Magnetorotational Mechanism of the Explosion of Core-Collapse Supernovae

TL;DR

This paper explores how magnetic fields and rotation in collapsing stars can drive supernova explosions, producing jets or equatorial ejections, with implications for neutrino signals and black hole formation.

Contribution

It introduces a magnetorotational mechanism for supernova explosions, emphasizing the role of magnetic field configurations and instabilities in energy transfer and matter ejection.

Findings

Magnetorotational instability facilitates energy transfer regardless of initial magnetic strength.

Different magnetic configurations lead to jet or equatorial matter ejection.

The model explains observed supernova energies and neutrino emission patterns.

Abstract

The idea of the magnetorotational explosion mechanism is that the energy of rotation of the neutron star formed in the course of a collapse is transformed into the energy of an expanding shock wave by means of a magnetic field. In the two-dimensional case, the time of this transformation depends weakly on the initial strength of the poloidal magnetic field because of the development of a magnetorotational instability. Differential rotation leads to the twisting and growth of the toroidal magnetic-field component, which becomes much stronger than the poloidal component. In the case where the initial configuration of the magnetic field is close to a dipole configuration, the ejection of matter has a jet character, whereas, in the case of a quadrupole configuration, there arises an equatorial ejection. In either case, the energy release is sufficient for explaining the observed average energy of supernova explosion. Neutrinos are emitted as the collapse and the formation of a rapidly rotating neutron star proceeds. In addition, neutrino radiation arises in the process of magnetorotational explosion owing to additional rotational-energy losses. In order to explain an interval of 4.5 hours between the two observed neutrino signals from SN 1987A, it is necessary to assume a weakening of the magnetorotional instability and a small initial magnetic field (10(9)-10(10)G) in the newly formed rotating neutron star. The existence of a black hole in the SN 1987A remnant could explain the absence of any visible pointlike source at the center of the explosion.