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Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation. / Stoyanovskaya, O. P.; Akimkin, V. V.; Vorobyov, E. I. и др.

в: Journal of Physics: Conference Series, Том 1103, № 1, 012008, 15.10.2018.

Результаты исследований: Научные публикации в периодических изданияхстатья по материалам конференцииРецензирование

Harvard

Stoyanovskaya, OP, Akimkin, VV, Vorobyov, EI, Glushko, TA, Pavlyuchenkov, YN, Snytnikov, VN & Snytnikov, NV 2018, 'Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation', Journal of Physics: Conference Series, Том. 1103, № 1, 012008. https://doi.org/10.1088/1742-6596/1103/1/012008

APA

Stoyanovskaya, O. P., Akimkin, V. V., Vorobyov, E. I., Glushko, T. A., Pavlyuchenkov, Y. N., Snytnikov, V. N., & Snytnikov, N. V. (2018). Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation. Journal of Physics: Conference Series, 1103(1), [012008]. https://doi.org/10.1088/1742-6596/1103/1/012008

Vancouver

Stoyanovskaya OP, Akimkin VV, Vorobyov EI, Glushko TA, Pavlyuchenkov YN, Snytnikov VN и др. Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation. Journal of Physics: Conference Series. 2018 окт. 15;1103(1):012008. doi: 10.1088/1742-6596/1103/1/012008

Author

Stoyanovskaya, O. P. ; Akimkin, V. V. ; Vorobyov, E. I. и др. / Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation. в: Journal of Physics: Conference Series. 2018 ; Том 1103, № 1.

BibTeX

@article{f56128bf0a05460086c656f8d1f30cb3,
title = "Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation",
abstract = "Circumstellar discs, from which planetary systems are formed, consist of gas, dust and solids. Simulations of self-consistent dynamics of gas, dust and solids in circumstellar discs is a challenging problem. In the paper we present fast algorithms for computing the drag force (momentum transfer) between solid phase and gas. These algorithms (a) are universal and applicable to dust and solids with any sizes smaller than the mean free path of gas molecules, (b) can be used to calculate the momentum transfer between dust and gas instead of one-way effect, as it is done in many models, (c) can perform simulations, without a loss in accuracy, with the time step determined by gas-dynamic parameters rather than by drag force, and (d) are compatible with the widely used parallel algorithms for solving 3D equations of gas dynamics, hydrodynamic equations for dust, and the collisionless Boltzmann equation for large bodies. Preliminary results of supercomputer simulation of the gas-dust disc dynamics within the developed approach are reported.",
author = "Stoyanovskaya, {O. P.} and Akimkin, {V. V.} and Vorobyov, {E. I.} and Glushko, {T. A.} and Pavlyuchenkov, {Ya N.} and Snytnikov, {V. N.} and Snytnikov, {N. V.}",
note = "Publisher Copyright: {\textcopyright} 2018 Institute of Physics Publishing. All rights reserved.; Workshop on Numerical Modeling in MHD and Plasma Physics: Methods, Tools, and Outcomes. Honor of academician Anatoly Alekseev's 90th Birthday ; Conference date: 11-10-2018 Through 12-10-2018",
year = "2018",
month = oct,
day = "15",
doi = "10.1088/1742-6596/1103/1/012008",
language = "English",
volume = "1103",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation

AU - Stoyanovskaya, O. P.

AU - Akimkin, V. V.

AU - Vorobyov, E. I.

AU - Glushko, T. A.

AU - Pavlyuchenkov, Ya N.

AU - Snytnikov, V. N.

AU - Snytnikov, N. V.

N1 - Publisher Copyright: © 2018 Institute of Physics Publishing. All rights reserved.

PY - 2018/10/15

Y1 - 2018/10/15

N2 - Circumstellar discs, from which planetary systems are formed, consist of gas, dust and solids. Simulations of self-consistent dynamics of gas, dust and solids in circumstellar discs is a challenging problem. In the paper we present fast algorithms for computing the drag force (momentum transfer) between solid phase and gas. These algorithms (a) are universal and applicable to dust and solids with any sizes smaller than the mean free path of gas molecules, (b) can be used to calculate the momentum transfer between dust and gas instead of one-way effect, as it is done in many models, (c) can perform simulations, without a loss in accuracy, with the time step determined by gas-dynamic parameters rather than by drag force, and (d) are compatible with the widely used parallel algorithms for solving 3D equations of gas dynamics, hydrodynamic equations for dust, and the collisionless Boltzmann equation for large bodies. Preliminary results of supercomputer simulation of the gas-dust disc dynamics within the developed approach are reported.

AB - Circumstellar discs, from which planetary systems are formed, consist of gas, dust and solids. Simulations of self-consistent dynamics of gas, dust and solids in circumstellar discs is a challenging problem. In the paper we present fast algorithms for computing the drag force (momentum transfer) between solid phase and gas. These algorithms (a) are universal and applicable to dust and solids with any sizes smaller than the mean free path of gas molecules, (b) can be used to calculate the momentum transfer between dust and gas instead of one-way effect, as it is done in many models, (c) can perform simulations, without a loss in accuracy, with the time step determined by gas-dynamic parameters rather than by drag force, and (d) are compatible with the widely used parallel algorithms for solving 3D equations of gas dynamics, hydrodynamic equations for dust, and the collisionless Boltzmann equation for large bodies. Preliminary results of supercomputer simulation of the gas-dust disc dynamics within the developed approach are reported.

UR - http://www.scopus.com/inward/record.url?scp=85056414942&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/1103/1/012008

DO - 10.1088/1742-6596/1103/1/012008

M3 - Conference article

AN - SCOPUS:85056414942

VL - 1103

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012008

T2 - Workshop on Numerical Modeling in MHD and Plasma Physics: Methods, Tools, and Outcomes. Honor of academician Anatoly Alekseev's 90th Birthday

Y2 - 11 October 2018 through 12 October 2018

ER -

ID: 17408862