2 citations · 2 across the 2 of their papers we have counts for
7 papers
Geometry, Not Calorimetry, Drives the Radio/Infrared/Gamma-Ray Correlation
Troy A. Porter, Igor V. Moskalenko, Gudlaugur Johannesson
We investigate whether the observed radio-infrared--ray correlation in star-forming galaxies is a geometric effect rather than a signature of local cosmic-ray (CR) calorimetry.…
Gamma-ray signature of superluminous supernovae: Fermi-LAT GeV detection of SN 2017egm and evidence of a central engine
F. Acero, A. Acharyya, A. Adelfio +116
Superluminous supernovae (SLSNe) are a rare class of transients with peak luminosities 10-100 times greater than those of standard core-collapse supernovae (SNe). The mechanisms po…
Simulating the Diffuse Neutrino Emission from the Milky Way with GALPROP
P. D. Marinos, T. A. Porter, G. P. Rowell +2
We use the GALPROP cosmic ray (CR) propagation framework to model the diffuse neutrino and gamma-ray emissions from the Galaxy. A collection of realistic bounding models are develo…
Characterizing Candidate Blazar Counterparts of the Ultra-High-Energy Event KM3-230213A
KM3NeT Collaboration, MessMapp Group, LAT Collaboration +13
High-energy astrophysical neutrinos serve as crucial messengers for understanding hadronic acceleration processes and identifying the origins of cosmic rays, with blazars among the…
Very Local Impact on the Spectrum of Cosmic-Ray Nuclei below 100 TeV
Mikhail Malkov, Igor Moskalenko, Patrick Diamond +1
Recent measurements of primary and secondary CR spectra, their arrival directions, and our improved knowledge of the magnetic field geometry around the heliosphere allow us to set…
On the Temporal Variability of the Galactic Multi-TeV Interstellar Emissions
P. D. Marinos, T. A. Porter, G. P. Rowell +2
We use the GALPROP cosmic ray (CR) framework to model the Galactic CR distributions and associated non-thermal diffuse emissions up to PeV energies. We consider ensembles of discre…