Carmelo Evoli

3.5k total citations · 1 hit paper
56 papers, 1.8k citations indexed

About

Carmelo Evoli is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Atmospheric Science. According to data from OpenAlex, Carmelo Evoli has authored 56 papers receiving a total of 1.8k indexed citations (citations by other indexed papers that have themselves been cited), including 53 papers in Nuclear and High Energy Physics, 23 papers in Astronomy and Astrophysics and 5 papers in Atmospheric Science. Recurrent topics in Carmelo Evoli's work include Dark Matter and Cosmic Phenomena (47 papers), Astrophysics and Cosmic Phenomena (43 papers) and Neutrino Physics Research (14 papers). Carmelo Evoli is often cited by papers focused on Dark Matter and Cosmic Phenomena (47 papers), Astrophysics and Cosmic Phenomena (43 papers) and Neutrino Physics Research (14 papers). Carmelo Evoli collaborates with scholars based in Italy, Germany and United States. Carmelo Evoli's co-authors include Dario Grasso, Daniele Gaggero, Luca Maccione, Pasquale Blasi, Roberto Aloisio, Giovanni Morlino, Giuseppe Di Bernardo, Maurizio Giannotti, Alessandro Mirizzi and Alexandre Payez and has published in prestigious journals such as Physical Review Letters, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

Carmelo Evoli

52 papers receiving 1.8k citations

Hit Papers

Revisiting the SN1987A gamma-ray limit on ultralight axio... 2015 2026 2018 2022 2015 50 100 150 200

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Carmelo Evoli Italy 24 1.7k 1.1k 85 35 14 56 1.8k
Daniele Gaggero Italy 24 1.5k 0.9× 1.2k 1.1× 58 0.7× 21 0.6× 9 0.6× 63 1.8k
E. Orlando United States 13 1.2k 0.7× 1.0k 0.9× 49 0.6× 86 2.5× 33 2.4× 39 1.4k
R. Taillet France 18 1.3k 0.7× 805 0.7× 66 0.8× 37 1.1× 21 1.5× 35 1.3k
Philipp Mertsch Germany 19 960 0.6× 575 0.5× 35 0.4× 15 0.4× 14 1.0× 47 1.1k
T. A. Porter United States 20 1.6k 0.9× 1.2k 1.1× 57 0.7× 102 2.9× 52 3.7× 57 1.8k
B. L. Dingus United States 21 1.1k 0.6× 1.1k 1.0× 26 0.3× 17 0.5× 23 1.6× 87 1.3k
V. A. Dogiel Russia 15 1.1k 0.7× 938 0.8× 46 0.5× 25 0.7× 13 0.9× 65 1.3k
Giovanni Morlino Italy 21 1.2k 0.7× 1.0k 0.9× 32 0.4× 19 0.5× 4 0.3× 56 1.3k
P. Lipari Italy 25 2.4k 1.4× 513 0.5× 28 0.3× 17 0.5× 22 1.6× 67 2.4k
M. Ahlers United States 27 2.7k 1.5× 1.4k 1.3× 141 1.7× 20 0.6× 9 0.6× 77 2.7k

