Are Standard Solar Models Reliable?

John N. Bahcall, M. H. Pinsonneault, Sarbani Basu, and J. Christensen-Dalsgaard
Phys. Rev. Lett. 78, 171 – Published 13 January 1997
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Abstract

The sound speeds of solar models that include element diffusion agree with helioseismological measurements to a rms discrepancy of better than 0.2% throughout almost the entire Sun. Models that do not include diffusion, or in which the interior of the Sun is assumed to be significantly mixed, are effectively ruled out by helioseismology. Standard solar models predict the measured properties of the Sun more accurately than is required for applications involving solar neutrinos.

  • Received 24 September 1996

DOI:https://doi.org/10.1103/PhysRevLett.78.171

©1997 American Physical Society

Authors & Affiliations

John N. Bahcall

  • Institute for Advanced Study, Princeton, New Jersey 08540

M. H. Pinsonneault

  • Department of Astronomy, Ohio State University, Columbus, Ohio 43210

Sarbani Basu and J. Christensen-Dalsgaard

  • Theoretical Astrophysics Center, Danish National Research Foundation, and Institute for Physics and Astronomy, Aarhus University, DK 8000 Aarhus C, Denmark

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Vol. 78, Iss. 2 — 13 January 1997

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