Sajal Mukherjee

554 total citations
20 papers, 213 citations indexed

About

Sajal Mukherjee is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Statistical and Nonlinear Physics. According to data from OpenAlex, Sajal Mukherjee has authored 20 papers receiving a total of 213 indexed citations (citations by other indexed papers that have themselves been cited), including 19 papers in Astronomy and Astrophysics, 10 papers in Nuclear and High Energy Physics and 6 papers in Statistical and Nonlinear Physics. Recurrent topics in Sajal Mukherjee's work include Pulsars and Gravitational Waves Research (12 papers), Astrophysical Phenomena and Observations (11 papers) and Cosmology and Gravitation Theories (9 papers). Sajal Mukherjee is often cited by papers focused on Pulsars and Gravitational Waves Research (12 papers), Astrophysical Phenomena and Observations (11 papers) and Cosmology and Gravitation Theories (9 papers). Sajal Mukherjee collaborates with scholars based in India, Czechia and Slovakia. Sajal Mukherjee's co-authors include Sumanta Chakraborty, S. Mitra, R. K. Nayak, Naresh Dadhich, Sourav Chatterjee, Sayak Datta, Georgios Lukes-Gerakopoulos, Indranil Chakraborty, Nicholas Loutrel and Andrea Maselli and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Physics Letters B and Journal of High Energy Physics.

In The Last Decade

Sajal Mukherjee

20 papers receiving 207 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Sajal Mukherjee India 10 204 122 34 14 6 20 213
Roberto Oliveri France 10 198 1.0× 168 1.4× 49 1.4× 7 0.5× 5 0.8× 16 224
Kenta Hioki Japan 4 429 2.1× 324 2.7× 35 1.0× 21 1.5× 3 0.5× 6 431
Z. Stuchlík Czechia 7 375 1.8× 315 2.6× 35 1.0× 11 0.8× 9 1.5× 10 391
Saeed Ullah Khan China 11 278 1.4× 172 1.4× 28 0.8× 9 0.6× 1 0.2× 21 290
Thomas F. M. Spieksma Portugal 8 203 1.0× 117 1.0× 14 0.4× 23 1.6× 3 0.5× 10 243
Arne Grenzebach Germany 5 417 2.0× 320 2.6× 37 1.1× 41 2.9× 3 0.5× 7 440
Wan-Zhe Feng United States 13 170 0.8× 301 2.5× 22 0.6× 10 0.7× 3 0.5× 22 313
J. W. Richardson United States 5 95 0.5× 50 0.4× 16 0.5× 41 2.9× 3 0.5× 8 125
Prashant Kocherlakota United States 10 367 1.8× 254 2.1× 26 0.8× 29 2.1× 4 0.7× 13 390
O. S. Stashko Ukraine 8 97 0.5× 100 0.8× 35 1.0× 33 2.4× 2 0.3× 20 147

Countries citing papers authored by Sajal Mukherjee

Since Specialization
Citations

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

Fields of papers citing papers by Sajal Mukherjee

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Sajal Mukherjee

This figure shows the co-authorship network connecting the top 25 collaborators of Sajal Mukherjee. A scholar is included among the top collaborators of Sajal Mukherjee 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 Sajal Mukherjee. Sajal Mukherjee 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.
Chakraborty, Indranil, et al.. (2025). Signatures of gravitational wave memory in the radiative process of entangled quantum probes. Physical review. D. 111(2). 3 indexed citations
2.
Loutrel, Nicholas, Sajal Mukherjee, Andrea Maselli, & Paolo Pani. (2024). Analytical model of precessing binaries using post-Newtonian theory in the extreme mass-ratio limit: General formalism. Physical review. D. 110(2). 4 indexed citations
3.
Mukherjee, Sajal, et al.. (2024). Detectability of stochastic gravitational wave background from weakly hyperbolic encounters. Astronomy and Astrophysics. 684. A17–A17. 5 indexed citations
4.
Mukherjee, Sajal, et al.. (2023). Resonance crossing of a charged body in a magnetized Kerr background: An analog of extreme mass ratio inspiral. Physical review. D. 107(6). 11 indexed citations
5.
Mukherjee, Sajal & Sumanta Chakraborty. (2023). Transition from inspiral to plunge for braneworld EMRI. Classical and Quantum Gravity. 40(14). 145013–145013. 5 indexed citations
6.
Chakraborty, Indranil, et al.. (2023). Entanglement harvesting for different gravitational wave burst profiles with and without memory. Journal of High Energy Physics. 2023(9). 7 indexed citations
7.
Mukherjee, Sajal, Georgios Lukes-Gerakopoulos, & R. K. Nayak. (2022). Extended bodies moving on geodesic trajectories. General Relativity and Gravitation. 54(9). 2 indexed citations
8.
Mukherjee, Sajal & Naresh Dadhich. (2022). Pure Gauss–Bonnet NUT black hole solution: I. The European Physical Journal C. 82(4). 2 indexed citations
9.
Mukherjee, Sajal, S. Mitra, & Sourav Chatterjee. (2021). Gravitational wave observatories may be able to detect hyperbolic encounters of black holes. Monthly Notices of the Royal Astronomical Society. 508(4). 5064–5073. 31 indexed citations
10.
Datta, Sayak & Sajal Mukherjee. (2021). Possible connection between the reflection symmetry and existence of equatorial circular orbit. Physical review. D. 103(10). 13 indexed citations
11.
Mukherjee, Sajal & Naresh Dadhich. (2020). Pure Gauss-Bonnet NUT black hole with and without non-central singularity. arXiv (Cornell University). 6 indexed citations
12.
Mukherjee, Sajal, et al.. (2020). Resonant orbits for a spinning particle in Kerr spacetime. Physical review. D. 101(12). 9 indexed citations
13.
Mukherjee, Sajal & Sumanta Chakraborty. (2020). Multipole moments of compact objects with NUT charge: Theoretical and observational implications. Physical review. D. 102(12). 15 indexed citations
14.
Mukherjee, Sajal, Sumanta Chakraborty, & Naresh Dadhich. (2019). On some novel features of the Kerr–Newman-NUT spacetime. The European Physical Journal C. 79(2). 20 indexed citations
15.
Mukherjee, Sajal & Sumanta Chakraborty. (2018). Horndeski theories confront the Gravity Probe B experiment. Physical review. D. 97(12). 25 indexed citations
16.
Mukherjee, Sajal. (2018). Periastron shift for a spinning test particle around naked singularities. Physical review. D. 97(12). 8 indexed citations
17.
Mukherjee, Sajal & R. K. Nayak. (2018). Collisional Penrose process and jets in Kerr naked singularity. Astrophysics and Space Science. 363(8). 9 indexed citations
18.
Mukherjee, Sajal. (2018). Collisional Penrose process with spinning particles. Physics Letters B. 778. 54–59. 26 indexed citations
19.
Mukherjee, Sajal & R. K. Nayak. (2018). Off-equatorial stable circular orbits for spinning particles. Physical review. D. 98(8). 9 indexed citations
20.
Mukherjee, Sajal & R. K. Nayak. (2017). Carter constant and angular momentum. International Journal of Modern Physics D. 27(1). 1750180–1750180. 3 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