The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Neutrino Afterglow from Gamma‐Ray Bursts: ∼1018eV
Open accessAbstract
We show that a significant fraction of the energy of a γ-ray burst (GRB) is probably converted to a burst of 10 17 -10 19 eV neutrinos and multiple GeV γ-rays that follow the main GRB by ~10 s. If GRBs accelerate protons to ~10 20 eV, a suggestion that recently gained support from observations of GRB afterglows, then both the neutrinos and the γ-rays may be detectable.
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Citations
Cites
Fluid dynamics of relativistic blast waves
Blandford, R. D., & McKee, C. F. (1976) · The Physics of Fluids · doi:10.1063/1.861619 · Cited by 1,215
Cited by
The physics of gamma-ray bursts & relativistic jets
Kumar, P., & Zhang, B. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.09.008 · Cited by 952
GAMMA-RAY BURSTS: PROGRESS, PROBLEMS & PROSPECTS
ZHANG, B., & MÉSZÁROS, P. (2004) · International Journal of Modern Physics A · doi:10.1142/s0217751x0401746x · Cited by 783
The Astrophysics of Ultrahigh-Energy Cosmic Rays
Kotera, K., & Olinto, A. V. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102620 · Cited by 470
Metadata
- Authors
- Waxman, E., & Bahcall, J. N.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2000-10
- Volume
- 541
- Issue
- 2
- Pages
- 707-711
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2053392891
- Cited by
- 196
- References
- 1
- FWCI
- 7.16
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Waxman, E., & Bahcall, J. N. (2000). Neutrino Afterglow from Gamma‐Ray Bursts: ∼1018eV. The Astrophysical Journal. https://doi.org/10.1086/309462
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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