12 citations · 12 across the 1 of their papers we have counts for
4 papers
Simulating TeV gamma-ray morphologies of shell-type supernova remnants
Matteo Pais, Christoph Pfrommer
Supernova remnant (SNR) shocks provide favourable sites of cosmic ray (CR) proton acceleration if the local magnetic field direction is quasi-parallel to the shock normal. Using th…
Evolution and observational signatures of the cosmic ray electron spectrum in SN 1006
Georg Winner, Christoph Pfrommer, Philipp Girichidis +2
Supernova remnants (SNRs) are believed to be the source of Galactic cosmic rays (CRs). SNR shocks accelerate CR protons and electrons which reveal key insights into the non-thermal…
Constraining the coherence scale of the interstellar magnetic field using TeV gamma-ray observations of supernova remnants
Matteo Pais, Christoph Pfrommer, Kristian Ehlert +2
Galactic cosmic rays (CRs) are believed to be accelerated at supernova remnant (SNR) shocks. In the hadronic scenario the TeV gamma-ray emission from SNRs originates from decaying…
The effect of cosmic-ray acceleration on supernova blast wave dynamics
M. Pais, C. Pfrommer, K. Ehlert +1
Non-relativistic shocks accelerate ions to highly relativistic energies provided that the orientation of the magnetic field is closely aligned with the shock normal (quasi-parallel…