Further studies of the OMNIS supernova neutrino observatory: optimisation of detector configuration and possible extension to solar neutrinos
Author:
Publisher
Elsevier BV
Subject
Astronomy and Astrophysics
Reference48 articles.
1. The nu-process
2. OMNIS—an improved low-cost detector to measure mass and mixing of mu/tau neutrinos from a Galactic supernova
3. A new method for detection of distant supernova neutrino bursts
4. Prospects for detection of a cosmologically significant neutrino mass from a galactic supernova neutrino burst using a neutral-current-based detector
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1. References;The Physics of Neutrino Interactions;2020-06-30
2. Neutrino-nucleus cross-sections at supernova neutrino energies;International Journal of Modern Physics E;2017-07
3. Element synthesis in the supernova environment and neutrino oscillations;Journal of Physics G: Nuclear and Particle Physics;2013-06-26
4. Studies of a three-stage dark matter and neutrino observatory based on multi-ton combinations of liquid xenon and liquid argon detectors;Astroparticle Physics;2012-08
5. Results from the first science run of the ZEPLIN-III dark matter search experiment;Physical Review D;2009-09-25
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