Neutron conversion-diffusion: a new model for structured short gamma-ray burst jets compatible with GRB 170817

TL;DR

This paper introduces a neutron conversion-diffusion model explaining the structured jet of GW170817, aligning with observed gamma-ray burst data and providing insights into jet composition and energy distribution.

Contribution

The model is the first to incorporate neutron conversion-diffusion effects, explaining the jet structure and energy distribution in neutron star merger events.

Findings

The jet has an isotropic energy distribution proportional to θ^{-4}.

The model is compatible with GW170817/GRB 170817A observations.

Provides a new framework for understanding short gamma-ray burst jets.

Abstract

We present a generic theoretical model for the structuring of a relativistic jet propagating through the ejecta of a binary neutron star merger event, introducing the effects of the neutron conversion-diffusion, which provides a baryon flux propagating transversely from the ejecta towards the jet axis. This results naturally in an increased baryon load structure of the outer jet with the approximate isotropic energy distribution $E_{iso}(\theta) \propto \theta^{-4}$, which is compatible with the first gravitational wave and short gamma-ray burst event GW170817/GRB 170817A observed at an off-axis angle of the jet.