activity
20212026
most citedRevisiting the propagation of highly-energetic gamma rays in the Galaxy

3 citations · 4 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2026

Cascades from ultra-high-energy neutrinos

Gaetano Di Marco, Rhorry Gauld, Rafael Alves Batista +2

Neutrinos produced at the highest energies can interact with cosmic neutrino and radiation backgrounds during their propagation to Earth. The many available , , and $νγ…

astro-ph.HE2026

Cosmic Ray Diffusion and the Origin of Very High Energy Gamma-Ray Emission in Young Massive Stellar Clusters

Lucas Barreto-Mota, Elisabete M. de Gouveia Dal Pino, Gaetano Di Marco +2

The search for Galactic sources capable of accelerating cosmic rays (CRs) to PeV energies has advanced significantly in recent years. High-energy observatories such as LHAASO have…

astro-ph.HE2026

Simulations of Electromagnetic Cascades in the Intergalactic Medium with Plasma Instabilities: the grplinst Code

Rafael Alves Batista, Andrey Saveliev

Electromagnetic cascades initiated by TeV gamma rays from distant blazars provide one of the cleanest indirect probes of the intergalactic medium and, in particular, of intergalact…

astro-ph.HE2026

The impact of gamma-ray propagation effects on indirect dark matter searches

Ignacio Martínez López, Rafael Alves Batista, Miguel A. Sánchez-Conde +1

In this work, we investigate dark matter (DM) detection in the context of weakly interacting massive particles (WIMPs). Upon annihilation, WIMPs generate cascades of secondary part…

hep-ph2025

Exploring New Propagation Scales With Galactic Neutrinos

Miller MacDonald, Kiara Carloni, Carlos A. Argüelles +2

The recent observation of high-energy Galactic neutrinos by IceCube allows for searches of new physics affecting neutrino propagation on scales of $O(10^9-10^{15})\,\mathrm{km/GeV}…

astro-ph.HE2025

CRPropa 3.3: Toward a Unified Multi-Messenger Framework from GeV to ZeV Energies

Sophie Aerdker, Rafael Alves Batista, Julia Becker Tjus +11

We present CRPropa 3.3, the latest release of the publicly available Monte Carlo framework for simulating the propagation of high-energy particles in astrophysical environments. Th…

astro-ph.HE2025

Spectra for the Vacuum Cherenkov Effect in Astrophysical Electromagnetic Cascades with Lorentz Invariance Violation

Andrey Saveliev, Rafael Alves Batista, Feodor Mishin

Lorentz invariance violation is a feature of several quantum gravity models in which Lorentz symmetry is broken at high energies, possibly leading to changes in particle behavior a…

astro-ph.HE2025★ 1 cited

Effects of extragalactic magnetic field on the spectra of ultra-high-energy cosmic rays from jetted sources

Sarah Soares Sippert, Carlos Magno R. da Costa, Rogerio M. de Almeida +2

The origins and acceleration mechanisms of ultra-high-energy cosmic rays (UHECRs) are unknown. Many models attribute their extreme energies to powerful astrophysical jets. Understa…

astro-ph.HE2024

The Quest for the Origins of Ultra-High-Energy Cosmic Rays

Rafael Alves Batista

Significant progress has been made over the past decades towards unveiling the sources of the most energetic particles in nature, the ultra-high-energy cosmic rays (UHECRs). Despit…

astro-ph.HE2024★ 3 cited

Revisiting the propagation of highly-energetic gamma rays in the Galaxy

Gaetano Di Marco, Rafael Alves Batista, Miguel Ángel Sánchez-Conde

Recent gamma-ray observations have detected photons up to energies of a few PeV. These highly energetic gamma rays are emitted by the most powerful sources in the Galaxy. Propagati…

astro-ph.HE2021

High-Energy Neutrino Production in Clusters of Galaxies

Saqib Hussain, Rafael Alves Batista, Elisabete de Gouveia Dal Pino +1

In this work, we compute the contribution from clusters of galaxies to the diffuse neutrino background. Clusters of galaxies can potentially produce cosmic rays (CRs) up to very-hi…

astro-ph.HE2021

High-Energy Neutrino Production in Clusters of Galaxies

Saqib Hussain, Rafael Alves Batista, Elisabete M. de Gouveia Dal Pino +1

Clusters of galaxies can potentially produce cosmic rays (CRs) up to very-high energies via large-scale shocks and turbulent acceleration. Due to their unique magnetic-field config…