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Supernova Relic Neutrinos in Liquid Argon detectors

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arxiv hep-ph/0408031 v2 pith:6742AHBQ submitted 2004-08-03 hep-ph

A.G. Cocco , A. Ereditato , G. Fiorillo , G. Mangano , V. Pettorino This is my paper · ORCID
classification hep-ph
keywords argondetectorsliquidneutrinossupernovabackgroundenergykton
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We study the possibility of detecting the background of Supernova Relic Neutrinos (SRN) with liquid Argon Time Projection Chamber (TPC) detectors. As far as this study is concerned, these experimental devices are mainly sensitive to electron neutrino signals, and could provide further information on both Supernova explosion mechanism and on star formation rate at redshifts z <2. We study in details the main contributions to background in the relevant energy range from 8B and hep solar neutrinos as well as from low energy atmospheric neutrino fluxes. Depending on the theoretical prediction for the SRN flux we find that for a 3 kton and a 100 kton liquid Argon TPC detectors the signal may be observed at the 1 sigma and 4 sigma level, respectively, with 5 years of data taking.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Diffuse Supernova Neutrino Background and Neutrino Non-Radiative Decay: a Bayesian Perspective

    hep-ph 2024-12 conditional novelty 6.0 of 10

    A Bayesian forecast of upcoming DSNB detectors shows neutrino decay can be distinguished from stability for quasi-degenerate or inverted mass patterns, but not for strong normal hierarchy.

  2. Diffuse Supernova Neutrinos with Secret Neutrino Interactions

    hep-ph 2026-06 unverdicted novelty 5.0 of 10

    Models scalar-mediated νSI on the DSNB in a full three-flavor PMNS framework for four coupling structures and projects 3σ sensitivities at JUNO, Hyper-Kamiokande-Gd, and DUNE reaching g∼10^{-8} for m_ϕ∼100-300 eV.

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