Implication for the core collapse supernova rate from 21 years of data of the Large Volume Detector

Abstract

The Large Volume Detector (LVD) has been continuously taking data since 1992 at the INFN Gran Sasso National Laboratory. LVD is sensitive to neutrino bursts from gravitational stellar collapses with full detection probability over the Galaxy. We have searched for neutrino bursts in LVD data taken in 7335 days of operation. No evidence of neutrino signals has been found between June 1992 and December 2013. The 90% C.L. upper limit on the rate of core-collapse and failed supernova explosions out to distances of 25 kpc is found to be 0.114/y.

arXiv commentPublished

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Cited by in corpus (21)

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• Stellar Collapse Diversity and the Diffuse Supernova Neutrino Background
• KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars
• Triangulation Pointing to Core-Collapse Supernovae with Next-Generation Neutrino Detectors
• Generalized uncertainty principle in resonant detectors of gravitational waves
• Characterization of the varying flux of atmospheric muons measured with the Large Volume Detector for 24 years
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• Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande
• Pinpointing astrophysical bursts of low-energy neutrinos embedded into the noise
• Flux measurement of fast neutrons in the Gran Sasso underground laboratory
• Search for supernova neutrinos and constraint on the galactic star formation rate with the KamLAND data
• The Diffuse Supernova Neutrino Background in the Standard and Double Collapse Models
• The core collapse supernova rate from 24 years of data of the Large Volume Detector
• Supernova electron-neutrino interactions with xenon in the nEXO detector
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