Fundamental physics from black holes, neutron stars and gamma-ray bursts
arXiv:1107.0862 · doi:10.1142/S0218271811019876
Abstract
Gamma-ray bursts (GRBs) and supernovae (SNe) bring new perspectives to the study of neutron stars and white dwarfs, as well as opening new branches of theoretical physics and astrophysics.
83 pages, 47 figures, to appear in the Proceedings of the Twelfth Marcel Grossmann Meeting on General Relativity
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Cited by in corpus (7)
- Hypercritical Accretion, Induced Gravitational Collapse, and Binary-Driven Hypernovae
- On the Induced Gravitational Collapse of a Neutron Star to a Black Hole by a Type Ib/c Supernova
- Constraining the electric charges of some astronomical bodies in Reissner-Nordstrom spacetimes and generic r^-2-type power-law potentials from orbital motions
- GRB 090618: The First Example of a Neutron Star Gravitational Collapse to a Black Hole Induced by a Type Ib/c Supernova
- Induced Gravitational Collapse, Binary-Driven Hypernovae, Long Gramma-ray Bursts and Their Connection with Short Gamma-ray Bursts
- Induced gravitational collapse at extreme cosmological distances: the case of GRB 090423
- Black Holes, Supernovae and Gamma Ray Bursts