We review and analyze the available information on the nuclear-fusion cross sections that
are most important for solar energy generation and solar neutrino production. We provide …

Oscillations detected on the solar surface provide a unique opportunity for investigations of
the interior properties of a star. Through major observational efforts, including extensive …

Low-energy cross section data for 86 charged-particle induced reactions involving light (1⩽
Z⩽ 14), mostly stable, nuclei are compiled. The corresponding Maxwellian-averaged …

We present a large and updated stellar evolution database for low-, intermediate-, and high-
mass stars in a wide metallicity range, suitable for studying Galactic and extragalactic simple …

We calculate accurate solar models and report the detailed time dependences of important
solar quantities. We use helioseismology to constrain the luminosity evolution of the Sun …

A wealth of new experimental and theoretical results has been obtained in solar physics
since the first edition of this textbook appeared in 1989. Thus all nine chapters have been …

We present a thorough analysis of the current solar neutrino data, in the context of two-flavor
active neutrino oscillations. We aim at performing an accurate and exhaustive statistical …

Helioseismology has allowed us to study the structure of the Sun in unprecedented detail.
One of the triumphs of the theory of stellar evolution was that helioseismic studies had …

▪ Abstract Low-mass particles, such as neutrinos, axions, other Nambu-Goldstone bosons,
and gravitons, are produced in the hot and dense interior of stars. Therefore, astrophysical …

This review is focused on neutrino mixing and neutrino oscillations in the light of the recent
experimental developments. After discussing possible types of neutrino mixing for Dirac and …