most citedSolar flux: Revisiting bounds on neutrino magnetic moments and solar magnetic field

17 citations · 18 across the 3 of their papers we have counts for

collaborators

6 papers

hep-ph2024

The next galactic supernova can uncover mass and couplings of particles decaying to neutrinos

Bernanda Telalovic, Damiano F. G. Fiorillo, Pablo Martínez-Miravé +2

Many particles predicted by extensions of the Standard Model feature interactions with neutrinos, e.g., Majoron-like bosons . If the mass of is larger than about 10 keV, the…

hep-ph2024

Effects of Neutrino-Ultralight Dark Matter Interaction on the Cosmic Neutrino Background

Pablo Martínez-Miravé, Yuber F. Perez-Gonzalez, Manibrata Sen

Ultralight dark matter interacting with sterile neutrinos would modify the evolution and properties of the cosmic neutrino background through active-sterile neutrino mixing. We inv…

astro-ph.HE2024

The Sun and core-collapse supernovae are leading probes of the neutrino lifetime

Pablo Martínez-Miravé, Irene Tamborra, Mariam Tórtola

The large distances travelled by neutrinos emitted from the Sun and core-collapse supernovae together with the characteristic energy of such neutrinos provide ideal conditions to p…

hep-ph20231 cited

Neutrino properties from the laboratory and the cosmos

Pablo Martínez-Miravé

Neutrinos are amongst the most abundant particles in the universe. The fact that they are massive particles proves that the Standard Model is an incomplete theory and needs to be e…

hep-ph2023

Neutrino CPT violation in the solar sector

Gabriela Barenboim, Pablo Martínez-Miravé, Christoph A. Ternes +1

In this paper we place new bounds on CPT violation in the solar neutrino sector analyzing the results from solar experiments and KamLAND. We also discuss the sensitivity of the nex…

hep-ph202217 cited

Solar flux: Revisiting bounds on neutrino magnetic moments and solar magnetic field

Evgeny Akhmedov, Pablo Martínez-Miravé

The interaction of neutrino transition magnetic dipole moments with magnetic fields can give rise to the phenomenon of neutrino spin-flavour precession (SFP). For Majorana neutrino…