Cosmological radiative transfer comparison project - II. the radiation-hydrodynamic tests

Monthly Notices of the Royal Astronomical Society

Volumn 400, Issue 3, 2009, Pages 1283-1316

  Iliev, Ilian T ^a,b,c   Whalen, Daniel ^d   Mellema, Garrelt ^e   Ahn, Kyungjin ^f,g   Baek, Sunghye ^h   Gnedin, Nickolay Y ⁱ   Kravtsov, Andrey V ^j   Norman, Michael ^k   Raicevic, Milan ^l   Reynolds, Daniel R ^m   Sato, Daisuke ⁿ   Shapiro, Paul R ^g   Semelin, Benoit ^h   Smidt, Joseph ^o   Susa, Hajime ^p   Theuns, Tom ^l,q   Umemura, Masayuki ⁿ  

^a UNIVERSITY OF SUSSEX   (United Kingdom)

^b UNIVERSITY OF ZURICH   (Switzerland)

^c UNIVERSITY OF TORONTO   (Canada)

^d LOS ALAMOS NATIONAL LABORATORY   (United States)

^e STOCKHOLM UNIVERSITY   (Sweden)

^f Chosun University   (South Korea)

^g The University of Texas at Austin   (United States)

^h OBSERVATOIRE DE PARIS   (France)

ⁱ FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^j UNIVERSITY OF CHICAGO   (United States)

^k UNIVERSITY OF CALIFORNIA   (United States)

^l DURHAM UNIVERSITY   (United Kingdom)

^m SOUTHERN METHODIST UNIVERSITY   (United States)

ⁿ UNIVERSITY OF TSUKUBA   (Japan)

^o UNIVERSITY OF CALIFORNIA   (United States)

^p KONAN UNIVERSITY   (Japan)

^q UNIVERSITY OF ANTWERP   (Belgium)

more..

Author keywords

Cosmology: theory; Galaxies: high redshift; H ii regions; Intergalactic medium; Methods: numerical; Radiative transfer

Indexed keywords

CODES (SYMBOLS); FLOW OF FLUIDS; GALAXIES; HYDRODYNAMICS; IONIZATION OF GASES; NUMERICAL METHODS; RADIATIVE TRANSFER;

APPROXIMATE ANALYTICAL SOLUTIONS; COSMOLOGY: THEORY; DENSITY FIELDS; FLUID-FLOW; GALAXIES:HIGH-REDSHIFT; H II REGION; INTERGALACTIC MEDIUM; METHOD: NUMERICAL; NUMERICAL CODE; RADIATION HYDRODYNAMICS;

COSMOLOGY;

EID: 71849102164     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15558.x     Document Type: Article

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