A. Meregaglia

22 papers receiving 552 citations

Hit Papers

The GENIE neutrino Monte Carlo generator20092026201420202009100200300

Peers

A. Meregaglia
Comparison fields: 5 of 25
  • Nuclear and High Energy Physics 552
  • Astronomy and Astrophysics 50
  • Statistical and Nonlinear Physics 47
  • Atomic and Molecular Physics, and Optics 33
  • Radiation 26
Replace V. A. Naumov with:
V. A. Naumov Russia
B. Ostrick Germany
J. Spitz United States
Th. Thümmler Germany
Alexander Nozik Russia
F. Terranova Italy
F. Vannucci Switzerland
H. K. Walter Switzerland
K. Sudhakar India
T. Sanuki Japan
A. Meregaglia relative to V. A. Naumov Russia V. A. Naumov's profile →
Citations per field
00.5×3.4×
V. A. Naumov · 1×
Citations per year

Countries citing papers authored by A. Meregaglia

Since Specialization
Citations

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

Fields of papers citing papers by A. Meregaglia

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of A. Meregaglia

This figure shows the co-authorship network connecting the top 25 collaborators of A. Meregaglia. A scholar is included among the top collaborators of A. Meregaglia 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 A. Meregaglia. A. Meregaglia 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
#WorkIndexed citations
1 0
2 2
3 6
4 22
5 4
6 0
7 12
8 6
9 0
10 4
11 18
12
The GENIE neutrino Monte Carlo generatorbreakdown →
350
13 4
14 24
15 42
16 1
17 46
18 1
19 2
20 7

About A. Meregaglia

A. Meregaglia is a scholar working on Nuclear and High Energy Physics, Radiation and Statistical and Nonlinear Physics, having authored 25 papers that have together received 567 indexed citations. Recurring topics across this work include Neutrino Physics Research (18 papers), Particle physics theoretical and experimental studies (17 papers) and Dark Matter and Cosmic Phenomena (9 papers). The work is most often cited by research in Nuclear and High Energy Physics (552 citations), Statistical and Nonlinear Physics (47 citations) and Astronomy and Astrophysics (50 citations). A. Meregaglia has collaborated with scholars based in France, Switzerland and Italy. Frequent co-authors include A. Rubbia, C. Andreopoulos, H. Gallagher, F. Cavanna, J. E. Y. Dobson, S. Dytman, Pauli Kehayias, P. Guzowski, D. Bhattacharya and A. J. Bell. Their work appears in journals such as Journal of High Energy Physics, New Journal of Physics and Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment.

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