Electroweak Hall Effect of Neutrino and Coronal Heating

The inversion of temperature at the solar corona is hard to understand from classical physics, and the coronal heating mechanism remains unclear. The heating in the quiet region seems contradicting with the thermodynamics and is a keen problem for physicists. A new mechanism for the coronal heating...

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Bibliographic Details
Published in:arXiv.org 2015-03
Main Authors: Ishikawa, Kenzo, Tobita, Yutaka
Format: Article
Language:English
Subjects:
Hall effect
Heating
Physicists
Solar corona
Solar neutrinos
Online Access:Get full text
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Summary:The inversion of temperature at the solar corona is hard to understand from classical physics, and the coronal heating mechanism remains unclear. The heating in the quiet region seems contradicting with the thermodynamics and is a keen problem for physicists. A new mechanism for the coronal heating based on the neutrino radiative transition unique in the corona region is studied. The probability is enormously amplified by an electroweak Chern-Simons form and overlapping waves, and the sufficient energy is transfered. Thus the coronal heating is understood from the quantum effects of the solar neutrino.
ISSN:2331-8422