activity
19962022
most citedAssisted inflation via tachyon condensation

287 citations · 728 across the 38 of their papers we have counts for

collaborators

38 papers

hep-ph2022

Are neutrino oscillation mixings linked to the smallness of solar neutrino scale?

Eduardo Becerra-García, Abdel Pérez-Lorenzana

Observed reactor and atmospheric neutrino oscillation mixing values appear to be related to the neutrino scale ratio in a way that suggest that the ne…

astro-ph.CO2022★ 28 cited

Massive neutrino self-interactions with a light mediator in cosmology

Jorge Venzor, Gabriela Garcia-Arroyo, Abdel Pérez-Lorenzana +1

Nonstandard self-interactions can alter the evolution of cosmological neutrinos, mainly by damping free streaming, which should leave traces in cosmological observables. Although o…

hep-ph2021

Dirac CP phases in a 3+1 neutrino scenario with symmetry

Eduardo Becerra-García, Abdel Pérez-Lorenzana

A sterile neutrino in the scheme, where the sterile accounts for neutrino anomalies not explained solely by the weak active neutrinos, arises as a natural source for the brea…

hep-ph2020★ 1 cited

Small and solar neutrino oscillation parameters from symmetry

Abdel Pérez-Lorenzana

Exchange symmetry in the effective Majorana neutrino mass matrix does predict a maximal mixing for atmospheric neutrino oscillations asides to a null mixing that cannot be st…

hep-ph2020★ 47 cited

Bounds on neutrino-scalar nonstandard interactions from big bang nucleosynthesis

Jorge Venzor, Abdel Pérez-Lorenzana, Josue De-Santiago

Coherent forward scattering processes by neutrino-scalar nonstandard interactions (SNSI) induce an effective neutrino mass. In the Early Universe, a large neutrino effective mass r…

astro-ph.CO2020

Constraints on the velocity dispersion of Dark Matter from Cosmology and new bounds on scattering from the Cosmic Dawn

Iván Rodríguez-Montoya, Vladimir Ávila-Reese, Abdel Pérez-Lorenzana +1

The observational value of the velocity dispersion, , is missing in the Dark Matter (DM) puzzle. Non-zero or non-thermal DM velocities can drastically influence Large Sc…