We review the application of the one-dimensional Mixing Length Theory (MLT) model of
convection in stellar interiors and low-mass stellar evolution. We summarize the history of …

The origins of the elements and isotopes of cosmic material is a critical aspect of
understanding the evolution of the universe. Nucleosynthesis typically requires physical …

A bstract We present an updated global analysis of neutrino oscillation data as of September
2024. The parameters θ 12, θ 13,\(\Delta {m} _ {21}^ 2\), and\(\mid\Delta {m} _ {3\ell} …

As a free, intensive, rarely interactive, and well directional messenger, solar neutrinos have
been driving both solar physics and neutrino physics developments for more than half a …

In this paper, we report the first measurement of CNO solar neutrinos by Borexino that uses
the correlated integrated directionality (CID) method, exploiting the subdominant Cherenkov …

A bstract A series of experiments studying neutrinos from intense radioactive sources have
reported a deficit in the measured event rate which, in combination, has reached a statistical …

Context. The Sun acts as a cornerstone of stellar physics. Thanks to spectroscopic,
helioseismic and neutrino flux observations, we can use the Sun as a laboratory of …

The nature of dark matter in the Universe is one of the hardest unsolved problems in modern
physics. Indeed, on one hand, the overwhelming indirect evidence from astrophysics seems …

A bstract We determine the solar neutrino fluxes from the global analysis of the most up-to-
date terrestrial and solar neutrino data including the final results of the three phases of …

Axions, if discovered, could serve as a powerful new messenger for studying astrophysical
objects. In this study we show how the Sun's spatial and spectral" axion image" can be …