Björn Eichmann

496 total citations
20 papers, 183 citations indexed

About

Björn Eichmann is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Electrical and Electronic Engineering. According to data from OpenAlex, Björn Eichmann has authored 20 papers receiving a total of 183 indexed citations (citations by other indexed papers that have themselves been cited), including 19 papers in Nuclear and High Energy Physics, 12 papers in Astronomy and Astrophysics and 1 paper in Electrical and Electronic Engineering. Recurrent topics in Björn Eichmann's work include Astrophysics and Cosmic Phenomena (18 papers), Dark Matter and Cosmic Phenomena (12 papers) and Neutrino Physics Research (11 papers). Björn Eichmann is often cited by papers focused on Astrophysics and Cosmic Phenomena (18 papers), Dark Matter and Cosmic Phenomena (12 papers) and Neutrino Physics Research (11 papers). Björn Eichmann collaborates with scholars based in Germany, Italy and France. Björn Eichmann's co-authors include J. Becker Tjus, S. M. Saba, Ali Kheirandish, F. Halzen, Lukas Merten, M. Kachelrieß, Foteini Oikonomou, Gero Müller, A. Dundovic and R.‐J. Dettmar and has published in prestigious journals such as The Astrophysical Journal, Astronomy and Astrophysics and Journal of Cosmology and Astroparticle Physics.

In The Last Decade

Björn Eichmann

18 papers receiving 167 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
Björn Eichmann Germany 7 174 118 4 3 2 20 183
Najimuddin Khan India 8 247 1.4× 148 1.3× 5 1.3× 3 1.0× 20 251
D. Kuempel Germany 3 180 1.0× 91 0.8× 7 1.8× 3 1.0× 6 181
A. Gurrola United States 10 218 1.3× 97 0.8× 2 0.5× 3 1.0× 19 222
A. Furniss United States 5 104 0.6× 90 0.8× 3 0.8× 5 1.7× 14 108
V. Fallah Ramazanı Finland 5 109 0.6× 108 0.9× 2 0.5× 4 1.3× 15 118
R. McFadden Australia 5 99 0.6× 86 0.7× 3 0.8× 2 0.7× 11 107
Anne-Kathrin Baczko Germany 5 112 0.6× 124 1.1× 2 0.5× 2 0.7× 6 128
J. Biteau France 6 140 0.8× 104 0.9× 2 0.5× 6 2.0× 13 143
L. Caramete Germany 6 84 0.5× 85 0.7× 2 0.5× 3 1.0× 11 97
G. Decerprit France 3 108 0.6× 53 0.4× 4 1.0× 2 0.7× 4 108

Countries citing papers authored by Björn Eichmann

Since Specialization
Citations

This map shows the geographic impact of Björn Eichmann's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by Björn Eichmann with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Björn Eichmann more than expected).

Fields of papers citing papers by Björn Eichmann

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Björn Eichmann. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by Björn Eichmann. The network helps show where Björn Eichmann may publish in the future.

