Gamma Ray Bursts as Electromagnetic Outflows
Maxim Lyutikov (1), Roger Blandford (2), ((1) McGill University, (2), Kavli Institute for Particle Astrophysics, Cosmology)

TL;DR
This paper presents a model where gamma ray bursts originate from relativistic electromagnetic explosions driven by a rotating stellar core losing energy as Poynting flux, leading to observable gamma-ray and afterglow emissions.
Contribution
It introduces a novel electromagnetic explosion model for gamma ray bursts involving non-spherical, Poynting flux-driven bubble expansion and subsequent relativistic shell formation.
Findings
Electromagnetic shells can drive relativistic blast waves in GRBs.
Magnetic instabilities lead to gamma-ray emission.
Energy transfer from electromagnetic shell to blast wave explains afterglow.
Abstract
(Abridged) We interpret gamma ray bursts as relativistic, electromagnetic explosions. Specifically, we propose that they are created when a rotating, relativistic, stellar-mass progenitor loses much of its rotational energy in the form of a Poynting flux during an active period lasting s. Initially, a non-spherically symmetric, electromagnetically-dominated bubble expands non-relativistically inside the star, most rapidly along the rotational axis of the progenitor. After the bubble breaks out from the stellar surface and most of the electron-positron pairs annihilate, the bubble expansion becomes highly relativistic. After the end of the source activity most of the electromagnetic energy is concentrated in a thin shell inside the contact discontinuity between the ejecta and the shocked circumstellar material. This electromagnetic shell pushes a relativistic blast wave into…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Solar and Space Plasma Dynamics · Astro and Planetary Science
