provides a unique astrophysical site for studying neutrino-matter int...
Detecting neutrinos—elementary particles that barely interact with other matter—usually requires det...
In this letter we point out the possibility to study new physics in the neutrino sector using dark m...
We study the effect of including flavor changing neutral currents (FCNC) in the analysis of the neut...
We study the sensitivity of large-scale xenon detectors to low-energy solar neutrinos, to coherent n...
The sources of the astrophysical neutrino flux discovered by IceCube are for the most part unresolve...
We analyze the possibility of probing non-standard neutrino interactions (NSI, for short) through th...
Knowledge of the ionization and scintillation responses of liquid xenon (LXe) to nuclear recoils is ...
We propose that neutrino-proton elastic scattering, {nu} + p {yields} {nu} + p, can be used for the ...