• Corpus ID: 118482129

Electroweak Hall Effect of Neutrino and Coronal Heating

@article{Ishikawa2015ElectroweakHE,
  title={Electroweak Hall Effect of Neutrino and Coronal Heating},
  author={Kenzo Ishikawa and Yutaka Tobita},
  journal={arXiv: High Energy Physics - Phenomenology},
  year={2015}
}

• K. Ishikawa, Y. Tobita
• Published 25 March 2015
• Physics
• arXiv: High Energy Physics - Phenomenology

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.