activity
20052026
most citedCGC/saturation approach: a new impact-parameter dependent model in the next-to-leading order of perturbative QCD

19 citations · 69 across the 14 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2026

Quasi-Keplerian Be-Star Disks with Mimicking Viscosity

Michel Cure, Ignacio Araya, Rodrigo Meneses +5

Classical Be stars are fast-rotating B-type stars with gaseous quasi-Keplerian disks formed by equatorial ejection of material. While the viscous decretion disk (VDD) model reprodu…

hep-ph2025

Modified Homotopic approach for diffractive production

Carlos Contreras, José Garrido, Eugene Levin +1

We review the recent developments of the use of the homotopy method for solving the non-linear evolution equation for the diffractive production in deep inelastic scattering. We in…

hep-ph2024★ 2 cited

Modified homotopy approach for diffractive production in the saturation region

Carlos Contreras, José Garrido, Eugene Levin +1

In this paper we continue to develop the homotopy method for solving of the non linear evolution equation for the diffractive production in deep inelastic scattering(DIS). We intro…

hep-ph2023★ 3 cited

Homotopy solution to non-linear evolution for heavy nuclei

Carlos Contreras, Eugene Levin, Rodrigo Meneses

In the paper we suggest the homotopy method for solving of the non linear evolution equation. This method consists of two steps. First is the analytical solution for the linearized…

astro-ph.SR2022

Revisiting Viscous Transonic Decretion Disks of Be Stars

Michel Curé, Rodrigo Meneses, Ignacio Araya +4

In the context of Be stars, we restudied the viscous transonic decretion disk model of these stars. This model is driven by a radiative force due to an ensemble of optically-thin l…

hep-ph2020★ 5 cited

Non-linear equation in the re-summed next-to-leading order of perturbative QCD: the leading twist approximation

Carlos Contreras, Eugene Levin, Rodrigo Meneses +1

In this paper, we use the re-summation procedure, suggested in Refs.\cite{DIMST,SALAM,SALAM1,SALAM2}, to fix the BFKL kernel in the NLO. However, we suggest a different way to intr…