Standard

Shock waves in carbon dioxide : Simulations using different kinetic-theory models. / Alekseev, I. V.; Kosareva, A. A.; Kustova, E. V.; Nagnibeda, E. A.

31st International Symposium on Rarefied Gas Dynamics, RGD 2018. American Institute of Physics, 2019. 060005 (AIP Conference Proceedings; Том 2132, № 1).

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференцийстатья в сборнике материалов конференцииРецензирование

Harvard

Alekseev, IV, Kosareva, AA, Kustova, EV & Nagnibeda, EA 2019, Shock waves in carbon dioxide: Simulations using different kinetic-theory models. в 31st International Symposium on Rarefied Gas Dynamics, RGD 2018., 060005, AIP Conference Proceedings, № 1, Том. 2132, American Institute of Physics, 31st International Symposium on Rarefied Gas Dynamics, RGD 2018, Glasgow, Великобритания, 23/07/18. https://doi.org/10.1063/1.5119545

APA

Alekseev, I. V., Kosareva, A. A., Kustova, E. V., & Nagnibeda, E. A. (2019). Shock waves in carbon dioxide: Simulations using different kinetic-theory models. в 31st International Symposium on Rarefied Gas Dynamics, RGD 2018 [060005] (AIP Conference Proceedings; Том 2132, № 1). American Institute of Physics. https://doi.org/10.1063/1.5119545

Vancouver

Alekseev IV, Kosareva AA, Kustova EV, Nagnibeda EA. Shock waves in carbon dioxide: Simulations using different kinetic-theory models. в 31st International Symposium on Rarefied Gas Dynamics, RGD 2018. American Institute of Physics. 2019. 060005. (AIP Conference Proceedings; 1). https://doi.org/10.1063/1.5119545

Author

Alekseev, I. V. ; Kosareva, A. A. ; Kustova, E. V. ; Nagnibeda, E. A. / Shock waves in carbon dioxide : Simulations using different kinetic-theory models. 31st International Symposium on Rarefied Gas Dynamics, RGD 2018. American Institute of Physics, 2019. (AIP Conference Proceedings; 1).

BibTeX

@inproceedings{99c51edbbdb140e5b590359b69333968,
title = "Shock waves in carbon dioxide: Simulations using different kinetic-theory models",
abstract = "Shock wave structure in carbon dioxide is studied on the basis of several continuum models and compared to the solution obtained using the kinetic approach. The problem is solved in the frame of one- A nd two-temperature Euler equations as well as Navier-Stokes equations accounting for the bulk viscosity. The Rankine-Hugoniot relations with constant specific heat ratio fail to predict accurately the final equilibrium state in polyatomic gases. A good qualitative agreement of the solutions obtained using the continuum and kinetic approaches is shown. Taking into account the bulk viscosity leads to a considerable increase in the shock wave width; its variation in a flow modifies the profiles of gas-dynamic parameters. In the multi-temperature approach, solving the Euler equations coupled to the relaxation equation for the vibrational energy provides the results similar to those obtained within the kinetic approach taking into account the effect of bulk viscosity.",
author = "Alekseev, {I. V.} and Kosareva, {A. A.} and Kustova, {E. V.} and Nagnibeda, {E. A.}",
year = "2019",
month = aug,
day = "5",
doi = "10.1063/1.5119545",
language = "English",
series = "AIP Conference Proceedings",
publisher = "American Institute of Physics",
number = "1",
booktitle = "31st International Symposium on Rarefied Gas Dynamics, RGD 2018",
address = "United States",
note = "31st International Symposium on Rarefied Gas Dynamics, RGD 2018 ; Conference date: 23-07-2018 Through 27-07-2018",

}

RIS

TY - GEN

T1 - Shock waves in carbon dioxide

T2 - 31st International Symposium on Rarefied Gas Dynamics, RGD 2018

AU - Alekseev, I. V.

AU - Kosareva, A. A.

AU - Kustova, E. V.

AU - Nagnibeda, E. A.

PY - 2019/8/5

Y1 - 2019/8/5

N2 - Shock wave structure in carbon dioxide is studied on the basis of several continuum models and compared to the solution obtained using the kinetic approach. The problem is solved in the frame of one- A nd two-temperature Euler equations as well as Navier-Stokes equations accounting for the bulk viscosity. The Rankine-Hugoniot relations with constant specific heat ratio fail to predict accurately the final equilibrium state in polyatomic gases. A good qualitative agreement of the solutions obtained using the continuum and kinetic approaches is shown. Taking into account the bulk viscosity leads to a considerable increase in the shock wave width; its variation in a flow modifies the profiles of gas-dynamic parameters. In the multi-temperature approach, solving the Euler equations coupled to the relaxation equation for the vibrational energy provides the results similar to those obtained within the kinetic approach taking into account the effect of bulk viscosity.

AB - Shock wave structure in carbon dioxide is studied on the basis of several continuum models and compared to the solution obtained using the kinetic approach. The problem is solved in the frame of one- A nd two-temperature Euler equations as well as Navier-Stokes equations accounting for the bulk viscosity. The Rankine-Hugoniot relations with constant specific heat ratio fail to predict accurately the final equilibrium state in polyatomic gases. A good qualitative agreement of the solutions obtained using the continuum and kinetic approaches is shown. Taking into account the bulk viscosity leads to a considerable increase in the shock wave width; its variation in a flow modifies the profiles of gas-dynamic parameters. In the multi-temperature approach, solving the Euler equations coupled to the relaxation equation for the vibrational energy provides the results similar to those obtained within the kinetic approach taking into account the effect of bulk viscosity.

UR - http://www.scopus.com/inward/record.url?scp=85070669177&partnerID=8YFLogxK

UR - http://www.mendeley.com/research/shock-waves-carbon-dioxide-simulations-using-different-kinetictheory-models

U2 - 10.1063/1.5119545

DO - 10.1063/1.5119545

M3 - Conference contribution

AN - SCOPUS:85070669177

T3 - AIP Conference Proceedings

BT - 31st International Symposium on Rarefied Gas Dynamics, RGD 2018

PB - American Institute of Physics

Y2 - 23 July 2018 through 27 July 2018

ER -

ID: 50837859