Abstract
Gamma-ray burst sources appear to fulfill all the conditions for being efficient cosmic ray accelerators, and being extremely compact, are also expected to produce multi-GeV to PeV neutrinos. I review the basic model predictions for the expected neutrino fluxes in classical GRBs as well as in low luminosity and choked bursts, discussing the recent IceCube observational constraints and implications from the observed diffuse neutrino flux.
| Original language | English (US) |
|---|---|
| Title of host publication | Neutrino Astronomy |
| Subtitle of host publication | Current Status, Future Prospects |
| Publisher | World Scientific Publishing Co. Pte Ltd |
| Pages | 1-14 |
| Number of pages | 14 |
| ISBN (Electronic) | 9789814759410 |
| ISBN (Print) | 9789814759403 |
| DOIs | |
| State | Published - Mar 20 2017 |
All Science Journal Classification (ASJC) codes
- Physics and Astronomy(all)