Hydrodynamical Processes in High Energy Astrophysics

这个项目将由世界领先的理论天体物理学家之一实施，将使用现代基于网格的氢码，改编自成功的空气动力学代码，以研究大规模的宇宙结构，以及物质落向致密物体。真正的流体动力学计算方法已经开发出来，它可以处理冲击和辐射过程，并允许直接计算x射线发射、宇宙背景辐射波动和以前无法用数值方法获得的其他现象。

This program, to be carried out by one of the world's leading theoretical astrophysicists, will use modern grid-based hydrocodes, adapted from successful aerodynamic codes to study large-scale cosmic structure, and the infall of matter onto compact objects. True hydrodynamic computational methods have been developed, which can treat shocks and radiative processes, and which will permit the direct calculation of X-ray emission, fluctuations in the cosmic background radiation, and other phenomena not previously accessible from numerical approaches.