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Open AccessJournal ArticleDOI

Supernova Relic Neutrino Search at Super-Kamiokande

K. Bays, +118 more
- 22 Mar 2012 - 
- Vol. 85, Iss: 5, pp 052007
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TLDR
A new Super-Kamiokande search for supernova relic neutrinos was conducted using 2853 live days of data as mentioned in this paper, and the results showed that the neutrino flux was between 2.8 and 3.3 MeV.
Abstract
A new Super-Kamiokande search for supernova relic neutrinos was conducted using 2853 live days of data. Sensitivity is now greatly improved compared to the 2003 Super-Kamiokande result, which placed a flux limit near many theoretical predictions. This more detailed analysis includes a variety of improvements such as increased efficiency, a lower energy threshold, and an expanded data set. New combined upper limits on supernova relic neutrino flux are between 2.8 and $3.1{\overline{\ensuremath{\nu}}}_{e}\text{ }\text{ }{\mathrm{cm}}^{\ensuremath{-}2}\text{ }{\mathrm{s}}^{\ensuremath{-}1}g16\text{ }\text{ }\mathrm{MeV}$ total positron energy (17.3 MeV ${\mathrm{E}}_{\ensuremath{\nu}}$).

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Journal ArticleDOI

Neutrino Physics with JUNO

Fengpeng An, +229 more
- 10 Feb 2016 - 
TL;DR: The Jiangmen Underground Neutrino Observatory (JUNO) as mentioned in this paper is a 20kton multi-purpose underground liquid scintillator detector with the determination of neutrino mass hierarchy (MH) as a primary physics goal.
Journal ArticleDOI

Neutrino Physics with JUNO

Fengpeng An, +229 more
TL;DR: The Jiangmen Underground Neutrino Observatory (JUNO) as mentioned in this paper is a 20 kton multi-purpose underground liquid scintillator detector with the determination of the neutrino mass hierarchy as a primary physics goal.
Journal ArticleDOI

Supernova neutrinos: production, oscillations and detection

TL;DR: In this paper, the authors assess the capability of current and planned large underground neutrino detectors to yield faithful information of the time and flavor dependent neutrinos signal from a future Galactic supernova.
Posted ContentDOI

Supernova Neutrinos: Production, Oscillations and Detection

TL;DR: In this article, the authors assess the capability of current and planned large underground neutrino detectors to yield faithful information of the time and flavor dependent neutrinos signal from a future Galactic supernova.
Journal ArticleDOI

Supernova Neutrino Detection

TL;DR: A core-collapse supernova will produce an enormous burst of neutrinos of all flavors in the few-tens-of-MeV range as mentioned in this paper, which will yield answers to many physics and astrophysics questions.
References
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Journal ArticleDOI

Scalar triplet leptogenesis without right-handed neutrino decoupling

TL;DR: In this article, leptogenesis in the context of type-II seesaw in the case in which in addition to the scalar electroweak triplet decays the lepton asymmetry is also induced by right-handed neutrino decays (mild hierarchical scenarios).

The Super-Kamiokande Collaboration

TL;DR: A total of 614 upward through-going muons of minimum energy 1.6 GeV were observed by Super-Kamiokande during 537 detector live days as discussed by the authors.
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