Co-authorship network of co-authors of Björn Eichmann

This figure shows the co-authorship network connecting the top 25 collaborators of Björn Eichmann. A scholar is included among the top collaborators of Björn Eichmann based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with Björn Eichmann. Björn Eichmann is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Eichmann, Björn, et al.. (2025). Stochastic Acceleration in Weakly Turbulent Astrophysical Environments. The Astrophysical Journal. 981(1). 22–22.
2.
Schoeffler, K. M., Björn Eichmann, Fulvia Pucci, & Maria Elena Innocenti. (2025). Particle-in-cell simulations of the tearing instability for relativistic pair plasmas. Journal of Plasma Physics. 91(1).
3.
Padovani, P., E. Resconi, M. Ajello, et al.. (2024). High-energy neutrinos from the vicinity of the supermassive black hole in NGC 1068. Nature Astronomy. 8(9). 1077–1087. 14 indexed citations
4.
Eichmann, Björn, et al.. (2024). Possible jet contribution to the γ-ray luminosity in NGC 1068. Astronomy and Astrophysics. 687. A139–A139. 3 indexed citations
5.
Merten, Lukas, Rafael Alves Batista, J. Becker Tjus, et al.. (2023). CRPropa 3.2: a public framework for high-energy astroparticle simulations. arXiv (Cornell University). 1471–1471. 1 indexed citations
6.
Eichmann, Björn & M. Kachelrieß. (2023). Impact of the finite life-time of UHECR sources. Journal of Cosmology and Astroparticle Physics. 2023(2). 53–53. 3 indexed citations
7.
Eichmann, Björn, M. Kachelrieß, & Foteini Oikonomou. (2022). Explaining the UHECR spectrum, composition and large-scale anisotropies with radio galaxies. arXiv (Cornell University). 12 indexed citations
8.
Batista, Rafael Alves, J. Becker Tjus, A. Dundovic, et al.. (2022). CRPropa 3.2 — an advanced framework for high-energy particle propagation in extragalactic and galactic spaces. Journal of Cosmology and Astroparticle Physics. 2022(9). 35–35. 56 indexed citations
9.
Batista, Rafael Alves, J. Becker Tjus, A. Dundovic, et al.. (2021). CRPropa 3.2: a framework for high-energy astroparticle propagation. Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021). 978–978. 3 indexed citations
10.
Rachen, J. P. & Björn Eichmann. (2019). A parametrized catalog of radio galaxies as UHECR sources. ICRC. 36. 396. 2 indexed citations
11.
Eichmann, Björn. (2019). Summing up Ultra-High-Energy Cosmic Rays from Radio Galaxies. Journal of Physics Conference Series. 1181. 12028–12028. 1 indexed citations
12.
Winchen, T. & Björn Eichmann. (2019). Modification of the Energy Spectrum of UHECR by the Galactic Magnetic Field for Anisotropic Arrival Directions. Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019). 468–468. 1 indexed citations
13.
Eichmann, Björn. (2019). Ultra-high-energy cosmic rays by Cygnus A or the bulk of non-local radio galaxies?. Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019). 245–245. 3 indexed citations
14.
Merten, Lukas, J. Becker Tjus, Björn Eichmann, & R.‐J. Dettmar. (2017). On the non-thermal electron-to-proton ratio at cosmic ray acceleration sites. Astroparticle Physics. 90. 75–84. 15 indexed citations
15.
Tjus, J. Becker, Björn Eichmann, M. Kroll, & Nils Nierstenhöfer. (2016). Gamma-ray emitting supernova remnants as the origin of Galactic cosmic rays?. Astroparticle Physics. 81. 1–11. 6 indexed citations
16.
Kroll, M., J. Becker Tjus, Björn Eichmann, & Nils Nierstenhöfer. (2015). Gamma-ray emitting supernova remnants as the origin of Galactic cosmic rays. 2. 57–62. 2 indexed citations
17.
Tjus, J. Becker, Björn Eichmann, F. Halzen, Ali Kheirandish, & S. M. Saba. (2014). High-energy neutrinos from radio galaxies. Physical review. D. Particles, fields, gravitation, and cosmology. 89(12). 48 indexed citations
18.
Eichmann, Björn, R. Schlickeiser, & W. Rhode. (2012). DIFFERENCES OF LEPTONIC AND HADRONIC RADIATION PRODUCTION IN FLARING BLAZARS. The Astrophysical Journal. 749(2). 155–155. 7 indexed citations
19.
Eichmann, Björn, R. Schlickeiser, & W. Rhode. (2011). ON THE DURATION OF BLAZAR SYNCHROTRON FLARES. The Astrophysical Journal. 744(2). 153–153. 3 indexed citations
20.
Eichmann, Björn, R. Schlickeiser, & W. Rhode. (2009). Retardation of non-thermal photon light curves from flaring blazars. Astronomy and Astrophysics. 511. A26–A26. 3 indexed citations

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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