Electroweak Hall Effect of Neutrino and Coronal Heating

TL;DR

This paper proposes a novel quantum-mechanical mechanism involving neutrino electroweak effects to explain the longstanding mystery of coronal heating and temperature inversion in the solar corona.

Contribution

It introduces a new coronal heating mechanism based on neutrino radiative transitions amplified by electroweak Chern-Simons effects, linking quantum physics to solar phenomena.

Findings

Neutrino radiative transition probability is significantly amplified in the corona.

Quantum effects of neutrinos can transfer sufficient energy for coronal heating.

The mechanism offers a new perspective on the temperature inversion in the solar corona.

Abstract

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.