Relativistic effects in the solar EOS. A helioseismic forward analysis

Details Relativistic effects in the solar EOS. A helioseismic forward analysis Relativistic effects in the solar EOS. A helioseismic forward analysis

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...375.1062b&link_type=abstract

Astronomy and Astrophysics, v.375, p.1062-1064 (2001)

Astronomy and Astrophysics

Astrophysics

2

Sun: Interior, Sun: Oscillations, Equation Of State

Scientific paper

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 l = 0, 1, 2, 3 modes to confirm that the inclusion of the relativistic corrections to the adiabatic exponent Gamma1 computed from both OPAL and MHD EOS leads to a more reliable theoretical modelling of the innermost layers of the Sun.

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