On the Possible Enhancement of the Magnetic Field by Neutrino Reemission Processes in the Mantle of a Supernova

Details On the Possible Enhancement of the Magnetic Field by Neutrino Reemission Processes in the Mantle of a Supernova On the Possible Enhancement of the Magnetic Field by Neutrino Reemission Processes in the Mantle of a Supernova

1999-09-09

arxiv.org/abs/astro-ph/9909154v1

JETP Lett. 69 (1999) 365-370

Astronomy and Astrophysics

Astrophysics

8 pages, latex

Scientific paper

URCA neutrino reemission processes under the conditions in the mantle of a supernova with a strong toroidal magnetic field are investigated. It is shown that parity violation in these processes can be manifested macroscopically as a torque that rapidly spins up the region of the mantle occupied by such a field. Neutrino spin-up of the mantle can strongly affect the mechanism of further generation of the toroidal field, specifically, it can enhance the field in a small neighborhood of the rigid-body-rotating core of the supernova remnant.

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