Smooth particle hydrodynamics: importance of correction terms in adaptive resolution algorithms

被引:17
作者
Alimi, JM
Serna, A [1 ]
Pastor, C
Bernabeu, G
机构
[1] Observ Paris, CNRS, LUTH 4862, Lab Univers & Theories, F-92195 Meudon, Spain
[2] Univ Miguel Hernandez, Dept Fis & AC, E-03202 Elche, Spain
[3] Univ Alicante, Dept Fis & Ingn Sistemas, E-03080 Alicante, Spain
关键词
methods; numerical; hydrodynamics; galaxies; formation;
D O I
10.1016/S0021-9991(03)00351-6
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
We describe TREEASPH, a new code to evolve self-gravitating fluids, both with and without a collisionless component. In TREEASPH, gravitational forces are computed from a hierarchical tree algorithm (TREEcode), while hydrodynamic properties are computed by using a SPH method that includes the delh correction terms appearing when the spatial resolution h(t, r) is not a constant. Another important feature, which considerably increases the code efficiency on sequential and vectorial computers, is that time-stepping is performed from a PEC scheme (Predict-Evaluate-Correct) modified to allow for individual timesteps. Some authors have previously noted that the delh correction terms are needed to avoid the introduction on simulations of a non-physical entropy. By using TREEASPH we show here that, in cosmological simulations, this non-physical entropy has a negative sign. As a consequence, when the delh terms are neglected, the density peaks associated to shock fronts are overestimated. This in turn results in an overestimated efficiency of star-formation processes. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码:157 / 174
页数:18
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