A Binary Neutron Star GRB Model
arXiv:astro-ph/9711307 · doi:10.1063/1.55436
Abstract
In this paper we present the preliminary results of a model for the production of gamma-ray bursts (GRBs) through the compressional heating of binary neutron stars near their last stable orbit prior to merger.
5 pages, 2 figures. Submitted to the Conference Proceedings of the 4th Huntsville Gamma-Ray Burst Symposium
Cited by in corpus (5)
- The central engine of gamma-ray bursters
- Simulations of binary coalescence of a neutron star and a black hole
- General Relativistic Augmentation of Neutrino Pair Annihilation Energy Deposition Near Neutron Stars
- Neutrino Annihilation between Binary Neutron Stars
- Neutrino oscillations and gamma-ray bursts