NUMERICAL-SIMULATION OF VISCOUS-FLOW BY SMOOTHED PARTICLE HYDRODYNAMICS

被引:333
作者
TAKEDA, H
MIYAMA, SM
SEKIYA, M
机构
[1] NATL ASTRON OBSERV,MITAKA,TOKYO 181,JAPAN
[2] KYUSHU UNIV,DEPT EARTH & PLANETARY SCI,FUKUOKA 812,JAPAN
来源
PROGRESS OF THEORETICAL PHYSICS | 1994年 / 92卷 / 05期
关键词
D O I
10.1143/PTP.92.939
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Smoothed particle hydrodynamics (SPH) is an effective numerical method to solve various problems, especially in astrophysics, but its applications have been limited to inviscid flows since it is considered not to yield ready solutions to fluid equations with second-order derivatives. Here we present a new SPH method that can be used to solve the Navier-Stokes equations for constant viscosity. The method is applied to two-dimensional Poiseuille flow, three-dimensional Hagen Poiseuille flow and two-dimensional isothermal flows around a cylinder. In the former two cases, the temperature of fluid is assumed to be linearly dependent on a coordinate variable x along the flow direction. The numerical results agree well with analytic solutions, and we obtain nearly uniform density distributions and the expected parabolic and paraboloid velocity profiles. The density and velocity field in the latter case are compared with the results obtained using a finite difference method. Both methods give similar results for Reynolds number R(e)=6, 10, 20, 30 and 55, and the differences in the total drag coefficients are about 2 similar to 4%. Our numerical simulations indicate that SPH is also an effective numerical method for calculation of viscous flows.
引用
收藏
页码:939 / 960
页数:22
相关论文
共 39 条
[1]   THE ORIGIN OF THE MOON AND THE SINGLE-IMPACT HYPOTHESIS .2. [J].
BENZ, W ;
SLATTERY, WL ;
CAMERON, AGW .
ICARUS, 1987, 71 (01) :30-45
[2]   A METHOD OF CALCULATING RADIATIVE HEAT DIFFUSION IN PARTICLE SIMULATIONS [J].
BROOKSHAW, L .
PROCEEDINGS ASTRONOMICAL SOCIETY OF AUSTRALIA, 1985, 6 (02) :207-210
[3]   THE ORIGIN OF THE MOON AND THE SINGLE IMPACT HYPOTHESIS-IV [J].
CAMERON, AGW ;
BENZ, W .
ICARUS, 1991, 92 (02) :204-216
[4]   EXPERIMENTAL-DETERMINATION OF MAIN FEATURES OF VISCOUS-FLOW IN WAKE OF A CIRCULAR-CYLINDER IN UNIFORM TRANSLATION .1. STEADY FLOW [J].
COUTANCEAU, M ;
BOUARD, R .
JOURNAL OF FLUID MECHANICS, 1977, 79 (FEB22) :231-+
[5]   NUMERICAL SOLUTIONS FOR STEADY FLOW PAST A CIRCULAR CYLINDER AT REYNOLDS NUMBERS UP TO 100 [J].
DENNIS, SCR ;
CHANG, GZ .
JOURNAL OF FLUID MECHANICS, 1970, 42 :471-&
[6]   RADIATION-HYDRODYNAMIC CALCULATION OF SUB-EDDINGTON ACCRETION DISKS [J].
EGGUM, GE ;
CORONITI, FV ;
KATZ, JI .
ASTROPHYSICAL JOURNAL, 1987, 323 (02) :634-646
[7]   A NUMERICAL STUDY OF STEADY VISCOUS-FLOW PAST A CIRCULAR-CYLINDER [J].
FORNBERG, B .
JOURNAL OF FLUID MECHANICS, 1980, 98 (JUN) :819-855
[8]   SMOOTHED PARTICLE HYDRODYNAMICS - THEORY AND APPLICATION TO NON-SPHERICAL STARS [J].
GINGOLD, RA ;
MONAGHAN, JJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1977, 181 (02) :375-389
[9]  
INUTSUKA S, 1994, THESIS
[10]  
INUTSUKA S, 1994, UNPUB J COMPUT PHYS