Zobrazeno 1 - 10
of 18
pro vyhledávání: '"L. S. Marochnik"'
Autor:
L. S. Marochnik, D. A. Usikov
Publikováno v:
Universe, Vol 8, Iss 9, p 464 (2022)
The dark energy from virtual gravitons is consistent with observational data on supernovas with the same accuracy as the ΛCDM model. The fact that virtual gravitons are capable of producing a de Sitter accelerated expansion of the FLRW universe was
Externí odkaz:
https://doaj.org/article/5e2cc28f0f3d408ca4970f60e89f1885
Autor:
L. S. Marochnik, A. A. Suchkov
Publikováno v:
The Magellanic Clouds ISBN: 9780792311119
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::373ce58329aa4f6aa1b004f031ea55d1
https://doi.org/10.1007/978-94-011-3432-3_119
https://doi.org/10.1007/978-94-011-3432-3_119
Publikováno v:
Galactic and Intergalactic Magnetic Fields ISBN: 9780792307051
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fa36bb062880c32252da478c6f7ee2db
https://doi.org/10.1007/978-94-009-0569-6_48
https://doi.org/10.1007/978-94-009-0569-6_48
Autor:
L. S. Marochnik
Publikováno v:
Astrophysics. 19:278-283
Autor:
L. S. Marochnik
Publikováno v:
The Moon and the Planets. 26:353-370
It is shown that when the solar wind interacts with comets, its magnetic field may penetrate through the discontinuity surface into the cometary ionosphere. In case of Venus-like planets the effect of regular motion of magnetic field lines through, t
Publikováno v:
Astrophysics. 18:97-106
The dynamic role of primordial black holes in the early Universe is examined in terms of their formation and properties of the mass distribution. Particular attention is given to the early density perturbations caused by the presence of black holes.
Autor:
L. S. Marochnik
Publikováno v:
Astrophysics and Space Science. 69:31-43
Autor:
A. A. Suchkov, L. S. Marochnik
Publikováno v:
Astrophysics and Space Science. 4:317-326
The spiral waves in a model galaxy consisting of differentially rotating and non-rotating subsystems are considered on the basis of participating phenomena. The subsystems involved represent the Populations I and II of normal spirals, respectively. T
Autor:
L. S. Marochnik
Publikováno v:
Astrophysics. 5:242-246