Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Vacuum nonsingular black hole
1992497 citationsIrina DymnikovaGeneral Relativity and Gravitationprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by Irina Dymnikova
Since
Specialization
Citations
This map shows the geographic impact of Irina Dymnikova'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 Irina Dymnikova with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Irina Dymnikova more than expected).
This network shows the impact of papers produced by Irina Dymnikova. 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 Irina Dymnikova. The network helps show where Irina Dymnikova may publish in the future.
Co-authorship network of co-authors of Irina Dymnikova
This figure shows the co-authorship network connecting the top 25 collaborators of Irina Dymnikova.
A scholar is included among the top collaborators of Irina Dymnikova 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 Irina Dymnikova. Irina Dymnikova is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Dymnikova, Irina, et al.. (2001). Limits on the Sizes of Fundamental Particles and Gravitational Mass of the Higgs Particle. Gravitation and Cosmology. 7. 122–130.4 indexed citations
Dymnikova, Irina. (1999). Dynamics of the cosmological term in a spherically symmetric case.. Gravitation and Cosmology. 5. 15–28.1 indexed citations
15.
Dymnikova, Irina & Maxim Khlopov. (1998). Self-consistent initial conditions in inflationary cosmology.. Gravitation and Cosmology. 4. 50–55.8 indexed citations
16.
Dymnikova, Irina. (1997). Internal structure of nonsingular spherical black holes. 13. 422.12 indexed citations
17.
Dymnikova, Irina. (1992). Vacuum nonsingular black hole. General Relativity and Gravitation. 24(3). 235–242.497 indexed citations breakdown →
18.
Dymnikova, Irina. (1986). Inflationary universe from the point of view of general relativity. Journal of Experimental and Theoretical Physics. 63(6). 1111.2 indexed citations
19.
Dymnikova, Irina. (1986). The inflationary universe and general relativity.. 90. 1900–1907.1 indexed citations
20.
Dymnikova, Irina, et al.. (1975). A nonsingular Friedmann cosmology. 1. 93.7 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.