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researcher

J. Rachen

161 papers hereh-index 9668.3k citations378 works total

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

author position
  • sole author3
  • first author7
  • middle author42
  • last author9

Across the 61 of 161 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO79
  • astro-ph.GA30
  • astro-ph.HE22
  • astro-ph.IM17
  • astro-ph9
  • physics.pop-ph2
same name
  • J. Rachen — 15 papers, h 13

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

activity
19952023
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 36.2k across the 158 of their papers we have counts for

collaborators
Showing 1998Show all

4 papers · 1 filter

astro-ph1998★ 330 cited

On the cosmic ray bound for models of extragalactic neutrino production

K. Mannheim, R. J. Protheroe, J. P. Rachen

We obtain the maximum diffuse neutrino intensity predicted by hadronic photoproduction models of the type which have been applied to the jets of active galactic nuclei or gamma ray…

astro-ph1998★ 13 cited

Cosmic Rays and Neutrinos from Gamma Ray Bursts

Jorg P. Rachen, P. Meszaros

We review the hypothesis that the acceleration of protons at internal shocks in Gamma Ray Bursts (GRB) could be the origin of the ultra-high energy cosmic rays (UHECR) observed at…

astro-ph1998★ 97 cited

On photohadronic processes in astrophysical environments

A. Muecke, J. P. Rachen, R. Engel +2

We discuss the first applications of our newly developed Monte Carlo event generator SOPHIA to multiparticle photoproduction of relativistic protons with thermal and power law radi…

astro-ph1998★ 315 cited

Photohadronic Neutrinos from Transients in Astrophysical Sources

Jorg P. Rachen, P. Meszaros

We investigate the spectrum of photohadronically produced neutrinos at very high energies (VHE, >10^14 eV) in astrophysical sources whose physical properties are constrained by the…

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