# Supernova neutrino detection

@article{Scholberg2000SupernovaND,
title={Supernova neutrino detection},
author={Kate Scholberg},
journal={Journal of Physics: Conference Series},
year={2000},
volume={375},
pages={042036}
}
• K. Scholberg
• Published 22 August 2000
• Physics
• Journal of Physics: Conference Series
282 Citations
• A. Weinstein
• Physics
Journal of Physics: Conference Series
• 2020
The Deep Underground Neutrino Experiment (DUNE) experiment, a 40-kton underground liquid argon time-projection-chamber detector, will have unique sensitivity to the electron flavor component of a
Neutrinos are key particles in core-collapse supernovae. Traveling unimpeded through the stellar core, neutrinos can be direct probes of the still uncertain and fascinating supernova mechanism.
• Physics
Supernovae
• 2018
Neutrinos are fundamental particles in the collapse of massive stars. Because of their weakly interacting nature, neutrinos can travel undisturbed through the stellar core and be direct probes of the
• Physics
Space Science Reviews
• 2018
Neutrinos are fundamental particles in the collapse of massive stars. Because of their weakly interacting nature, neutrinos can travel undisturbed through the stellar core and be direct probes of the
• Physics
• 2021
In this theoretical study of successful core-collapse supernovae, the authors provide a detailed model of neutrino emission from the different phases of the transition - explosion to proto-neutron
• Physics
• 2018
Modern neutrino facilities will be able to detect a large number of neutrinos from the next Galactic supernova. We investigate the viability of the triangulation method to locate a core-collapse
• Physics
• 2018
Modern neutrino facilities will be able to detect a large number of neutrinos from the next Galactic supernova. We investigate the viability of the triangulation method to locate a core-collapse
• Physics
• 2021
Neutrinos from a Galactic core-collapse supernova will be measured by neutrino detectors minutes to days before an optical signal reaches Earth. We present a novel calculation showing the ability of
• Physics
• 2015
In the late stages of nuclear burning for massive stars (M > 8 M⊙), the production of neutrino–antineutrino pairs through various processes becomes the dominant stellar cooling mechanism. As the star

## References

SHOWING 1-10 OF 78 REFERENCES

• Bionta
• Physics
Physical review letters
• 1987
A burst of eight neutrino events preceding the optical detection of the supernova in the Large Magellanic cloud has been observed in a large underground water Cherenkov detector. The events span an
Neutrinos have been an important feature of theories of stellar processes for many decades. As a star forms from interstellar matter, its temperature gradually increases because of its gravitational
• Physics
• 2002
We study the effects of neutrino oscillation on supernova neutrinos in the case of the inverted mass hierarchy (m 3 10 - 3 ) and that θ 1 3 can be probed effectively by SuperKamiokande if the
• Physics
Physical review. D, Particles and fields
• 1994
A high energy neutrino telescope is simulated to detect a galactic supernova at or above the 5\ensuremath{\sigma} level; this capability requires detectors with roughly 3 times the number of optical modules; thus, this will be within easy reach of the next generation detectors.
• Physics
• 2002
We propose that neutrino-proton elastic scattering, ν+p→ν+p, can be used for the detection of supernova neutrinos in scintillator detectors. Though the proton recoil kinetic energy spectrum is soft,
• Physics
• 2003
We examine the prospects for using lead as a supernova-neutrino detector by considering the spectrum of electrons produced, and the number of one- and two-neutron events. We show that the electron
• Physics
• 2000
We study the role that the future detection of the neutrino burst from a galactic supernova can play in the reconstruction of the neutrino mass spectrum. We consider all possible 3$\nu$ mass and
• Physics
• 1987
We discuss here the characteristics of the event detected in the Mont Blanc Underground Neutrino Observatory on February 23, 1987, consisting of 5 interactions recorded during 7s. The measured
• Physics
• 2002
We estimate possible delayed β decay signatures of the neutrino induced reactions on 16O in a two-step model: the primary neutrino (ν,l) process, where l is the lepton in the final state, is