Zobrazeno 1 - 10
of 13
pro vyhledávání: '"S. V. Smerechynskyi"'
Autor:
S. V. Smerechynskyi, D. V. Dzikovskyi
Publikováno v:
Odessa Astronomical Publications, Vol 30, Iss 0, Pp 128-134 (2017)
The macroscopic characteristics of the degenerate dwarves were calculated based on the equation of state of a spin-polarized electron gas at T = 0K as well as at finite temperatures. It was shown that the spin-polarization cause an increase of the r
Externí odkaz:
https://doaj.org/article/759204d523d046019518eb30687cdd93
We study the density distribution of the minimally-coupled scalar field dark energy inside a neutron star. The dark energy is considered in the hydrodynamical representation as a perfect fluid with three parameters (background density, equation of st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47b93f306efc41d7079a5e2774ac5751
http://arxiv.org/abs/2009.14612
http://arxiv.org/abs/2009.14612
Publikováno v:
Physical Review D. 101
We investigate the radial density distribution of the dynamical dark energy inside the white dwarfs (WDs) and its possible impact on their intrinsic structure. The minimally-coupled dark energy with barotropic equation of state which has three free p
Publikováno v:
Proceedings of the International Astronomical Union. 14:139-142
We show that the structure of magnetized accretion gas flows between the components of the Beta Lyrae system can cause a scattering gas shell that masks completely these components in soft X-ray region. Also we have calculated the inner structure of
Publikováno v:
Advances in Astronomy and Space Physics. 8:9-15
Using the equation of state of electron-nuclear model at high densities and the mechanical equilibrium equation we have investigated the influence of interparticle interactions and axial rotation on the macroscopic characteristics of massive white dw
Publikováno v:
Mathematical Modeling and Computing. 4:107-115
Publikováno v:
Journal of Physical Studies. 22
Autor:
M. V. Vavrukh, S. V. Smerechynskyi
Publikováno v:
Astronomy Reports. 56:363-378
We suggest a generalization of the standard Chandrasekhar model for degenerate dwarfs. We apply an equation of state for a degenerate ideal electron gas in the form of a Sommerfeld expansion in the parameter k B T(r)/m 0 c 2. The radial temperature d
Publikováno v:
Astronomy Reports. 55:505-524
Based on the radii and masses of degenerate dwarfs derived from HIPPARCOS and other observations, we estimate the microscopic parameters of a Chandrasekhar model (the relativistic parameter at the stellar center x0, and the chemical-composition param
Publikováno v:
Ukrainian Journal of Physics. 63:777
Using the equation of state of the electron-nuclear model at high densities and the mechanical equilibrium equation, we have investigated the influence of interparticle interactions and the axial rotation on the macroscopic characteristics (mass, sur