PREPRINT
B2910705-5890-484E-9A22-99276CEE7FC7

The determination of the internal structure of the sun by the density distribution

Hans J. Haubold, Arak Mathai Mathai
arXiv:math/9505213

Submitted on 19 May 1995

Abstract

This paper examines a number of analytic models which can describe the gravitationally stabilized fusion reactor of the Sun. An analytical multiparameter model is shown to reproduce various structure parameters such as density, mass, pressure and temperature throughout the solar core, which have been obtained by solving numerically the system of solar structure differential equations. For simplicity, numerical and analytical results are discussed in detail for a two-parameter model.

Preprint

Subjects: Mathematics - Classical Analysis and ODEs; Astrophysics

URL: https://arxiv.org/abs/math/9505213