GRB941017: A Case Study of Neutrino Production in Gamma Ray Bursts
arXiv:astro-ph/0310417 · doi:10.1086/383568
Abstract
GRB941017, a gamma-ray burst of exceptional fluence, has recently been shown to have a high-energy component which is not consistent with the standard fireball phenomenology. If this component is the result of photomeson interactions in the burst fireball, it provides new and compelling support for substantial high-energy neutrino fluxes from this and similar sources. In this letter, we consider what impact this new information has on the neutrino spectra of gamma-ray bursts and discuss how this new evidence impacts the prospects for detection of such events in next generation neutrino telescopes.
References in corpus (12)
- High Energy Neutrinos from Cosmological Gamma-Ray Burst Fireballs
- COSMOLOGICAL GAMMA RAY BURSTS AND THE HIGHEST ENERGY COSMIC RAYS
- On the acceleration of Ultra High Energy Cosmic Rays in Gamma Ray Bursts
- High-energy Neutrino Astronomy: The Cosmic Ray Connection
- Neutrinos From Individual Gamma-Ray Bursts in the BATSE Catalog
- Propagation of Muons and Taus at High Energies
- High Energy Neutrinos from Gamma Ray Bursts
- Possible High-energy neutrinos from the cosmic accelerator RXJ1713.7-3946
- On the Neutrino Flux from Gamma-Ray Bursts
- High Energy Neutrinos from Gamma Ray Bursts: Event Rates in Neutrino Telescopes
- Neutrino Event Rates from Gamma Ray Bursts
- Gamma Ray Astronomy With IceCube
Cited by in corpus (5)
- Modeling the observations of GRB 180720B: From radio to sub-TeV gamma-rays
- GRB 110731A: Early afterglow in stellar wind powered by a magnetized outflow
- GRB 221009A: A light dark matter burst or an extremely bright Inverse Compton component?
- Neutrino emission from high-energy component gamma-ray bursts
- Constraints on the very high energy gamma-ray emission from short GRBs with HAWC