Abstract
High-energy neutrinos from Gamma-Ray Bursts (GRBs) have been expected since the pre-Swift era. Such signals may be detected by future large neutrino detectors such as IceCube. Recently Swift has shown several novel phenomena. We suggest the new prospects for high-energy neutrino emission in the Swift era. Expected signals, if detected, are useful for revealing of the nature of GRBs.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1529-1530 |
| Number of pages | 2 |
| Journal | Nuovo Cimento della Societa Italiana di Fisica B |
| Volume | 121 |
| Issue number | 12 |
| DOIs | |
| State | Published - Dec 2006 |
All Science Journal Classification (ASJC) codes
- Physics and Astronomy(all)