M. Malekjani

987 total citations
37 papers, 678 citations indexed

About

M. Malekjani is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Oceanography. According to data from OpenAlex, M. Malekjani has authored 37 papers receiving a total of 678 indexed citations (citations by other indexed papers that have themselves been cited), including 37 papers in Astronomy and Astrophysics, 25 papers in Nuclear and High Energy Physics and 3 papers in Oceanography. Recurrent topics in M. Malekjani's work include Cosmology and Gravitation Theories (37 papers), Galaxies: Formation, Evolution, Phenomena (30 papers) and Black Holes and Theoretical Physics (17 papers). M. Malekjani is often cited by papers focused on Cosmology and Gravitation Theories (37 papers), Galaxies: Formation, Evolution, Phenomena (30 papers) and Black Holes and Theoretical Physics (17 papers). M. Malekjani collaborates with scholars based in Iran, Greece and United Kingdom. M. Malekjani's co-authors include Mehdi Rezaei, Spyros Basilakos, Francesco Pace, Joan Solà, Eoin Ó Colgáin, M. M. Sheikh-Jabbari, Hosein Haghi, David F. Mota, S. Rahvar and Özgür Akarsu and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Physical review. D.

In The Last Decade

M. Malekjani

37 papers receiving 640 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
M. Malekjani Iran 17 655 420 57 54 29 37 678
Giovanni Cabass United States 16 538 0.8× 321 0.8× 40 0.7× 59 1.1× 54 1.9× 19 575
Vivian Miranda United States 14 587 0.9× 344 0.8× 56 1.0× 34 0.6× 55 1.9× 33 628
Lavrentios Kazantzidis Greece 11 576 0.9× 346 0.8× 40 0.7× 21 0.4× 28 1.0× 11 606
H. K. Jassal India 11 946 1.4× 669 1.6× 49 0.9× 79 1.5× 20 0.7× 22 968
D. Sapone Chile 15 957 1.5× 579 1.4× 79 1.4× 56 1.0× 59 2.0× 26 973
Matteo Biagetti Switzerland 15 492 0.8× 236 0.6× 38 0.7× 47 0.9× 90 3.1× 24 528
David M. Wilkinson United Kingdom 2 800 1.2× 422 1.0× 70 1.2× 41 0.8× 112 3.9× 2 811
Kavilan Moodley South Africa 13 712 1.1× 393 0.9× 48 0.8× 41 0.8× 63 2.2× 34 735
Siqi Liu China 5 627 1.0× 350 0.8× 73 1.3× 60 1.1× 50 1.7× 16 672
B. Rabii United Kingdom 8 814 1.2× 553 1.3× 49 0.9× 72 1.3× 41 1.4× 14 865

Countries citing papers authored by M. Malekjani

Since Specialization
Citations

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

Fields of papers citing papers by M. Malekjani

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Malekjani

This figure shows the co-authorship network connecting the top 25 collaborators of M. Malekjani. A scholar is included among the top collaborators of M. Malekjani 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 M. Malekjani. M. Malekjani 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.
Malekjani, M., et al.. (2025). ΛCDM model against cosmography: a possible deviation after DESI 2024. Monthly Notices of the Royal Astronomical Society. 537(1). 436–447. 12 indexed citations
2.
Malekjani, M., et al.. (2025). $$\varLambda $$CDM model against gravity-thermodynamics conjecture: observational constraints after DESI 2024. The European Physical Journal C. 85(1). 2 indexed citations
3.
Malekjani, M., et al.. (2025). Thermodynamics-gravity conjecture in the context of cosmography: observational constraints and potential deviations. The European Physical Journal C. 85(6). 1 indexed citations
4.
Malekjani, M., et al.. (2024). On redshift evolution and negative dark energy density in Pantheon + Supernovae. The European Physical Journal C. 84(3). 36 indexed citations
5.
Akarsu, Özgür, et al.. (2023). S 8 increases with effective redshift in ΛCDM cosmology. Monthly Notices of the Royal Astronomical Society Letters. 528(1). L20–L26. 36 indexed citations
6.
Malekjani, M., et al.. (2022). New parameterizations of generalized Chaplygin gas model constrained at background and perturbation levels. Journal of Astrophysics and Astronomy. 43(1). 2 indexed citations
7.
Rezaei, Mehdi & M. Malekjani. (2021). Comparison between different methods of model selection in cosmology. The European Physical Journal Plus. 136(2). 34 indexed citations
8.
Malekjani, M., et al.. (2021). A new comparison between holographic dark energy and standard $$\varLambda $$-cosmology in the context of cosmography method. The European Physical Journal C. 81(7). 6 indexed citations
9.
Malekjani, M., et al.. (2018). New parametrization for unified dark matter and dark energy. Physical review. D. 97(12). 10 indexed citations
10.
Rezaei, Mehdi, et al.. (2017). Constraints to Dark Energy Using PADE Parameterizations. The Astrophysical Journal. 843(1). 65–65. 57 indexed citations
11.
Rezaei, Mehdi & M. Malekjani. (2017). Spherical collapse model in agegraphic dark energy cosmologies. Physical review. D. 96(6). 10 indexed citations
12.
Malekjani, M., et al.. (2016). Growth of spherical overdensities in scalar–tensor cosmologies. Monthly Notices of the Royal Astronomical Society. 458(4). 3795–3807. 16 indexed citations
13.
Pace, Francesco, et al.. (2016). Constraints on shear and rotation with massive galaxy clusters. Monthly Notices of the Royal Astronomical Society. 465(3). 2687–2697. 17 indexed citations
14.
Malekjani, M., et al.. (2015). Effects of ghost dark energy perturbations on the evolution of spherical overdensities. Monthly Notices of the Royal Astronomical Society. 453(4). 4149–4159. 17 indexed citations
15.
Malekjani, M., et al.. (2015). Evolution of spherical overdensities in holographic dark energy models. Monthly Notices of the Royal Astronomical Society. 447(2). 1873–1884. 22 indexed citations
16.
Malekjani, M., et al.. (2013). Interacting Holographic Polytropic Gas Model of Dark Energy. International Journal of Theoretical Physics. 52(10). 3405–3412. 5 indexed citations
17.
Malekjani, M., et al.. (2011). The effect of cosmological background dynamics on the spherical collapse in MOND. New Astronomy. 17(2). 149–153. 2 indexed citations
18.
Malekjani, M., et al.. (2010). Cosmic behavior, statefinder diagnostic and w−w ′ analysis for interacting new agegraphic dark energy model in non-flat universe. Astrophysics and Space Science. 331(1). 265–273. 25 indexed citations
19.
Malekjani, M., S. Rahvar, & Hosein Haghi. (2009). SPHERICAL COLLAPSE IN MODIFIED NEWTONIAN DYNAMICS. The Astrophysical Journal. 694(2). 1220–1227. 13 indexed citations
20.
Malekjani, M., et al.. (2008). Two component baryonic–dark matter structure formation in top-hat model. New Astronomy. 14(4). 398–405. 4 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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