Recycling of Neutron Stars in Common Envelopes and Hypernova Explosions
Maxim V. Barkov, Serguei S. Komissarov

TL;DR
This paper proposes a new supernova explosion mechanism in binary systems involving neutron stars and common envelope phases, leading to highly energetic explosions and unique remnants like magnetars or Wolf-Rayet binaries.
Contribution
It introduces a novel model where neutron star accretion and magnetic field amplification cause supernova explosions with distinctive observational features.
Findings
Explosion energies up to 10^52 erg.
Supernovae with high luminosity and steep light curves.
Remnants as magnetars or Wolf-Rayet star binaries.
Abstract
In this paper we propose a new plausible mechanism of supernova explosions specific to close binary systems. The starting point is the common envelope phase in the evolution of a binary consisting of a red super giant and a neutron star. As the neutron star spirals towards the center of its companion it spins up via disk accretion. Depending on the specific angular momentum of gas captured by the neutron star via the Bondi-Hoyle mechanism, it may reach millisecond periods either when it is still inside the common envelope or after it has merged with the companion core. The high accretion rate may result in strong differential rotation of the neutron star and generation of the magnetar-strength magnetic field. The magnetar wind can blow away the common envelope if its magnetic field is as strong as G, and can destroy the entire companion if it is as strong as G. The…
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