Supercomputer Simulation of a Gravitating Gaseous Circumstellar Disk Using SPH Full article
| Journal |
Bulletin of the Novosibirsk Computing Center. Series: Numerical Analysis
ISSN: 1680-7006 |
|---|---|
| Output data | Year: 2016, Volume: 18, Pages: 67-75 Pages count : 9 |
| Authors |
|
| Affiliations |
Funding (2)
| 1 | The Ministry of Education and Science of the Russian Federation | МК-5915.2016.1 |
| 2 | Russian Foundation for Basic Research | 16-07-00916 |
Abstract:
New parallel algorithm is developed for simulating the dynamics of a thin circumstellar disk. It is based on the combination of a gridless method of smoothed particle hydrodynamics (SPH) and the grid-based convolution method for calculating a gravitational potential. To develop the algorithm, we made software pro ling of numerical experiments aimed at simulating gravitational fragmentation and subsequent inward migration of dense clumps onto the star.
Cite:
Stoyanovskaya O.P.
, Snytnikov N.V.
Supercomputer Simulation of a Gravitating Gaseous Circumstellar Disk Using SPH
Bulletin of the Novosibirsk Computing Center. Series: Numerical Analysis. 2016. V.18. P.67-75. РИНЦ
Supercomputer Simulation of a Gravitating Gaseous Circumstellar Disk Using SPH
Bulletin of the Novosibirsk Computing Center. Series: Numerical Analysis. 2016. V.18. P.67-75. РИНЦ
Identifiers:
| Elibrary: | 29454479 |
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