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A. G. Doroshkevich
Researcher at Russian Academy of Sciences
Publications - 75
Citations - 1811
A. G. Doroshkevich is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Cosmology & Dark matter. The author has an hindex of 19, co-authored 73 publications receiving 1699 citations. Previous affiliations of A. G. Doroshkevich include Lebedev Physical Institute & Keldysh Institute of Applied Mathematics.
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Spatial structure of perturbations and origin of galactic rotation in fluctuation theory
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Gauss - Legendre sky pixelization (GLESP) for CMB maps
A. G. Doroshkevich,Pavel Naselsky,Pavel Naselsky,Oleg V. Verkhodanov,Dmitry Novikov,V. I. Turchaninov,Igor D. Novikov,P. R. Christensen,Lung-Yih Chiang +8 more
TL;DR: A new scheme of sky pixelization is developed for CMB maps based on the Gauss–Legendre polynomials zeros and allows one to create strict orthogonal expansion of the map.
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Two-dimensional simulation of the gravitational system dynamics and formation of the large-scale structure of the universe
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Review of scientific topics for the Millimetron space observatory
Nikolai S. Kardashev,Igor D. Novikov,Igor D. Novikov,V. N. Lukash,Sergei Vladimirovich Pilipenko,Elena V. Mikheeva,D. V. Bisikalo,D. Wiebe,A. G. Doroshkevich,A. V. Zasov,Igor Zinchenko,Igor Zinchenko,Pavel B. Ivanov,V. I. Kostenko,T. I. Larchenkova,S. F. Likhachev,I. F. Malov,Valery Mikhajlovich Malofeev,Alexey Stepanovich Pozanenko,Andrey Smirnov,A. M. Sobolev,Anatolii M. Cherepashchuk,Yuri Shchekinov +22 more
TL;DR: In this paper, a wide range of questions in astrophysics and cosmology can be answered by astronomical observations in the far-IR to millimeter wavelength range and which include the formation and evolution of stars and planets, galaxies and the interstellar medium, the study of black holes, and the development of the cosmological model.
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Formation of structure in a universe with unstable neutrinos
TL;DR: In this article, the influence of neutrinos massifs vis-a-vis des desintegrations ν H →ν L +μ(f) on the processus de formation de la structure dans l'Univers is discussed.