В. М. Чечеткин
About
In The Last Decade
В. М. Чечеткин
132 papers receiving 1.3k citations
Peers
Comparison fields: 5 of 54
- Astronomy and Astrophysics 1.1k
- Nuclear and High Energy Physics 551
- Geophysics 123
- Computational Mechanics 86
- Atomic and Molecular Physics, and Optics 64
Countries citing papers authored by В. М. Чечеткин
This map shows the geographic impact of В. М. Чечеткин'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 В. М. Чечеткин with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites В. М. Чечеткин more than expected).
Fields of papers citing papers by В. М. Чечеткин
This network shows the impact of papers produced by В. М. Чечеткин. 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 В. М. Чечеткин. The network helps show where В. М. Чечеткин may publish in the future.
Co-authorship network of co-authors of В. М. Чечеткин
This figure shows the co-authorship network connecting the top 25 collaborators of В. М. Чечеткин. A scholar is included among the top collaborators of В. М. Чечеткин 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 В. М. Чечеткин. В. М. Чечеткин is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 0 | |
| 3 | On kinetic instabilities in collisionless ultra-relativistic streaming cold electron-proton plasma | 1 |
| 4 | Mass transfer in close binary stars | 53 |
| 5 | Driven-disk model for binaries with a precessing donor star: Three-dimensional simulations | 1 |
| 6 | Three-dimensional modeling of mass transfer in close binary systems with asynchronous rotation | 1 |
| 7 | Supernovae explosions in the presence of large-scale convective instability in a rotating protoneutron star | 0 |
| 8 | Evidence for the absence of a stream-disk shock interaction in semi-detached binary systems: Comparison of mathematical modeling results and observations | 10 |
| 9 | On the neutrino mechanism of supernova explosions | 4 |
| 10 | Studies of equilibrium configurations for a gaseous cloud near a gravitating center | 1 |
| 11 | A possible mechanism for the formation of molecular flows | 1 |
| 12 | Physical basis for nucleosynthesis of heavy elements | 4 |
| 13 | The structure of accretion disks in symbiotic stars: An isothermal case | 2 |
| 14 | Instability of the detonation wave in a thermonuclear supernova model | 1 |
| 15 | Production of light elements by cascades from energetic antiprotons in the early Universe and problems of nuclear cosmoarchaeology | 1 |
| 16 | Antiprotons in the Universe as a cosmological test of grand unification | 6 |
| 17 | Neutrino emission spectra of collapsing degenerate stellar cores - Calculations by the Monte Carlo method | 1 |
| 18 | Astrophysical constraints on the mass of heavy stable neutral leptons | 56 |
| 19 | Primordial black holes and the deuterium problem | 11 |
| 20 | Momentum and energy transfer by neutrino radiation to the mantle of a collapsing star and supernovae explosions | 1 |
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.