The Adiabatic Exponent in the Solar Core

Astronomy and Astrophysics – Astronomy

Scientific paper

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Equation Of State, Sun: Interior, Sun: Oscillations

Scientific paper

We present helioseismic inversions of solar p-mode frequencies obtained by the Michelson Doppler Imager instrument of the Solar Oscillation Investigation project on board SOHO, which indicate a lower central value for the adiabatic exponent Gamma 1 in the Sun than in current models. We show how the inclusion of relativistic effects in the equation of state removes the discrepancy and allows almost perfect agreement in Gamma 1 between the models and the Sun. This increases our confidence both in the reliability of the equation-of-state calculation and the determination of solar p-mode frequencies.

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