Countries citing papers authored by Carmelo Evoli

Since Specialization
Citations

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

Fields of papers citing papers by Carmelo Evoli

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Carmelo Evoli

This figure shows the co-authorship network connecting the top 25 collaborators of Carmelo Evoli. A scholar is included among the top collaborators of Carmelo Evoli 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 Carmelo Evoli. Carmelo Evoli 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.
Aloisio, Roberto, Antonio Ambrosone, & Carmelo Evoli. (2026). Constraining superheavy dark matter with the KM3-230213A neutrino event. Physical review. D. 113(4).
2.
Ambrosone, Antonio, et al.. (2025). The origin of very high-energy diffuse γ-ray emission: The case for galactic source cocoons. Astronomy and Astrophysics. 698. L18–L18.
3.
Evoli, Carmelo, et al.. (2023). TeV halos and the role of pulsar wind nebulae as sources of cosmic-ray positrons. Physical review. D. 107(12). 11 indexed citations
4.
Luque, Pedro De la Torre, Daniele Gaggero, Dario Grasso, et al.. (2023). Galactic diffuse gamma rays meet the PeV frontier. Astronomy and Astrophysics. 672. A58–A58. 27 indexed citations
5.
Dundovic, A., Carmelo Evoli, Daniele Gaggero, & Dario Grasso. (2021). Datafile for HERMES code. Springer Link (Chiba Institute of Technology). 22 indexed citations
6.
Evoli, Carmelo, et al.. (2021). Intermediate-mass and heavy Galactic cosmic-ray nuclei: The case of new AMS-02 measurements. Physical review. D. 103(12). 11 indexed citations
7.
Evoli, Carmelo, Elena Amato, Pasquale Blasi, & Roberto Aloisio. (2021). Galactic factories of cosmic-ray electrons and positrons. Physical review. D. 103(8). 40 indexed citations
8.
Evoli, Carmelo, Pasquale Blasi, Elena Amato, & Roberto Aloisio. (2020). Signature of Energy Losses on the Cosmic Ray Electron Spectrum. Physical Review Letters. 125(5). 51101–51101. 22 indexed citations
9.
Evoli, Carmelo, Giovanni Morlino, Pasquale Blasi, & Roberto Aloisio. (2020). AMS-02 beryllium data and its implication for cosmic ray transport. Physical review. D. 101(2). 80 indexed citations
10.
Dundovic, A., Oreste Pezzi, Pasquale Blasi, Carmelo Evoli, & W. H. Matthaeus. (2020). Novel aspects of cosmic ray diffusion in synthetic magnetic turbulence. Physical review. D. 102(10). 48 indexed citations
11.
Evoli, Carmelo, Giovanni Morlino, Pasquale Blasi, & Roberto Aloisio. (2019). The AMS-02 beryllium and its implication for Cosmic Ray transport. arXiv (Cornell University). 1 indexed citations
12.
Blasi, Pasquale, et al.. (2019). Atmospheric neutrinos and the knee of the cosmic ray spectrum. Astroparticle Physics. 114. 22–29. 5 indexed citations
13.
Galanti, Giorgio, F. Tavecchio, M. Roncadelli, & Carmelo Evoli. (2018). Photon-ALP oscillations from a blazar to us up to 1000 TeV. arXiv (Cornell University).
14.
Evoli, Carmelo, Pasquale Blasi, Giovanni Morlino, & Roberto Aloisio. (2018). Origin of the Cosmic Ray Galactic Halo Driven by Advected Turbulence and Self-Generated Waves. Physical Review Letters. 121(2). 21102–21102. 59 indexed citations
15.
Batista, Rafael Alves, M. Erdmann, Carmelo Evoli, et al.. (2015). CRPropa: A public framework to propagate UHECRs in the universe. Springer Link (Chiba Institute of Technology). 2 indexed citations
16.
Evoli, Carmelo, Daniele Gaggero, & Dario Grasso. (2015). Secondary antiprotons as a Galactic Dark Matter probe. INFM-OAR (INFN Catania). 43 indexed citations
17.
Gasperin, F. de, Carmelo Evoli, M. Brüggen, et al.. (2014). Discovery of the supernova remnant G351.0-5.4. Astronomy and Astrophysics. 568. A107–A107. 4 indexed citations
18.
Gaggero, Daniele, Luca Maccione, Giuseppe Di Bernardo, Carmelo Evoli, & Dario Grasso. (2013). Three-Dimensional Model of Cosmic-Ray Lepton Propagation Reproduces Data from the Alpha Magnetic Spectrometer on the International Space Station. Physical Review Letters. 111(2). 21102–21102. 67 indexed citations
19.
Evoli, Carmelo, Stefania Pandolfi, & Andrea Ferrara. (2013). Cosmic microwave background constraints on light dark matter candidates. Monthly Notices of the Royal Astronomical Society. 433(2). 1736–1744. 8 indexed citations
20.
Maccione, Luca, Carmelo Evoli, Daniele Gaggero, & Dario Grasso. (2011). DRAGON: Galactic Cosmic Ray Diffusion Code. Astrophysics Source Code Library. 5 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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