activity
20062024
most citedOn possible interpretations of the high energy electron-positron spectrum measured by the Fermi Large Area Telescope

263 citations · 574 across the 18 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2024

Nonlinear feedback of the electrostatic instability on the blazar-induced pair beam and GeV cascade

Mahmoud Alawashra, Martin Pohl

Relativistic pair beams produced in the cosmic voids by TeV gamma rays from blazars are expected to produce a detectable GeV-scale cascade that is missing in the observations. The…

astro-ph.IM2023★ 1 cited

Interpolation of Instrument Response Functions for the Cherenkov Telescope Array in the Context of pyirf

Rune Michael Dominik, Maximilian Linhoff, Julian Sitarek

The Cherenkov Telescope Array (CTA) will be the next generation ground-based very-high-energy gamma-ray observatory, constituted by tens of Imaging Atmospheric Cherenkov Telescopes…

astro-ph.HE2023

Variability studies of active galactic nuclei from the long-term monitoring program with the Cherenkov Telescope Array

Guillaume Grolleron, Josefa Becerra González, Jonathan Biteau +13

Blazars are active galactic nuclei (AGN) with a relativistic jet oriented toward the observer. This jet is composed of accelerated particles which can display emission over the ent…

astro-ph.HE2023

Evolution of Relativistic Pair Beams: Implications for Laboratory and TeV Astrophysics

Marvin Beck, Oindrila Ghosh, Florian Grüner +5

Missing cascades from TeV blazar beams indicate that collective plasma effects may play a significant role in their energy loss. It is possible to mimic the evolution of such highl…

astro-ph.GA2023★ 43 cited

Electron-Ion Temperature Ratio in Astrophysical Shocks

John C. Raymond, Parviz Ghavamian, Artem Bohdan +9

Collisionless shock waves in supernova remnants and the solar wind heat electrons less effectively than they heat ions, as is predicted by kinetic simulations. However, the values…

physics.plasm-ph2023★ 11 cited

Pre-acceleration in the Electron Foreshock II: Oblique Whistler Waves

Paul J. Morris, Artem Bohdan, Martin S. Weidl +3

Thermal electrons have gyroradii many orders of magnitude smaller than the finite width of a shock, thus need to be pre-accelerated before they can cross it and be accelerated by d…