Quantum Astronomy. Part I
天体物理学
2007-05-23 v1
摘要
The article describes new model of the Sun having a hollow core as introduced in [1]. The model helps to explain a number of experimental facts of kinetics, energetics, and Sun spectroscopy based on classic physics. The origin of the Sun's energy is not the thermonuclear process taking place in its core, but the coherent, anisotropic, gravitational compression of the atomic hydrogen in the solar shell at the temperature of 6289 K.
关键词
引用
@article{arxiv.astro-ph/9912537,
title = {Quantum Astronomy. Part I},
author = {Alexander M. Ilyanok},
journal= {arXiv preprint arXiv:astro-ph/9912537},
year = {2007}
}
备注
In Russian