Sep 8 – 13, 2013
Asilomar, California
US/Pacific timezone

Revealing Deaths of Massive Stars with High-Energy Neutrinos

Sep 10, 2013, 4:40 PM
20m
Asilomar, California

Asilomar, California

Asilomar Conference Grounds, 800 Asilomar Avenue, Pacific Grove, CA 93950-3704
Oral High-Energy Astrophysics (includes all cosmic ray physics) High Energy Astrophysics II

Speaker

Dr Kohta Murase (Institute for Advanced Study)

Description

Neutrinos play important roles in revealing energetic astrophysical explosions such as gamma-ray bursts (GRBs) and supernovae (SNe). The large neutrino detector, IceCube has opened a new window of the multi-messenger astronomy. I discuss neutrino emissions from GRBs in view of recent theoretical/observational progress, and emphasize the importance of sub-TeV neutrino astronomy. In particular, I show that neutron-loaded outflows lead to the promising signal from "subphotospheres". On the other hand, >>TeV neutrino production is largely prohibited inside stars for usual GRBs and jet-driven SNe, but possible for low-power GRBs. We stress the importance of dedicated searches for neutrinos from such low-power GRBs, which can also explain the PeV neutrino background observed by IceCube without violating GRB neutrino limits.

Primary author

Dr Kohta Murase (Institute for Advanced Study)

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