Mario Pitschmann

756 total citations
35 papers, 488 citations indexed

About

Mario Pitschmann is a scholar working on Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics and Astronomy and Astrophysics. According to data from OpenAlex, Mario Pitschmann has authored 35 papers receiving a total of 488 indexed citations (citations by other indexed papers that have themselves been cited), including 25 papers in Atomic and Molecular Physics, and Optics, 23 papers in Nuclear and High Energy Physics and 16 papers in Astronomy and Astrophysics. Recurrent topics in Mario Pitschmann's work include Cosmology and Gravitation Theories (16 papers), Atomic and Subatomic Physics Research (12 papers) and Particle physics theoretical and experimental studies (8 papers). Mario Pitschmann is often cited by papers focused on Cosmology and Gravitation Theories (16 papers), Atomic and Subatomic Physics Research (12 papers) and Particle physics theoretical and experimental studies (8 papers). Mario Pitschmann collaborates with scholars based in Austria, France and Russia. Mario Pitschmann's co-authors include A. N. Ivanov, H. Abele, N. I. Troitskaya, Philippe Brax, Tobias Jenke, M. Wellenzohn, Sebastian M. Schmidt, Craig D. Roberts, Chien-Yeah Seng and Michael J. Ramsey-Musolf and has published in prestigious journals such as Physical Review Letters, SHILAP Revista de lepidopterología and Physics Letters B.

In The Last Decade

Mario Pitschmann

33 papers receiving 477 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Mario Pitschmann Austria 14 316 269 195 84 48 35 488
Ion I. Cotǎescu Romania 11 292 0.9× 151 0.6× 246 1.3× 100 1.2× 5 0.1× 68 398
V. V. Flambaum Australia 7 387 1.2× 436 1.6× 205 1.1× 51 0.6× 30 0.6× 10 624
T. N. Sherry Ireland 12 368 1.2× 161 0.6× 152 0.8× 152 1.8× 10 0.2× 60 519
Vincenzo Branchina Italy 16 652 2.1× 176 0.7× 408 2.1× 114 1.4× 4 0.1× 43 800
David Smith United States 14 1.4k 4.6× 132 0.5× 676 3.5× 92 1.1× 13 0.3× 19 1.5k
Maxim Pospelov United States 20 1.2k 3.7× 282 1.0× 687 3.5× 176 2.1× 13 0.3× 29 1.3k
B. Hamil Algeria 16 300 0.9× 333 1.2× 248 1.3× 378 4.5× 6 0.1× 64 603
Gilad Pérez Israel 17 707 2.2× 461 1.7× 367 1.9× 49 0.6× 36 0.8× 41 1.0k
Jnanadeva Maharana India 14 620 2.0× 166 0.6× 289 1.5× 266 3.2× 12 0.3× 84 675
V. N. Pervushin Russia 12 400 1.3× 72 0.3× 139 0.7× 67 0.8× 6 0.1× 95 488

Countries citing papers authored by Mario Pitschmann

Since Specialization
Citations

This map shows the geographic impact of Mario Pitschmann'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 Mario Pitschmann with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Mario Pitschmann more than expected).

Fields of papers citing papers by Mario Pitschmann

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Mario Pitschmann. 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 Mario Pitschmann. The network helps show where Mario Pitschmann may publish in the future.

Co-authorship network of co-authors of Mario Pitschmann

This figure shows the co-authorship network connecting the top 25 collaborators of Mario Pitschmann. A scholar is included among the top collaborators of Mario Pitschmann 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 Mario Pitschmann. Mario Pitschmann 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.
Koch, Benjamin, et al.. (2026). Equivalence of scalar-tensor theories and scale-dependent gravity. Classical and Quantum Gravity. 43(4). 45012–45012.
2.
Intravaia, F., et al.. (2024). Force Metrology with Plane Parallel Plates: Final Design Review and Outlook. Physics. 6(2). 690–741. 4 indexed citations
3.
Abele, H., et al.. (2024). Search for environment-dependent dilatons. Physics of the Dark Universe. 43. 101419–101419. 11 indexed citations
4.
Pitschmann, Mario, et al.. (2023). Green’s function analysis of the neutron Lloyd interferometer. Zeitschrift für Naturforschung A. 78(7). 651–658. 2 indexed citations
5.
Pitschmann, Mario, et al.. (2023). New method for directly computing reduced density matrices. Physical review. D. 107(1). 13 indexed citations
6.
Pitschmann, Mario, et al.. (2023). Dilaton-induced open quantum dynamics. The European Physical Journal C. 83(8). 15 indexed citations
7.
Koch, Benjamin, et al.. (2023). Vacuum Energy, the Casimir Effect, and Newton’s Non-Constant. Universe. 9(11). 476–476. 2 indexed citations
8.
Brax, Philippe, et al.. (2022). The environment dependent dilaton in the laboratory and the solar system. The European Physical Journal C. 82(10). 934–934. 18 indexed citations
9.
Pitschmann, Mario, et al.. (2022). Density Matrix Formalism for Interacting Quantum Fields. Universe. 8(11). 601–601. 10 indexed citations
10.
Jenke, Tobias, et al.. (2021). Gravity resonance spectroscopy and dark energy symmetron fields. The European Physical Journal Special Topics. 230(4). 1131–1136. 16 indexed citations
11.
Brax, Philippe & Mario Pitschmann. (2018). Exact solutions to nonlinear symmetron theory: One- and two-mirror systems. Physical review. D. 97(6). 23 indexed citations
12.
Cronenberg, G., Roman Höllwieser, Tobias Jenke, et al.. (2016). Exact solution for chameleon field, self-coupled through the Ratra-Peebles potential withn=1and confined between two parallel plates. Physical review. D. 94(8). 20 indexed citations
13.
Pitschmann, Mario, Chien-Yeah Seng, Craig D. Roberts, & Sebastian M. Schmidt. (2015). Nucleon tensor charges and electric dipole moments. Physical review. D. Particles, fields, gravitation, and cosmology. 91(7). 39 indexed citations
14.
Ivanov, A. N., Mario Pitschmann, & M. Wellenzohn. (2015). Effective low-energy gravitational potential for slow fermions coupled to linearized massive gravity. Physical review. D. Particles, fields, gravitation, and cosmology. 92(10). 3 indexed citations
15.
Ivanov, A., Mario Pitschmann, N. I. Troitskaya, & Y. Berdnikov. (2014). Bound-stateβ−decay of the neutron re-examined. Physical Review C. 89(5). 7 indexed citations
16.
Mantry, Sonny, Mario Pitschmann, & Michael J. Ramsey-Musolf. (2014). Distinguishing axions from generic light scalars using electric dipole moment and fifth-force experiments. Physical review. D. Particles, fields, gravitation, and cosmology. 90(5). 21 indexed citations
17.
Faber, M., A. N. Ivanov, P. Kienle, J. Márton, & Mario Pitschmann. (2011). MOLECULE MODEL FOR KAONIC NUCLEAR CLUSTER $\bar{K}NN$. International Journal of Modern Physics E. 20(6). 1477–1490. 1 indexed citations
18.
Faber, M., A. N. Ivanov, В. А. Иванов, et al.. (2009). Continuum-state and bound-stateβ−-decay rates of the neutron. Physical Review C. 80(3). 18 indexed citations
19.
Kryshen, E., et al.. (2008). Time Modulation of theβ+-Decay Rate of H-LikePr58+140Ions. Physical Review Letters. 101(18). 182501–182501. 19 indexed citations
20.
Fischer, Peter, et al.. (2003). Space/time non-commutative field theories and causality. The European Physical Journal C. 29(1). 133–141. 27 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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2026