In this article we review the current state of the field of solar neutrinos, including flavor
oscillations, nonstandard effects, solar models, cross section measurements, and the broad …

We compute a new generation of standard solar models (SSMs) that includes recent
updates on some important nuclear reaction rates and a more consistent treatment of the …

The fundamental processes by which nuclear energy is generated in the Sun have been
known for many years. However, continuous progress in areas such as neutrino …

We explore the variation in single-star 15–30${M} _ {\odot} $, nonrotating, solar metallicity,
pre-supernova MESA models that is due to changes in the number of isotopes in a fully …

Since the first observations of solar oscillations in 1960, helioseismology has probably been
one of the most successful fields of astrophysics. Data of unprecedented quality were …

Continuum atomic processes initiated by photons and electrons occurring in a plasma are
fundamental in plasma physics, playing a key role in the determination of ionization balance …

The internal solar structure predicted by the standard solar model disagrees with the
helioseismic observations even by utilizing the most updated physical inputs, such as the …

We study the impact of new metallicity measurements, from solar wind data, on the solar
model. The" solar modeling problem" refers to the persisting discrepancy between …

Parameters of electron-impact (Stark) broadening and shift of spectral lines are of key
importance in various studies of plasma spectroscopy and astrophysics. To overcome the …

We critically examine recent claims of a high solar metallicity by von Steiger & Zurbuchen (,)
based on in situ measurements of the solar wind, rather than the standard spectroscopically …