Prospects of the search for neutrino bursts from Supernovae with Baksan Large Volume Scintillation Detector
arXiv:1508.01389 · doi:10.1134/S1063779616060204
Abstract
Observing a high-statistics neutrino signal from the supernova explosions in the Galaxy is a major goal of low-energy neutrino astronomy. The prospects for detecting all flavors of neutrinos and antineutrinos from the core-collapse supernova (ccSN) in operating and forthcoming large liquid scintillation detectors (LLSD) are widely discussed now. One of proposed LLSD is Baksan Large Volume Scintillation Detector (BLVSD). This detector will be installed at the Baksan Neutrino Observatory (BNO) of the Institute for Nuclear Research, Russian Academy of Sciences, at a depth of 4800 m.w.e. Low-energy neutrino astronomy is one of the main lines of research of the BLVSD.
Talk at the International Workshop on Prospects of Particle Physics: "Neutrino Physics and Astrophysics" , Valday, Russia, January 1 - February 8, 2015. Accepted for publication in Physics of Elementary Particles and Atomic Nuclei
References in corpus (6)
- Reference worldwide model for antineutrinos from reactors
- Advanced Scintillator Detector Concept (ASDC): A Concept Paper on the Physics Potential of Water-Based Liquid Scintillator
- Spectrum of Supernova Neutrinos in Ultra-pure Scintillators
- Research of the natural neutrino fluxes by use of large volume scintillation detector at Baksan
- The Physics Potential of the LENA Detector
- Neutrino Geophysics at Baksan (Part II): Possible Studies of Antineutrino- and Radiogenic Heat Sources in Earth Interior