Marta Orselli

1.7k total citations
36 papers, 683 citations indexed

About

Marta Orselli is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Statistical and Nonlinear Physics. According to data from OpenAlex, Marta Orselli has authored 36 papers receiving a total of 683 indexed citations (citations by other indexed papers that have themselves been cited), including 28 papers in Astronomy and Astrophysics, 28 papers in Nuclear and High Energy Physics and 7 papers in Statistical and Nonlinear Physics. Recurrent topics in Marta Orselli's work include Black Holes and Theoretical Physics (25 papers), Cosmology and Gravitation Theories (16 papers) and Pulsars and Gravitational Waves Research (15 papers). Marta Orselli is often cited by papers focused on Black Holes and Theoretical Physics (25 papers), Cosmology and Gravitation Theories (16 papers) and Pulsars and Gravitational Waves Research (15 papers). Marta Orselli collaborates with scholars based in Italy, Denmark and Sweden. Marta Orselli's co-authors include Troels Harmark, G. Grignani, Gordon W. Semenoff, Davide Astolfi, Valentina Giangreco M. Puletti, A. Placidi, Alessandro Nagar, Simone Albanesi, Sebastiano Bernuzzi and Niels A. Obers and has published in prestigious journals such as Nuclear Physics B, Monthly Notices of the Royal Astronomical Society and Physics Letters B.

In The Last Decade

Marta Orselli

34 papers receiving 655 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Marta Orselli Italy 14 564 488 166 35 35 36 683
Francesco Nitti France 12 1.1k 1.9× 729 1.5× 196 1.2× 32 0.9× 51 1.5× 27 1.1k
Julia Fang United States 8 338 0.6× 322 0.7× 211 1.3× 26 0.7× 48 1.4× 13 492
Amitabha Lahiri India 13 598 1.1× 444 0.9× 205 1.2× 27 0.8× 85 2.4× 58 668
Guido Festuccia United States 13 850 1.5× 579 1.2× 238 1.4× 114 3.3× 75 2.1× 21 945
Toshifumi Noumi Japan 17 750 1.3× 614 1.3× 244 1.5× 19 0.5× 114 3.3× 39 851
Claudio A. Scrucca Switzerland 18 1.0k 1.8× 665 1.4× 230 1.4× 29 0.8× 23 0.7× 36 1.1k
Nabamita Banerjee India 14 493 0.9× 376 0.8× 165 1.0× 18 0.5× 89 2.5× 38 546
Oleg Andreev Germany 19 1.2k 2.1× 500 1.0× 238 1.4× 43 1.2× 67 1.9× 54 1.2k
Satish D. Joglekar India 9 801 1.4× 160 0.3× 102 0.6× 26 0.7× 77 2.2× 50 855
Rudranil Basu India 12 560 1.0× 455 0.9× 338 2.0× 58 1.7× 60 1.7× 26 607

Countries citing papers authored by Marta Orselli

Since Specialization
Citations

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

Fields of papers citing papers by Marta Orselli

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Marta Orselli

This figure shows the co-authorship network connecting the top 25 collaborators of Marta Orselli. A scholar is included among the top collaborators of Marta Orselli 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 Marta Orselli. Marta Orselli 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.
Orselli, Marta, et al.. (2025). Charged binaries in gravitational tides. Journal of Cosmology and Astroparticle Physics. 2025(2). 28–28. 6 indexed citations
2.
Placidi, A., et al.. (2025). Direct current memory effects in effective-one-body waveform models. Physical review. D. 111(4). 4 indexed citations
3.
Grignani, G., et al.. (2025). Strong-gravity precession resonances for binary systems orbiting a Schwarzschild black hole. Physical review. D. 112(4). 3 indexed citations
4.
Harmark, Troels, et al.. (2024). Binary mergers in strong gravity background of Kerr black hole. Monthly Notices of the Royal Astronomical Society. 531(1). 1884–1904. 14 indexed citations
5.
Placidi, A., et al.. (2023). 2.5PN accurate waveform information for generic-planar-orbit binaries in effective one-body models. Physical review. D. 108(2). 12 indexed citations
6.
Grignani, G., et al.. (2023). Tidal deformations of a binary system induced by an external Kerr black hole. Physical review. D. 107(8). 16 indexed citations
7.
Albanesi, Simone, A. Placidi, Alessandro Nagar, Marta Orselli, & Sebastiano Bernuzzi. (2022). New avenue for accurate analytical waveforms and fluxes for eccentric compact binaries. Physical review. D. 105(12). 37 indexed citations
8.
Dias, Óscar J. C., G. Grignani, Troels Harmark, et al.. (2022). Blandford-Znajek monopole expansion revisited: novel non-analytic contributions to the power emission. Journal of Cosmology and Astroparticle Physics. 2022(7). 32–32. 17 indexed citations
9.
Pina, D. Marín, et al.. (2022). Event horizon of a charged black hole binary merger. Physical review. D. 106(8). 7 indexed citations
10.
Placidi, A., Simone Albanesi, Alessandro Nagar, et al.. (2021). Exploiting Newton-factorized, 2PN-accurate, waveform multipoles in effective-one-body models for spin-aligned noncircularized binaries. arXiv (Cornell University). 35 indexed citations
11.
Grignani, G., Troels Harmark, & Marta Orselli. (2018). Existence of the Blandford-Znajek monopole for a slowly rotating Kerr black hole. Physical review. D. 98(8). 7 indexed citations
12.
Grignani, G., et al.. (2016). Born-Infeld/gravity correspondence. Physical review. D. 94(6). 7 indexed citations
13.
Grignani, G., et al.. (2014). Thermal DBI action for the D3-brane at weak and strong coupling. Journal of High Energy Physics. 2014(3). 12 indexed citations
14.
Grignani, G., et al.. (2012). Thermal string probes in AdS and finite temperature Wilson loops. Journal of High Energy Physics. 2012(6). 19 indexed citations
15.
Astolfi, Davide, Valentina Giangreco M. Puletti, G. Grignani, Troels Harmark, & Marta Orselli. (2011). Finite-size corrections for quantum strings on $ {\text{Ad}}{{\text{S}}_4} \times \mathbb{C}{P^3} $. Journal of High Energy Physics. 2011(5). 13 indexed citations
16.
Astolfi, Davide, Valentina Giangreco M. Puletti, G. Grignani, Troels Harmark, & Marta Orselli. (2010). Full Lagrangian and Hamiltonian for quantum strings on AdS4 × CP 3 in a near plane wave limit. Journal of High Energy Physics. 2010(4). 17 indexed citations
17.
Astolfi, Davide, Troels Harmark, G. Grignani, & Marta Orselli. (2008). Finite-size corrections to the rotating string and the winding state. Journal of High Energy Physics. 2008(8). 99–99. 10 indexed citations
18.
Harmark, Troels, Kristján Kristjánsson, & Marta Orselli. (2007). Magnetic Heisenberg-chain/pp-wave correspondence. Journal of High Energy Physics. 2007(2). 85–85. 10 indexed citations
19.
Grignani, G., Marta Orselli, Gordon W. Semenoff, & Diego Trancanelli. (2003). The superstring Hagedorn temperature in a pp-wave background. Journal of High Energy Physics. 2003(6). 6–6. 22 indexed citations
20.
Grignani, G., Marta Orselli, & Gordon W. Semenoff. (2001). The target space depenedence of the Hagedorn temperature. Journal of High Energy Physics. 2001(11). 58–58. 8 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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