Zobrazeno 1 - 10
of 129
pro vyhledávání: '"I. Chugunov"'
Publikováno v:
Фінансово-кредитна діяльність: проблеми теорії та практики, Vol 2, Iss 37 (2021)
Анотація. Розкрито роль системи державних фінансів у забезпеченні макроекономічної стабільності, регулюванні економічних процесів та
Externí odkaz:
https://doaj.org/article/4f0ef197bd5743d89cab8b2036c52bcf
Autor:
I. Chugunov, V. Makogon
Publikováno v:
Фінансово-кредитна діяльність: проблеми теорії та практики, Vol 4, Iss 35 (2021)
Анотація. Розкрито роль пенсійної системи в забезпечені суспільного розвитку. Визначено напрями забезпечення стійкості та зміцнення ф
Externí odkaz:
https://doaj.org/article/781621c79dab49f8b79c805822faeffc
Autor:
Alena D. Khokhriakova, Andrey I. Chugunov, Sergei B. Popov, Mikhail E. Gusakov, Elena M. Kantor
Publikováno v:
Universe, Vol 8, Iss 7, p 354 (2022)
Neutron stars can appear as sources of different nature. In this paper we address the observability of a hypothetical class of neutron stars—HOt and Fast Non-Accreting Rotators, HOFNARs. These objects are heated due to the r-mode instability. With
Externí odkaz:
https://doaj.org/article/709b4ca9346e4308bbfb115bf07d4b7a
Publikováno v:
Universe; Volume 9; Issue 5; Pages: 220
Neutron stars are the densest objects in the Universe. They have a microscopically homogeneous core and heterogeneous crust. In particular, there may be a specific layer inside neutron stars, the mantle, which consists of substantially non-spherical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::364f6738711e5c0348f016866fad221b
Thermal emission of neutron stars in soft X-ray transients (SXTs) in a quiescent state is believed to be powered by the heat deposited in the stellar crust due to nuclear reactions during accretion (deep crustal heating paradigm). Confronting observa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a8633ffc04efb053d21b7ebd2e3918ea
Autor:
D A Baiko, A I Chugunov
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 510:2628-2643
Using path-integral Monte Carlo (PIMC) simulations, we have calculated energy of a crystal composed of atomic nuclei and uniform incompressible electron background in the temperature and density range, covering fully ionized layers of compact stellar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8825546a64eb1506102c797ed98abcde
https://doi.org/10.1093/mnras/stab3613
https://doi.org/10.1093/mnras/stab3613
Publikováno v:
Universe; Volume 8; Issue 11; Pages: 582
Nuclear pasta phases in the neutron stars mantle can affect the mechanical and transport properties of superdense matter, thus playing an important role in the dynamics and evolution of neutron stars. In this paper, we compare results obtained by the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4bc6870beb4c314d262729588362b34
Publikováno v:
Particles; Volume 5; Issue 3; Pages: 225-234
Neutron stars are the densest objects in the Universe. In this paper we consider so-called inner crust - the layer, where neutron-excess nuclei are immersed into degenerate gas of electrons and sea of quasi-free neutrons. It was generally believed th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c48bca404790e1f9494acc909514efec
http://arxiv.org/abs/2209.05851
http://arxiv.org/abs/2209.05851
Autor:
I., Chugunov1 chugunov055@gmail.com, V., Makogon2 makvknteu@gmail.com, Yu., Markuts3 j.markuts@gmail.com
Publikováno v:
Financial & Credit Activity: Problems of Theory & Practice. 2021, Vol. 2 Issue 37, p325-331. 7p.
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