activity
19992026
most citedTheoretical Constraints on the Vacuum Oscillation Solution to the Solar Neutrino Problem

41 citations · 70 across the 6 of their papers we have counts for

collaborators

6 papers

hep-ph2026

Archimedean Seesaw: Small Neutrino Masses and Large Lepton-number Violation

Tao Han, Alejandro Ibarra, Subhojit Roy +1

Contrary to the common lore that observable lepton-number violation (LNV) is inevitably suppressed by tiny neutrino masses, we identify a class of seesaw models in which arbitraril…

hep-ph2026

Leptogenesis without on-shell right-handed neutrinos

Simon Cléry, Alejandro Ibarra, Onur Yonar

We propose a novel mechanism for generating the baryon asymmetry of the Universe through leptogenesis in a scenario where the right-handed neutrinos are heavier than the maximal te…

hep-ph2026

Quantum effects on neutrino parameters from a flavored gauge boson

Alejandro Ibarra, Lukas Treuer

We calculate the one-loop renormalization group equations of the neutrino mass matrix when the Standard Model particle content is extended with a massive gauge boson which has fami…

hep-ph2024

Prospects for detecting the rare heavy Higgs decay through the channel at the LHC

M. A. Arroyo-Ureña, Alejandro Ibarra, Pablo Roig +1

We study the decay of a heavy CP-even neutral Higgs into an on-shell Standard Model-like Higgs boson and two photons, , in the two-Higgs doublet model. We argue that the…

hep-ph2006★ 29 cited

Hints on the high-energy seesaw mechanism from the low-energy neutrino spectrum

J. A. Casas, A. Ibarra, F. Jimenez-Alburquerque

It is an experimental fact that the mass ratio for the two heavier neutrinos, h = m_3/m_2 < 6, is much smaller than the typical quark and lepton hierarchies, which are O(20-300). W…

hep-ph1999★ 41 cited

Theoretical Constraints on the Vacuum Oscillation Solution to the Solar Neutrino Problem

J. A. Casas, J. R. Espinosa, A. Ibarra +1

The vacuum oscillation (VO) solution to the solar anomaly requires an extremely small neutrino mass splitting, Delta m^2_{sol}\leq 10^{-10} eV^2. We study under which circumstances…