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RES-NOVA sensitivity to core-collapse and failed core-collapse supernova neutrinos
- Source :
- Journal of Cosmology and Astroparticle Physics. 2021:064
- Publication Year :
- 2021
- Publisher :
- IOP Publishing, 2021.
-
Abstract
- RES-NOVA is a new proposed experiment for the investigation of astrophysical neutrino sources with archaeological Pb-based cryogenic detectors. RES-NOVA will exploit Coherent Elastic neutrino-Nucleus Scattering (CE$��$NS) as detection channel, thus it will be equally sensitive to all neutrino flavors produced by Supernovae (SNe). RES-NOVA with only a total active volume of (60 cm)$^3$ and an energy threshold of 1 keV will probe the entire Milky Way Galaxy for (failed) core-collapse SNe with $> 3 ��$ detection significance. The high detector modularity makes RES-NOVA ideal also for reconstructing the main parameters (e.g. average neutrino energy, star binding energy) of SNe occurring in our vicinity, without deterioration of the detector performance caused by the high neutrino interaction rate. For the first time, distances $
- Subjects :
- Physics
Physics - Instrumentation and Detectors
Physics::Instrumentation and Detectors
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
Collapse (topology)
Astronomy and Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Instrumentation and Detectors (physics.ins-det)
Nova (laser)
Astrophysics
Type II supernova
Core (optical fiber)
Neutrino detector
Astrophysics::Solar and Stellar Astrophysics
High Energy Physics::Experiment
Neutrino
Astrophysics - Instrumentation and Methods for Astrophysics
Instrumentation and Methods for Astrophysics (astro-ph.IM)
Subjects
Details
- ISSN :
- 14757516
- Volume :
- 2021
- Database :
- OpenAIRE
- Journal :
- Journal of Cosmology and Astroparticle Physics
- Accession number :
- edsair.doi.dedup.....b260675ba5f617e9dc4024217f9db717