Solar neutrino physics

XJ Xu, Z Wang, S Chen - Progress in Particle and Nuclear Physics, 2023 - Elsevier
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 …

[BOOK][B] Stars as laboratories for fundamental physics: The astrophysics of neutrinos, axions, and other weakly interacting particles

GG Raffelt - 1996 - books.google.com
For centuries the heavens have been a natural laboratory to test the classical laws of motion,
and more recently to test Einstein's theory of gravity. Today, astrophysics has become a vast …

Solar neutrinos and neutrino physics

M Maltoni, A Yu. Smirnov - The European Physical Journal A, 2016 - Springer
Solar neutrino studies triggered and largely motivated the major developments in neutrino
physics in the last 50 years. The theory of neutrino propagation in different media with matter …

Large neutrino secret interactions have a small impact on supernovae

DFG Fiorillo, GG Raffelt, E Vitagliano - Physical Review Letters, 2024 - APS
When hypothetical neutrino secret interactions (ν SI) are large, they form a fluid in a
supernova (SN) core, flow out with sonic speed, and stream away as a fireball. For the first …

Supernova emission of secretly interacting neutrino fluid: Theoretical foundations

DFG Fiorillo, GG Raffelt, E Vitagliano - Physical Review D, 2024 - APS
Neutrino-neutrino scattering could have a large secret component that would turn neutrinos
within a supernova (SN) core into a self-coupled fluid. Neutrino transport within the SN core …

Dirac neutrinos in dense matter

J Pantaleone - Physical Review D, 1992 - APS
The evolution of a supernova core can be dramatically different if the neutrinos trapped in
the core mix and/or flip helicity and escape as" sterile, right-handed" neutrinos. Thus the …

Do solar neutrinos decay?

JF Beacom, NF Bell - Physical Review D, 2002 - APS
Despite the fact that the solar neutrino flux is now well understood in the context of matter-
affected neutrino mixing, we find that it is not yet possible to set a strong and model …

Massive hidden photons as lukewarm dark matter

J Redondo, M Postma - Journal of Cosmology and Astroparticle …, 2009 - iopscience.iop.org
We study the possibility that a keV-MeV mass hidden photon (HP), ie a hidden sector U (1)
gauge boson, accounts for the observed amount of dark matter. We focus on the case where …

[HTML][HTML] Neutron-mirror neutron mixing and neutron stars

Z Berezhiani, R Biondi, M Mannarelli… - The European Physical …, 2021 - Springer
The oscillation of neutron n into mirror neutron\(n'\), its mass degenerate partner from dark
mirror sector, can gradually transform the neutron stars into the mixed stars consisting in part …

Neutrino physics

EK Akhmedov - arxiv preprint hep-ph/0001264, 2000 - arxiv.org
In the present lectures the following topics are considered: general properties of neutrinos,
neutrino mass phenomenology (Dirac and Majorana masses), neutrino masses in the …