A Hybrid Cosmological Hydrodynamic/N-body Code Based on a Weighted Essentially Non-Oscillatory Scheme

نویسندگان

  • Long-Long Feng
  • Chi-Wang Shu
  • Mengping Zhang
چکیده

We present a newly developed cosmological hydrodynamics code based on weighted essentially non-oscillatory (WENO) schemes for hyperbolic conservation laws and related Hamilton-Jacobi equations. WENO is a higher order accurate finite difference scheme designed for problems with piecewise smooth solutions containing discontinuities, and has been successful in application for problems involving both shocks and complicated smooth solution structures. We couple hydrodynamics based on the WENO scheme with standard Poisson solver particle-mesh (PM) algorithm for evolving the self-gravitating system. The third order total variation diminishing (TVD) Runge-Kutta scheme has been used for time-integration of the system. To test the performance of the code, we subject it to a number of typical tests including the Sod shock tube in multidimension, the Sedov blast wave and formation of the Zeldovich pancake. These tests validate the WENO hydrodynamics with fast convergence rate and high accuracy. Also, we evolve a low density flat cosmological model (ΛCDM) to explore validity of the code in practical simulations. Subject headings: cosmology: theory large-scale structure of the universe Purple Mountain Observatory, Nanjing, 210008, P.R. China. E-mail: [email protected] Center for Astrophysics, University of Science and Technology of China, Hefei, Anhui 230026, P.R. China National Astronomical Observatories, Chinese Academy of Science, Chao-Yang District, Beijing 100012, P.R. China Division of Applied Mathematics, Brown University, Providence, RI 02912, U.S.A. E-mail: [email protected] Department of Mathematics, University of Science and Technology of China, Hefei, Anhui 230026, P.R. China. E-mail: [email protected]

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

A Hybrid Cosmological Hydrodynamic/n-body Code Based on the Weighted Essentially Non-oscillatory Scheme

We describe a newly developed cosmological hydrodynamics code based on the weighted essentially non-oscillatory (WENO) schemes for hyperbolic conservation laws. High order finite difference WENO schemes are designed for problems with piecewise smooth solutions containing discontinuities, and have been successful in applications for problems involving both shocks and complicated smooth solution ...

متن کامل

Relativistic Hydrodynamic Flows Using Spatial and Temporal Adaptive Structured Mesh Refinement

Astrophysical relativistic flow problems require high resolution three-dimensional numerical simulations. In this paper, we describe a new parallel three-dimensional code for simulations of special relativistic hydrodynamics (SRHD) using both spatially and temporally structured adaptive mesh refinement (AMR). We used the method of lines to discretize the SRHD equations spatially and a total var...

متن کامل

A new multidimensional AMR Hydro+Gravity Cosmological code

A new cosmological multidimensional hydrodynamic and N-body code based on an Adaptive Mesh Refinement scheme is described and tested. The hydro part is based on modern high-resolution shock-capturing techniques, whereas N-body approach is based on the Particle Mesh method. The code has been specifically designed for cosmological applications. Tests including shocks, strong gradients, and gravit...

متن کامل

Hybrid weighted essentially non-oscillatory schemes with different indicators

A key idea in finite difference weighted essentially non-oscillatory (WENO) schemes is a combination of lower order fluxes to obtain a higher order approximation. The choice of the weight to each candidate stencil, which is a nonlinear function of the grid values, is crucial to the success of WENO. For the system case, WENO schemes are based on local characteristic decompositions and flux split...

متن کامل

Relativistic Flows Using Spatial and Temporal Adaptive Structured Mesh Refinement. I. Hydrodynamics

Astrophysical relativistic flow problems require high resolution three-dimensional numerical simulations. In this paper, we describe a new parallel three-dimensional code for simulations of special relativistic hydrodynamics (SRHD) using both spatially and temporally structured adaptive mesh refinement (AMR). We used method of lines to discrete SRHD equations spatially and used a total variatio...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008