Zobrazeno 1 - 10
of 20
pro vyhledávání: '"A. N. Kobyakov"'
Publikováno v:
Herald of the Russian Academy of Sciences. 92:313-322
Abstract The tasks of establishing an ecological network are presented, outlining some outcome of the long-term study of the Great Eurasian Natural Tract (Backbone), which is a continuous series of natural ecological systems from the Pacific Ocean to
Autor:
D. N. Kobyakov
In this paper, an effective field theory for proton superconductor (SC) interacting with neutron superfluid (SF), both with scalar order parameters, is developed and applied to the surface energy (SE) of a magnetized SC body in neutron stars (NS). Es
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::62640732e8786d71438c868e1d7297db
http://arxiv.org/abs/2208.02738
http://arxiv.org/abs/2208.02738
Autor:
Konstantin N. Kobyakov
Publikováno v:
Пернатые хищники и их охрана, Vol 0, Iss 1, Pp 238-239 (2018)
Одной из важных угроз для хищных птиц и мест их обитания является лесопользование, и, прежде всего, деятельность по заготовке древесины.
Externí odkaz:
https://doaj.org/article/910b24978e4f4f4aa2adb6847754b84a
Publikováno v:
Science and Education a New Dimension. :82-85
Publikováno v:
Pethick, C J, Zhang, Z-W & Kobyakov, D N 2020, ' Elastic properties of phases with nonspherical nuclei in dense matter ', Physical Review C, vol. 101, no. 5, 055802 . https://doi.org/10.1103/PhysRevC.101.055802
We consider the elastic constants of phases with nonspherical nuclei, so-called pasta phases, predicted to occur in the inner crust of a neutron star. First, we treat perfectly ordered phases and give numerical estimates for lasagna and spaghetti whe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fedcb076ec925e05cb1234faa2325d29
Autor:
D. N. Kobyakov, Christopher J. Pethick
The pasta phases predicted to occur near the inner boundary of the crust of a neutron star resemble liquid crystals, a smectic A in the case of sheet-like nuclei (lasagna) and the columnar phase in the case of rod-like nuclei (spaghetti). An importan
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e4392ea4e581d5907ed423514b2892d6
http://arxiv.org/abs/1803.06254
http://arxiv.org/abs/1803.06254
Autor:
D. N. Kobyakov
A mixture of superconducting and superfluid nuclear liquids of protons coupled to the ultrarelativistic electron gas, and neutrons is considered. In the magnetohydrodynamic (MHD) approximation, the energy-momentum (stress) tensor is derived, and the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2fe873ebba6c2f1e27bb9bcdaafd715d
Autor:
Christopher J. Pethick, D. N. Kobyakov
Publikováno v:
Physical Review C. 94
Autor:
D. N. Kobyakov, Christopher J. Pethick
The interaction between nuclei in the inner crust of neutron stars consists of two contributions, the so-called "direct" interaction and an "induced" one due to density changes in the neutron fluid. For large nuclear separations $r$ the contributions
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5435c8fde16ff6bcd4d19ef1f98c0e23
Autor:
D. N. Kobyakov, Christopher J. Pethick
We consider the hydrodynamics of the outer core of a neutron star under conditions when both neutrons and protons are superfluid. Starting from the equation of motion for the phases of the wave functions of the condensates of neutron pairs and proton
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f45b8a6de334f1e7f4616998d99a852d
http://arxiv.org/abs/1504.00570
http://arxiv.org/abs/1504.00570