Germano Nardini
About
In The Last Decade
Germano Nardini
39 papers receiving 2.2k citations
Hit Papers
Peers
Comparison fields: 5 of 37
- Astronomy and Astrophysics 2.0k
- Nuclear and High Energy Physics 1.7k
- Atomic and Molecular Physics, and Optics 138
- Oceanography 136
- Statistical and Nonlinear Physics 96
Countries citing papers authored by Germano Nardini
This map shows the geographic impact of Germano Nardini'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 Germano Nardini with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Germano Nardini more than expected).
Fields of papers citing papers by Germano Nardini
This network shows the impact of papers produced by Germano Nardini. 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 Germano Nardini. The network helps show where Germano Nardini may publish in the future.
Co-authorship network of co-authors of Germano Nardini
This figure shows the co-authorship network connecting the top 25 collaborators of Germano Nardini. A scholar is included among the top collaborators of Germano Nardini 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 Germano Nardini. Germano Nardini is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 7 | |
| 2 | 1 | |
| 3 | 10 | |
| 4 | 9 | |
| 5 | 25 | |
| 6 | 4 | |
| 7 | 31 | |
| 8 | 34 | |
| 9 | 43 | |
| 10 | 1 | |
| 11 | 96 | |
| 12 | 45 | |
| 13 | 8 | |
| 14 | 4 | |
| 15 | Dark matter versus $h → γγ$ and $h → γZ$ with supersymmetric triplets | 8 |
| 16 | Dark matter versus h ! and h ! Z with supersymmetric triplets | 5 |
| 17 | 45 | |
| 18 | 15 | |
| 19 | 45 | |
| 20 | 127 |
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.