Magnetic Ergostars, Jet Formation and Gamma-Ray Bursts: Ergoregions versus Horizons

TL;DR

This study uses general relativistic magnetohydrodynamic simulations to compare ergostars and black holes in their ability to launch relativistic jets, finding neither ergostars nor hypermassive neutron stars produce jets suitable for short gamma-ray bursts.

Contribution

First comprehensive GRMHD simulations of hypermassive neutron stars with ergoregions, analyzing their potential to produce relativistic jets compared to black holes.

Findings

Ergostars do not produce highly relativistic jets.

Magnetic outflows in ergostars are insufficient for gamma-ray bursts.

Blandford-Znajek mechanism requires a black hole presence.

Abstract

We perform the first fully general relativistic, magnetohydrodynamic simulations of dynamically stable hypermassive neutron stars with and without ergoregions to assess the impact of ergoregions on launching magnetically--driven outflows. The hypermassive neutron stars are modeled by a compressible and causal equation of state and are initially endowed with a dipolar magnetic field extending from the stellar interior into its exterior. We find that, after a few Alfv\'en times, magnetic field lines in the ergostar (star that contains ergoregions) and the normal star have been tightly wound in both cases into a helical funnel within which matter begins to flow outward. The maximum Lorentz factor in the outflow is $\Gamma_L \sim 2.5$, while the force-free parameter holds at $B^2/8\pi\rho_0\lesssim 10$. These values are incompatible with highly relativistic, magnetically-driven outflows (jets) and short $\gamma$-ray bursts. We compare these results with those of a spinning black hole surrounded by a magnetized, massless accretion disk that launches a bona fide jet. Our simulations suggest that the Blandford-Znajek mechanism for launching relativistic jets only operates when a black hole is present, though the Poynting luminosity in all cases is comparable. Therefore, one cannot distinguish a magnetized, accreting black hole from a magnetized hypermassive neutron star in the so-called mass-gap based solely on the value of the observed Poynting luminosity. These results complement our previous studies of supramassive remnants and suggest that it would be challenging for either normal neutron stars or ergostars in a hypermassive state to be the progenitors of short $\gamma$-ray bursts.