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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 III

15 Jun 2019, 16:00
Other Institutes

Other Institutes

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

Conveners

Contributed talks III

  • Christine Kraus

Presentation materials

There are no materials yet.

  1. 1. SuperNova Detection through CEvNS
    Rafael Lang (Purdue University)
    15/06/2019, 16:00
    Contributed Talk

    Coherent Elastic Neutrino Nucleus Scattering in direct dark matter experiments for supernova neutrino detection.

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  2. 4. Supernova Neutrino Observation in the JUNO Experiment
    Dr Huiling Li (Institute of High Energy Physics)
    15/06/2019, 16:20
    Contributed Talk

    The Jiangmen Underground Neutrino Observatory (JUNO) is a multi-purpose neutrino experiment under construction in China, designed with a 20 kton liquid scintillator detector. For the next galactic core-collapse supernova (SN), JUNO is promising to register full flavors of SN burst neutrinos with quite high statistics and a low energy threshold down to 0.2 MeV. A SN trigger system with the...

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  3. 22. Supernova Pointing Resolution of DUNE
    AJ Roeth (Duke University)
    15/06/2019, 16:40
    Contributed Talk

    One of the primary physics goals of the Deep Underground Neutrino Experiment (DUNE) is measuring the electron neutrino flux from a core-collapse supernova or black hole formation. If a neutrino burst were detected, an essential piece of information would be its source location, which would be shared via the Supernova Early Warning System (SNEWS). This would allow other astronomers to observe...

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  4. 8. IceCube Supernova Detection and Contributions to SNEWS 2.0
    Spencer Griswold (University of Rochester)
    15/06/2019, 17:00
    Contributed Talk

    The IceCube Neutrino Observatory is an anchor of the SuperNova Early Warning System (SNEWS). IceCube is comprised of 5160 digital optical modules (DOMs) instrumenting 1 km$^3$ of ice deep below the surface of the geographic South Pole. This large volume makes it sensitive to neutrinos generated by core-collapse supernovae (CCSNe) in the Milky Way at >10$\sigma$ for all progenitor models, and...

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  5. 2. Neutrino astronomy with supernova neutrinos
    Dr Xunjie XU (Max-Planck-Institut für Kernphysik)
    15/06/2019, 17:20
    Contributed Talk

    [arXiv:1802.02577] Modern neutrino facilities will be able to detect a large number of neutrinos from the next Galactic supernova. We investigate the viability of the triangulation method to locate a core-collapse supernova by employing the neutrino arrival time differences at various detectors. We perform detailed numerical fits in order to determine the uncertainties of these time...

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