Solar Core Homology, Solar Neutrinos and Helioseismology

Details Solar Core Homology, Solar Neutrinos and Helioseismology Solar Core Homology, Solar Neutrinos and Helioseismology

1995-11-22

arxiv.org/abs/astro-ph/9511107v4

Astrophys.J. 472 (1996) 412-418

Astronomy and Astrophysics

Astrophysics

14 pp., jnl.tex macro, minor corrections; accepted by Astrophysical Journal

Scientific paper

10.1086/178073

Precise numerical standard solar models (SSMs) now agree with one another and with helioseismological observations in the convective and outer radiative zones. Nevertheless these models obscure how luminosity, neutrino production and g-mode core helioseismology depend on such inputs as opacity and nuclear cross sections. Although the Sun is not homologous, its inner core by itself is chemically evolved and almost homologous, because of its compactness, radiative energy transport, and ppI-dominated luminosity production. We apply luminosity-fixed homology transformations to the core to estimate theoretical uncertainties in the SSM and to obtain a broad class of non-SSMs, parametrized by central temperature and density and purely radiative energy transport in the core.

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