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.
Neutron Star Cooling
2004534 citationsD. G. Yakovlev, C. J. PethickAnnual Review of Astronomy and Astrophysicsprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by D. G. Yakovlev
Since
Specialization
Citations
This map shows the geographic impact of D. G. Yakovlev'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 D. G. Yakovlev with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. G. Yakovlev more than expected).
This network shows the impact of papers produced by D. G. Yakovlev. 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 D. G. Yakovlev. The network helps show where D. G. Yakovlev may publish in the future.
Co-authorship network of co-authors of D. G. Yakovlev
This figure shows the co-authorship network connecting the top 25 collaborators of D. G. Yakovlev.
A scholar is included among the top collaborators of D. G. Yakovlev 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 D. G. Yakovlev. D. G. Yakovlev is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Heinke, C. O., G. R. Sivakoff, Wynn C. G. Ho, et al.. (2013). 全CHANDRA X線観測衛星検出器によるCASSIOPEIA Aにおける中性子星の冷却の測定. The Astrophysical Journal. 777. 1–22.1 indexed citations
Gusakov, M. E., D. G. Yakovlev, P. Haensel, & Oleg Y. Gnedin. (2004). Direct Urca process in a neutron star mantle. Springer Link (Chiba Institute of Technology).16 indexed citations
6.
Yakovlev, D. G. & C. J. Pethick. (2004). Neutron Star Cooling. Annual Review of Astronomy and Astrophysics. 42(1). 169–210.534 indexed citations breakdown →
Verner, D. A. & D. G. Yakovlev. (1995). Analytic FITS for partial photoionization cross sections.. Data Archiving and Networked Services (DANS). 109(1). 125–133.51 indexed citations
15.
Baiko, D. A. & D. G. Yakovlev. (1995). Thermal and electrical conductivities of Coulomb crystals in neutron stars and white dwarfs. 21(5). 702–709.2 indexed citations
16.
Gnedin, Oleg Y., D. G. Yakovlev, & Yu. A. Shibanov. (1994). Neutron and proton superfluidity in cooling neutron stars. Astronomy Letters. 20(4). 409–415.5 indexed citations
17.
Kaminker, A. D. & D. G. Yakovlev. (1993). Neutrino pair synchrotron radiation of electrons and positrons in a hot plasma. Journal of Experimental and Theoretical Physics. 76(2). 229–235.
18.
Urpin, V. & D. G. Yakovlev. (1980). Thermogalvanomagnetic Effects in White Dwarfs and Neutron Stars. 24. 425.4 indexed citations
19.
Yakovlev, D. G.. (1975). Trajectories and the radiation emitted by particles falling into a rotating black hole. Journal of Experimental and Theoretical Physics. 41. 179.1 indexed citations
20.
Yakovlev, D. G.. (1973). Spectroscopy of a turbulent plasma. Soviet physics. Technical physics. 17. 1248.2 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.