Mathematical modeling of vortex structures in fast-rotating astrophysical objects

mathematical modeling, conservative difference schemes, numerical methods, parallel algorithms, hydrodynamics, astrophysics, supernovae, gravity, vortex structures

Acknowledgment

The calculations were performed on the computational resources of the Interdepartmental Supercomputer Center of the Russian Academy of Sciences (MSC RAS).

Received

27.10.2018

Publication date

28.10.2018

Number of characters

379

Cite Download pdf To download PDF you should sign in

GOST	Babakov A., Aksenov A., Chechetkin V. Mathematical modeling of vortex structures in fast-rotating astrophysical objects // Zhurnal vychislitelnoi matematiki i matematicheskoi fiziki – 2018. – V. 58. – Issue 8 C. 182-188 [Electronic resource]. URL: http://ras.jes.su/zvmmf/s207987840001059-3-3-en (circulation date: 13.10.2024). DOI: 10.31857/S004446690002004-5
MLA	Babakov, A., Aksenov, A., Chechetkin, V. "Mathematical modeling of vortex structures in fast-rotating astrophysical objects." Zhurnal vychislitelnoi matematiki i matematicheskoi fiziki 58.8 (2018):182-188. DOI: 10.31857/S004446690002004-5
APA	Babakov A., Aksenov A., Chechetkin V. (2018). Mathematical modeling of vortex structures in fast-rotating astrophysical objects. Zhurnal vychislitelnoi matematiki i matematicheskoi fiziki 58(8), pp.182-188 DOI: 10.31857/S004446690002004-5

Размещенный ниже текст является ознакомительной версией и может не соответствовать печатной

Readers community rating: votes 0

1. S.M. Couch and C.D. Ott The role of turbulence in neutrino-driven core-collapse supernova explosions // Astroph. Journal. 2015. V. 799. P. 5.

2. V.M. Chechetkin, S.D. Ustyugov, A.A. Gorbunov, V.I. Polezhaev // Pis'ma astron. zh. 1997. T. 23. S. 34.

3. V.M. Suslin, S.D. Ustyugov, V.M. Chechetkin // Astron. zh. 2002. V. 78. P. 281

4. S. Chandrasekhar and N.R. Lebovitz. Non-Radial Oscillations and Convective Instability of Gaseous Masses // Astrophys. Journal. 1963. V. 138. P. 185.

5. O.M. Belotserkovskij, A.M. Oparin, V.M. Chechetkin. Turbulentnost'. Novye podkhody. M.: Nauka, 2002.

6. Shapiro S., T'yukolski S. Chernye dyry, belye karliki, nejtronnye zvezdy. M.: Mir, 1985.

7. O.M. Belotserkovskij, L.I. Severinov. Konservativnyj metod potokov i raschet obtekaniya tela konechnykh razmerov vyazkim teploprovodnym gazom // Zh. vychisl. matem. i matem. fiz. 1973. T. 13. № 2. S. 385–397.

8. O.M. Belotserkovskii, A.V. Babakov. The simulation of the coherent vortex structures in the turbulent flows. Advances in Mechanics, Poland, 1990. V. 13. № 3/4. P. 135–169.

9. A.V. Babakov. Chislennoe modelirovanie prostranstvenno-nestatsionarnykh struj szhimaemogo gaza na mnogoprotsessornom vychislitel'nom komplekse // Zh. vychisl.matem. i matem.fiz. 2011. T. 51. № 2. S. 251–260.

10. A.V. Babakov, M.V. Popov, V.M. Chechetkin. Modelirovanie ehvolyutsii massivnoj zvezdy na osnove gazodinamicheskoj modeli. //Zh. Matem. modelirovanie. 2017. T. 29. № 11. S. 131–139.

11. A.V. Babakov. Programmnyj kompleks “flux” dlya modelirovaniya fundamental'nykh i prikladnykh zadach aehrogidrodinamiki. //Zh. vychisl. matem. i matem. fiz. 2016. T. 56. № 6. S. 1174–1184.

12. A.G. Aksenov, S.I. Blinnikov. A Newton iteration method for obtaining equilibria of rapidly rotating stars // Astronomy and Astrophysics, 1994. № .290. R. 674–681.

13. A.G. Aksenov. Chislennoe reshenie uravneniya Puassona dlya trezmernogomodelirovaniya ehvolyutsii zvezd // Pis'ma v astron. zh. 1999. T. 25. S. 226–232.