Relativistic effects in the solar EOS
Astrophysics
2007-05-23 v1
Abstract
We study the sensitivity of the sound speed to relativistic corrections of the equation of state (EOS) in the standard solar model by means of a helioseismic forward analysis. We use the latest GOLF/SOHO data for modes to confirm that the inclusion of the relativistic corrections to the adiabatic exponent computed from both OPAL and MHD EOS leads to a more reliable theoretical modelling of the innermost layers of the Sun.
Cite
@article{arxiv.astro-ph/0107381,
title = {Relativistic effects in the solar EOS},
author = {A. Bonanno and A. L. Murabito and L. Paterno'},
journal= {arXiv preprint arXiv:astro-ph/0107381},
year = {2007}
}
Comments
3 pages, 3 figures, aa.cls, to appear on Astronomy and Astrophysics