Yu. Eroshenko

928 total citations
9 papers, 611 citations indexed

About

Yu. Eroshenko is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Infectious Diseases. According to data from OpenAlex, Yu. Eroshenko has authored 9 papers receiving a total of 611 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 9 papers in Nuclear and High Energy Physics and 0 papers in Infectious Diseases. Recurrent topics in Yu. Eroshenko's work include Cosmology and Gravitation Theories (8 papers), Black Holes and Theoretical Physics (6 papers) and Galaxies: Formation, Evolution, Phenomena (3 papers). Yu. Eroshenko is often cited by papers focused on Cosmology and Gravitation Theories (8 papers), Black Holes and Theoretical Physics (6 papers) and Galaxies: Formation, Evolution, Phenomena (3 papers). Yu. Eroshenko collaborates with scholars based in Russia, Italy and France. Yu. Eroshenko's co-authors include V. I. Dokuchaev, Eugeny Babichev, С. В. Чернов, V. Berezinsky and M. Kachelrieß and has published in prestigious journals such as Physical Review Letters, Classical and Quantum Gravity and Journal of Experimental and Theoretical Physics.

In The Last Decade

Yu. Eroshenko

8 papers receiving 596 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
Yu. Eroshenko Russia	7	601	534	72	21	16	9	611
Pantelis S. Apostolopoulos Greece	11	363 0.6×	338 0.6×	77 1.1×	10 0.5×	16 1.0×	20	369
Naureen Goheer South Africa	11	505 0.8×	486 0.9×	128 1.8×	31 1.5×	21 1.3×	14	525
Edi Halyo United States	10	363 0.6×	430 0.8×	75 1.0×	15 0.7×	19 1.2×	25	455
Kh. Saaidi Iran	16	534 0.9×	442 0.8×	68 0.9×	59 2.8×	12 0.8×	46	544
Ritabrata Biswas India	13	399 0.7×	350 0.7×	131 1.8×	19 0.9×	28 1.8×	52	411
S. Ghaffari Iran	13	525 0.9×	441 0.8×	127 1.8×	27 1.3×	14 0.9×	20	540
H. Farajollahi Iran	14	571 1.0×	505 0.9×	68 0.9×	43 2.0×	7 0.4×	45	579
Burin Gumjudpai Thailand	9	476 0.8×	428 0.8×	75 1.0×	22 1.0×	11 0.7×	22	483
D. Kalligas United States	8	406 0.7×	355 0.7×	68 0.9×	25 1.2×	11 0.7×	10	415
Hiroki Yajima Japan	5	379 0.6×	341 0.6×	60 0.8×	17 0.8×	32 2.0×	6	386

Countries citing papers authored by Yu. Eroshenko

Since Specialization

Citations

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

Fields of papers citing papers by Yu. Eroshenko

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Yu. Eroshenko

This figure shows the co-authorship network connecting the top 25 collaborators of Yu. Eroshenko. A scholar is included among the top collaborators of Yu. Eroshenko 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 Yu. Eroshenko. Yu. Eroshenko is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

9 of 9 papers shown

1.

Babichev, Eugeny, V. I. Dokuchaev, & Yu. Eroshenko. (2012). Backreaction of accreting matter onto a black hole in the Eddington–Finkelstein coordinates. Classical and Quantum Gravity. 29(11). 115002–115002. 22 indexed citations

2.

Berezinsky, V., et al.. (2010). Superdense cosmological dark matter clumps. Physical review. D. Particles, fields, gravitation, and cosmology. 81(10). 35 indexed citations

3.

Berezinsky, V., et al.. (2010). Annihilations of superheavy dark matter in superdense clumps. Physical review. D. Particles, fields, gravitation, and cosmology. 81(10). 12 indexed citations

4.

Babichev, Eugeny, С. В. Чернов, V. I. Dokuchaev, & Yu. Eroshenko. (2008). Perfect fluid around black holes and naked singularities. arXiv (Cornell University). 1 indexed citations

5.

Babichev, Eugeny, С. В. Чернов, V. I. Dokuchaev, & Yu. Eroshenko. (2008). Ultrahard fluid and scalar field in the Kerr-Newman metric. Physical review. D. Particles, fields, gravitation, and cosmology. 78(10). 46 indexed citations

6.

Babichev, Eugeny, V. I. Dokuchaev, & Yu. Eroshenko. (2005). The accretion of dark energy onto a black hole. Journal of Experimental and Theoretical Physics. 100(3). 528–538. 99 indexed citations

7.

Babichev, Eugeny, V. I. Dokuchaev, & Yu. Eroshenko. (2004). Black Hole Mass Decreasing due to Phantom Energy Accretion. Physical Review Letters. 93(2). 21102–21102. 299 indexed citations

8.

Babichev, Eugeny, V. I. Dokuchaev, & Yu. Eroshenko. (2004). Dark energy cosmology with generalized linear equation of state. Classical and Quantum Gravity. 22(1). 143–154. 97 indexed citations

9.

Berezinsky, V., V. I. Dokuchaev, & Yu. Eroshenko. (2004). Small dark matter clumps and annihilation signal. Nuclear Physics B - Proceedings Supplements. 138. 25–27.

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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