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Supernova Neutrinos in the Multi-Messenger Era, SNEWS 2.0

14–17 Jun 2019
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Canada/Eastern timezone

Session

Contributed talks VI

16 Jun 2019, 13:30
Other Institutes

Other Institutes

Laurentian University 935 Ramsey Lake Rd, Sudbury, ON P3E 2C6

Conveners

Contributed talks VI

  • Matthew Geske

Presentation materials

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  1. 10. High-Energy Neutrinos from Supernovae
    Prof. Kohta Murase (Penn State University)
    16/06/2019, 13:30
    Contributed Talk

    Neutrinos from supernovae (SNe) are crucial probes of explosive phenomena at the deaths of massive stars and neutrino physics and high-energy neutrinos are produced through hadronic processes by cosmic rays. We point out that IceCube and KM3Net can detect about 100-1000 events from a SN II-P (and >100,000 events from a SN IIn) at a distance of 10 kpc. We provide new quantitative predictions of...

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  2. 19. Supernova Early Warning in the Daya Bay Reactor Neutrino Experiment
    Zhe Wang (Tsinghua University)
    16/06/2019, 13:50
    Contributed Talk

    A prompt warning of supernova burst neutrino signals is quite attractive. The Daya Bay Reactor Neutrino Experiment, with liquid scintillator, is sensitive to the inverse-beta-decay (IBD) process of electron-antineutrinos, and it can give a real-time measurement of the full supernova burst neutrino energy spectrum. The Daya Bay experiment has 8 isolated neutrino detectors, so that the...

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  3. 17. First real-time results and CCSN alert triggering with the KM3NeT neutrino telescopes
    Massimiliano Lincetto (IN2P3/CPPM, Marseille)
    16/06/2019, 14:10
    Contributed Talk

    The KM3NeT collaboration has started to build the ARCA and ORCA neutrino detectors in the Mediterranean Sea. With the most recent data from the first instrumented lines deployed at each site, a detailed characterization of the detector and background has been achieved. The technique for Core-Collapse Supernova neutrino detection and its implementation as a real time trigger have been refined...

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