Neutrinos from Gamma-Ray Bursts in Pulsar Wind Bubbles: \sim 10^{16} eV
arXiv:astro-ph/0212045 · doi:10.1103/PhysRevLett.90.201103
Abstract
The supranova model for Gamma-Ray Bursts (GRBs) is becoming increasingly more popular. In this scenario the GRB occurs weeks to years after a supernova explosion, and is located inside a pulsar wind bubble (PWB). Protons accelerated in the internal shocks that emit the GRB may interact with the external PWB photons producing pions which decay into \sim 10^{16} eV neutrinos. A km^2 neutrino detector would observe several events per year correlated with the GRBs.
arXiv commentAccepted for publication in PRL. 4 pages, 3 figures, minor changes
References in corpus (16)
- Are Gamma-Ray Bursts in Star Forming Regions?
- High Energy Neutrinos from Cosmological Gamma-Ray Burst Fireballs
- High Energy Neutrinos from Astrophysical Sources: An Upper Bound
- COSMOLOGICAL GAMMA RAY BURSTS AND THE HIGHEST ENERGY COSMIC RAYS
- The Observed Offset Distribution of Gamma-Ray Bursts from Their Host Galaxies: A Robust Clue to the Nature of the Progenitors
- On the acceleration of Ultra High Energy Cosmic Rays in Gamma Ray Bursts
- Particle Physics with High Energy Neutrinos
- TeV Neutrinos from Successful and Choked Gamma-Ray Bursts
- A gamma ray burst with small contamination
- Neutrino afterglow from Gamma-Ray Bursts: ~10^{18} eV
- Efficiency and spectrum of internal gamma-ray burst shocks
- High Energy Emission from the Prompt Gamma-Ray Burst
- On the Neutrino Flux from Gamma-Ray Bursts
- Gamma-Ray Burst Afterglows in Pulsar-Wind Bubbles
- Observational Implications of a Plerionic Environment for GRBs
- Neutrinos from Pulsar Wind Bubbles as Precursors to Gamma-Ray Bursts
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- The Physics of Gamma-Ray Bursts
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- Neutrinos From Individual Gamma-Ray Bursts in the BATSE Catalog
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- High Energy Neutrinos from Gamma Ray Bursts
- Multimessenger astronomy with gravitational waves and high-energy neutrinos
- High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae
- High-energy neutrinos from reverse shocks in choked and successful relativistic jets
- Neutrino signatures of the supernova - gamma ray burst relationship
- Neutrinos from the pulsar wind nebulae
- Multimessenger Science Reach and Analysis Method for Common Sources of Gravitational Waves and High-energy Neutrinos
- Extra galactic sources of high energy neutrinos
- Neutrino Emission in Jet Propagation Process
- TeV-PeV Neutrino Oscillation of Low-luminosity Gamma-ray Bursts
- Neutrino Counterparts of Fast Radio Bursts
- Limits on the Transient Ultra-High Energy Neutrino Flux from Gamma-Ray Bursts (GRB) Derived from RICE Data
- Neutrino astronomy and gamma-ray bursts
- Prompt Neutrino Emission of Gamma-Ray Bursts in the Dissipative Photospheric Scenario Revisited: Possible Contributions from Cocoons
- High Energy Neutrinos and Photons from Curvature Pions in Magnetars