Zobrazeno 1 - 10
of 57
pro vyhledávání: '"V. S. Imshennik"'
Publikováno v:
Mathematical Models and Computer Simulations. 10:695-708
The effect of generation of high-energy protons and carbon nuclei is identified in the threedimensional model of the interaction of a high-power electromagnetic field with plasma with supercritical density by the numerical solution of the Vlasov–Ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d61ffef5967a970dd1e7da577f459772
https://doi.org/10.1134/s2070048218060078
https://doi.org/10.1134/s2070048218060078
Publikováno v:
Physics of Atomic Nuclei. 81:76-87
Within a three-dimensionalmodel of interaction of a powerful electromagnetic fieldwith plasma of solid-state density, the effect of acceleration of calcium nuclei ( 20 48 Ca) to high energies that are likely to be sufficient for the synthesis of supe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b4c97ee2d664e35abfbc3d5b3076b5e
https://doi.org/10.1134/s1063778818010118
https://doi.org/10.1134/s1063778818010118
Autor:
V. S. Imshennik
Publikováno v:
Herald of the Russian Academy of Sciences. 87:348-355
The development of theoretical research on collapsing supernovae at the Keldysh Institute of Applied Mathematics and the Alikhanov Institute for Theoretical and Experimental Physics is discussed. This theme has been investigated for almost half a cen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f3fdfba2b02e7fa8ad268aeac674a208
https://doi.org/10.1134/s1019331617040098
https://doi.org/10.1134/s1019331617040098
Publikováno v:
Mathematical Models and Computer Simulations. 8:40-53
Numerical solution of the Vlasov–Maxwell equations in a three-dimensional (3D) model for the interaction between a powerful electromagnetic field of laser radiation and electron–proton plasma with a supercritical density yields kinetic functions
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cb3ca8724fbef058a94ee7e229bd6f26
https://doi.org/10.1134/s207004821601004x
https://doi.org/10.1134/s207004821601004x
Publikováno v:
Mathematical Models and Computer Simulations. 7:203-213
The effect of the generation of high-energy protons and relativistic electrons has been obtained in a three-dimensional model of the interaction between the powerful electromagnetic field and supercritical density plasma by the numerical solution of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::010c178f7051039e07a593d9bf78f427
https://doi.org/10.1134/s2070048215030059
https://doi.org/10.1134/s2070048215030059
Publikováno v:
Plasma Physics Reports. 38:153-168
A three-dimensional (3D) model of the interaction of laser radiation with plasma in the framework of Maxwell-Vlasov equations has been used to calculate the anomalous optical absorption in plasma of supercritical density. The results of calculations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::840604a33935de3bea87d284f56cf69d
https://doi.org/10.1134/s1063780x12020043
https://doi.org/10.1134/s1063780x12020043
Autor:
V. O. Molokanov, V. S. Imshennik
Publikováno v:
Astronomy Letters. 36:721-737
A quasi-one-dimensional hydrodynamic model for the collapse of a rotating iron stellar core is used to determine the neutrino spectra in the limiting case of total transparency to neutrino emission (without any deposition effect). The derived spectra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8b10c5b6c9dfb1dc481f72e0c0dc1848
https://doi.org/10.1134/s1063773710100038
https://doi.org/10.1134/s1063773710100038
Autor:
V. S. Imshennik
Publikováno v:
Physics of Atomic Nuclei. 73:625-633
The standard problem of a radial motion of test particles in the stationary gravitational field of a spherically symmetric celestial body is solved and is used to determine the time features of this motion. The problem is solved for the equations of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::51543f1efc50a1a2c897832796b4b30a
https://doi.org/10.1134/s1063778810040071
https://doi.org/10.1134/s1063778810040071
Autor:
V. O. Molokanov, V. S. Imshennik
Publikováno v:
Astronomy Letters. 35:799-815
We have ascertained an important role of rotation effects in a collapsing stellar core using a quasi-one-dimensional hydrodynamic model with a rigorous allowance for the neutrino energy losses including the neutrino opacity stage. However, the neutri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d6a96f9e547adcf3792edf43e878e857
https://doi.org/10.1134/s1063773709120019
https://doi.org/10.1134/s1063773709120019
Autor:
V. S. Imshennik
Publikováno v:
Astronomy Letters. 34:375-388
We consider the evolution of a neutron star binary system under the effect of two factors: gravitational radiation and mass transfer between the components. Gravitational radiation is specified under the justified assumption of a circular orbit and p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6af41b649c277280769c93412c92e348
https://doi.org/10.1134/s1063773708060029
https://doi.org/10.1134/s1063773708060029