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Volumn 98, Issue 4, 2000, Pages 239-248

Monte Carlo simulation of a hard-sphere gas in the planar Fourier flow with a gravity field

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; DENSITY (SPECIFIC GRAVITY); FLOW OF FLUIDS; GRAVITATION; HEAT FLUX; MAXWELL EQUATIONS; MONTE CARLO METHODS; PRESSURE; TEMPERATURE;

EID: 0034688626     PISSN: 00268976     EISSN: None     Source Type: Journal    
DOI: 10.1080/002689700162667     Document Type: Article
Times cited : (6)

References (28)
  • 11
    • 0002550838 scopus 로고
    • reprinted in Brush, S. G., 1966, Kinetic Theory, Vol. 2, Irreversible Processes (Oxford: Pergamon). note
    • (n-5)/(n-1) of the relative velocity V of the two colliding molecules. In the case of inverse fifth-power forces (n = 5), the relative velocity drops out and the integration can be carried out without knowing the non-equilibrium distribution function. These fictitious particles interacting with a repulsive force inversely proportional to the fifth power of their distance are called Maxwell molecules.
    • (1867) Phil. Trans. Roy. Soc. (London) , vol.157 , pp. 49
    • Maxwell, J.C.1
  • 19
    • 0011076090 scopus 로고    scopus 로고
    • edited by R. Brun, R. Campargue, R. Gatignol and J.-C. Lengrand (Toulouse: Ćpadués)
    • Tij, M., Garzó, V., and Santos A., 1999, Rarefied Gas Dynamics Vol. 1, edited by R. Brun, R. Campargue, R. Gatignol and J.-C. Lengrand (Toulouse: Ćpadués), pp. 239-246.
    • (1999) Rarefied Gas Dynamics , vol.1 , pp. 239-246
    • Tij, M.1    Garzó, V.2    Santos, A.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.