A WENO algorithm for the radiative transfer and ionized sphere at reionization

[1]  Chi-Wang Shu,et al.  2D semiconductor device simulations by WENO-Boltzmann schemes: Efficiency, boundary conditions and comparison to Monte Carlo methods , 2006, J. Comput. Phys..

[2]  Chi-Wang Shu,et al.  Anti-diffusive flux corrections for high order finite difference WENO schemes , 2005 .

[3]  A. Loeb,et al.  A large neutral fraction of cosmic hydrogen a billion years after the Big Bang , 2004, Nature.

[4]  A. Maselli,et al.  CRASH: A radiative transfer scheme , 2003, astro-ph/0307117.

[5]  Irene M. Gamba,et al.  A WENO-solver for the transients of Boltzmann-Poisson system for semiconductor devices: performance and comparisons with Monte Carlo methods , 2003 .

[6]  Douglas Scott,et al.  Cosmological Hydrogen Reionization with Three-dimensional Radiative Transfer , 2001, astro-ph/0109111.

[7]  B. Ciardi,et al.  Cosmological reionization around the first stars: Monte Carlo radiative transfer , 2000, astro-ph/0005181.

[8]  M. Norman,et al.  Photon-conserving Radiative Transfer around Point Sources in Multidimensional Numerical Cosmology , 1998, astro-ph/9812151.

[9]  A. Leonard,et al.  P3M‐SPH simulations of the Lyα forest , 1998, astro-ph/9805119.

[10]  Chi-Wang Shu,et al.  Efficient Implementation of Weighted ENO Schemes , 1995 .

[11]  D. Osterbrock,et al.  Astrophysics of Gaseous Nebulae and Active Galactic Nuclei , 1989 .

[12]  Jeremy Bernstein,et al.  Kinetic theory in the expanding universe , 1988 .

[13]  Lyman Spitzer,et al.  Physical processes in the interstellar medium , 1998 .