A novel approach for accurate radiative transfer in cosmological hydrodynamic simulations

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 4, 2011, Pages 3731-3749

  Petkova, Margarita ^a   Springel, Volker ^a,b,c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b HEIDELBERG INSTITUTE FOR THEORETICAL STUDIES   (Germany)

^c UNIVERSITY OF HEIDELBERG   (Germany)

Author keywords

Intergalactic medium; Methods: numerical; Radiative transfer

Indexed keywords

ADVECTION; BOLTZMANN EQUATION; COSMIC RAYS; HYDRODYNAMICS; LIGHT; NUMERICAL METHODS; PHOTONS; RADIATIVE TRANSFER;

ANGULAR RESOLUTION; DENSITY FIELDS; HYDRODYNAMIC SIMULATION; INTERGALACTIC MEDIUM; METHOD: NUMERICAL; NUMERICAL IMPLEMENTATION; POINT-SOURCES; RADIATIVE FLUXES; STRUCTURED MESH; TRANSFER EQUATION;

COSMOLOGY;

EID: 80051820647     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18986.x     Document Type: Article

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