Spinar Paradigm and Gamma Ray Bursts Central Engine
V.Lipunov (1,2,3), E.Gorbovskoy (1,2,3) ((1) Sternberg Astronomical, Institute, (2) Dep. of Physics of Moscow State University, (3) Moscow Union, 'Optic')

TL;DR
This paper introduces a comprehensive collapse model of the spinar, a quasi-equilibrium object, to explain various features of gamma-ray bursts, including precursors and X-ray plateaus, by considering rotation, magnetic fields, and relativistic effects.
Contribution
It presents a new non-stationary three-parameter collapse model incorporating rotation, magnetic fields, and relativistic effects to unify diverse gamma-ray burst phenomena.
Findings
Model explains precursors, X-ray, and optical bursts.
Describes the temporal behavior of GRB central engines.
Unifies different GRB features within a single framework.
Abstract
A spinar is a quasi-equilibrium collapsing object whose equilibrium is maintained by the balance of centrifugal and gravitational forces and whose evolution is determined by its magnetic field. The spinar quasi equilibrium model recently discussed as the course for extralong X-ray plateu in GRB (Lipunov & Gorbovskoy, 2007). We propose a simple non stationary three-parameter collapse model with the determining role of rotation and magnetic field in this paper. The input parameters of the theory are the mass, angular momentum, and magnetic field of the collapsar. The model includes approximate description of the following effects: centrifugal force, relativistic effects of the Kerr metrics, pressure of nuclear matter, dissipation of angular momentum due to magnetic field, decrease of the dipole magnetic moment due to compression and general-relativity effects (the black hole has no hare),…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGamma-ray bursts and supernovae
