122 citations · 509 across the 9 of their papers we have counts for
7 papers
AAfrag 2.01: Interpolation routines for Monte Carlo results on secondary production including light antinuclei in hadronic interactions
M. Kachelriess, S. Ostapchenko, J. Tjemsland
Light antinuclei, like antideuteron and antihelium-3, are ideal probes for new, exotic physics because their astrophysical backgrounds are suppressed at low energies. In order to e…
ELMAG 3.01: A three-dimensional Monte Carlo simulation of electromagnetic cascades on the extragalactic background light and in magnetic fields
M. Blytt, M. Kachelriess, S. Ostapchenko
The version 3.01 of ELMAG, a Monte Carlo program for the simulation of electromagnetic cascades initiated by high-energy photons and electrons interacting with extragalactic backgr…
AAfrag: Interpolation routines for Monte Carlo results on secondary production in proton-proton, proton-nucleus and nucleus-nucleus interactions
M. Kachelriess, I. V. Moskalenko, S. Ostapchenko
We provide a compilation of predictions of the QGSJET-II-04m model for the production of secondary species (photons, neutrinos, electrons, positrons, and antinucleons) that are cov…
ELMAG: A Monte Carlo simulation of electromagnetic cascades on the extragalactic background light and in magnetic fields
M. Kachelriess, S. Ostapchenko, R. Tomas
A Monte Carlo program for the simulation of electromagnetic cascades initiated by high-energy photons and electrons interacting with extragalactic background light (EBL) is present…
Restricting UHECRs and cosmogenic neutrinos with Fermi-LAT
V. Berezinsky, A. Gazizov, M. Kachelriess +1
Ultrahigh energy cosmic ray (UHECR) protons interacting with the cosmic microwave background (CMB) produce UHE electrons and gamma-rays that in turn initiate electromagnetic cascad…
High energy neutrino yields from astrophysical sources II: Magnetized sources
M. Kachelriess, S. Ostapchenko, R. Tomas
We calculate the yield of high energy neutrinos produced in astrophysical sources for arbitrary interaction depths and magnetic field strengths . We take into account ener…