S. Khan

770 total citations
32 papers, 614 citations indexed

About

S. Khan is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Statistical and Nonlinear Physics. According to data from OpenAlex, S. Khan has authored 32 papers receiving a total of 614 indexed citations (citations by other indexed papers that have themselves been cited), including 28 papers in Astronomy and Astrophysics, 18 papers in Nuclear and High Energy Physics and 5 papers in Statistical and Nonlinear Physics. Recurrent topics in S. Khan's work include Cosmology and Gravitation Theories (26 papers), Black Holes and Theoretical Physics (17 papers) and Pulsars and Gravitational Waves Research (8 papers). S. Khan is often cited by papers focused on Cosmology and Gravitation Theories (26 papers), Black Holes and Theoretical Physics (17 papers) and Pulsars and Gravitational Waves Research (8 papers). S. Khan collaborates with scholars based in Pakistan, Saudi Arabia and China. S. Khan's co-authors include Z. Yousaf, M. Z. Bhatti, Akbar Ali, Abeer M. Albalahi, Arooj Adeel, P. K. Sahoo, Adnan Malik, Abdel‐Haleem Abdel‐Aty, Haifa I. Alrebdi and Maxim Khlopov and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Annals of Physics and Classical and Quantum Gravity.

In The Last Decade

S. Khan

32 papers receiving 602 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
S. Khan Pakistan 16 524 345 89 79 19 32 614
Ifra Noureen Pakistan 15 601 1.1× 448 1.3× 187 2.1× 51 0.6× 8 0.4× 29 620
O. Troconis Brazil 5 560 1.1× 371 1.1× 97 1.1× 56 0.7× 6 0.3× 5 583
Ido Ben-Dayan Israel 14 531 1.0× 389 1.1× 47 0.5× 50 0.6× 4 0.2× 32 553
Simon Pekar France 5 479 0.9× 429 1.2× 94 1.1× 95 1.2× 14 0.7× 12 514
Sergio Dain Germany 17 633 1.2× 564 1.6× 13 0.1× 84 1.1× 12 0.6× 43 688
Ulf S. Nilsson Sweden 9 314 0.6× 257 0.7× 24 0.3× 73 0.9× 3 0.2× 17 337
Nadiezhda Montelongo García Portugal 8 580 1.1× 507 1.5× 78 0.9× 70 0.9× 8 592
Filipe C. Mena Portugal 12 418 0.8× 358 1.0× 29 0.3× 60 0.8× 2 0.1× 46 440
Farook Rahaman India 15 746 1.4× 536 1.6× 140 1.6× 53 0.7× 1 0.1× 52 763
Tayyaba Naz Pakistan 15 563 1.1× 386 1.1× 192 2.2× 61 0.8× 4 0.2× 36 609

Countries citing papers authored by S. Khan

Since Specialization
Citations

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

Fields of papers citing papers by S. Khan

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. Khan

This figure shows the co-authorship network connecting the top 25 collaborators of S. Khan. A scholar is included among the top collaborators of S. Khan 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 S. Khan. S. Khan 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.
Khan, S., et al.. (2025). Modeling of Finch-Skea hybrid neutron stars with complexity-free characteristics. Physica Scripta. 100(8). 85302–85302. 4 indexed citations
2.
Iqbal, Naveed, et al.. (2025). Non-static, torsion-inspired hyperbolically symmetric stars with anisotropy and dissipation. The European Physical Journal C. 85(11). 3 indexed citations
3.
Khan, S., et al.. (2025). Quasi-homologous evolution of dynamical relativistic stars in nonmetricity-induced gravity. Physics of the Dark Universe. 51. 102190–102190. 2 indexed citations
4.
Khan, S., et al.. (2025). Anisotropic stellar fluids with zero complexity factor in torsion-inspired gravity. Physics of the Dark Universe. 49. 101974–101974. 7 indexed citations
5.
Khan, S., et al.. (2025). Zhao profile-based black holes embedded in fuzzy halos under Hu–Sawicki f ( R ) gravity. Physics of the Dark Universe. 49. 102053–102053. 6 indexed citations
6.
Khan, S., et al.. (2025). Einasto-inspired non-commutative black holes within dark matter galactic halos in f(Q) gravity. Annals of Physics. 481. 170130–170130. 8 indexed citations
7.
Yousaf, Z., et al.. (2025). Modeling anisotropic dark energy self-gravitating stars satisfying the Karmarkar condition. Annals of Physics. 474. 169921–169921. 11 indexed citations
8.
Yousaf, Z., et al.. (2025). Construction of complexity-free anisotropic Dark Energy Stars. Physics of the Dark Universe. 47. 101811–101811. 5 indexed citations
9.
Yousaf, Z., S. Khan, Bander Almutairi, T. Ganesan, & M. Z. Bhatti. (2025). Gravitationally decoupled fuzzy black holes inspired by Einasto density profile. Chinese Journal of Physics. 97. 210–222. 2 indexed citations
10.
Khan, S., et al.. (2025). Einasto-core generalization of the Dymnikova regular black hole metric. The European Physical Journal C. 85(12). 3 indexed citations
11.
Albalahi, Abeer M., Z. Yousaf, S. Khan, & Akbar Ali. (2024). Anisotropic interior models with Kohler–Chao–Tikekar-like complexity factor. The European Physical Journal C. 84(9). 15 indexed citations
12.
Yousaf, Z., T. Ganesan, Bander Almutairi, M. Z. Bhatti, & S. Khan. (2024). Effect of Einasto spike on the gravitationally decoupled self-gravitating dark matter halos. Physica Scripta. 99(12). 125302–125302. 5 indexed citations
13.
Khan, S. & Z. Yousaf. (2024). Construction of fuzzy black holes and self-gravitational droplets in exponential f(R) gravity. Physica Scripta. 99(9). 95304–95304. 11 indexed citations
14.
Albalahi, Abeer M., M. Z. Bhatti, Akbar Ali, & S. Khan. (2024). Electromagnetic field on the complexity of minimally deformed compact stars. The European Physical Journal C. 84(3). 30 indexed citations
15.
Albalahi, Abeer M., Z. Yousaf, Akbar Ali, & S. Khan. (2024). Isotropization and complexity shift of gravitationally decoupled charged anisotropic sources. The European Physical Journal C. 84(1). 40 indexed citations
16.
Yousaf, Z., S. Khan, Nasser Bin Turki, & Takayuki Suzuki. (2024). Modeling of self-gravitating compact configurations using radial metric deformation approach. Chinese Journal of Physics. 89. 1595–1610. 22 indexed citations
17.
Khan, S., Arooj Adeel, & Z. Yousaf. (2024). Structure of anisotropic fuzzy dark matter black holes. The European Physical Journal C. 84(6). 43 indexed citations
18.
Yousaf, Z., M. Z. Bhatti, S. Khan, et al.. (2023). Stability of Anisotropy Pressure in Self-Gravitational Systems in f(G) Gravity. Axioms. 12(3). 257–257. 57 indexed citations
19.
Yousaf, Z., M. Z. Bhatti, & S. Khan. (2022). Stability Analysis of Isotropic Spheres in Einstein Gauss–Bonnet Gravity. Annalen der Physik. 534(10). 19 indexed citations
20.
Bhatti, M. Z., Z. Yousaf, & S. Khan. (2021). Role of quasi-homologous condition to study complex systems in $$f({\mathbb {G}}, T)$$ gravity. The European Physical Journal Plus. 136(9). 21 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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