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E. M. D. G. D. Pino

3 papers hereh-index 14 citations8 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
same name
  • E. M. D. G. D. Pino — 2 papers, h 7
  • E. M. D. G. D. Pino — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedCosmic Ray Acceleration by Turbulence-Driven Magnetic Reconnection and the Origin of the Neutrinos in NGC 1068

1 citations · 1 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025★ 1 cited

Cosmic Ray Acceleration by Turbulence-Driven Magnetic Reconnection and the Origin of the Neutrinos in NGC 1068

Luana Passos-Reis, Elisabete M. de Gouveia Dal Pino, Juan Carlos Rodríguez-Ramírez +1

The Seyfert Type II galaxy NGC 1068 has been identified as a potential neutrino source by IceCube, with a 4.2σ significance detection of a 79−20+22​ neutrino excess from 2…

astro-ph.HE2025

Cosmic Ray Transport and Gamma-Ray Signatures in the Interstellar Medium

Lucas Barreto-Mota, Elisabete M. de Gouveia Dal Pino, Siyao Xu +4

The interaction of cosmic rays (CRs) with magnetic fields and the interstelar medium (ISM) leads to the production of nonthermal radiation. Although this has been a topic of study…

astro-ph.HE2018

Neutrino and γ-ray Emission from the Core of NGC1275 by Magnetic Reconnection: GRMHD Simulations and Radiative Transfer/Particle Calculations

J. C. Rodríguez-Ramírez, E. M. de Gouveia Dal Pino, R. Alves Batista

Very high energy (VHE) emission has been detected from the radio galaxy NGC1275, establishing it as a potential cosmic-ray (CR) accelerator and a high energy neutrino source. We he…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.