A test suite for quantitative comparison of hydrodynamic codes in astrophysics
- Author
- TASKER, Elizabeth J1 ; BRUNINO, Riccardo2 ; MITCHELL, Nigel L3 ; MICHIELSEN, Dolf2 ; HOPTON, Stephen2 ; PEARCE, Frazer R2 ; BRYAN, Greg L4 ; THEUNS, Tom3 5
[1] Department ofAstronomy, University of Florida, Gainesville, FL 32611, United States
[2] Department of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom
[3] Department of Physics, Institute for Computational Cosmology, University of Durham, South Road, Durham DH1 3LE, United Kingdom
[4] Department of Astronomy, Columbia University, New York, NY 10027, United States
[5] Department of Physics, University of Antwerp, Groenenborgerlaan 171, 2020 Antwerpen, Belgium - Source
Monthly Notices of the Royal Astronomical Society. 2008, Vol 390, Num 3, pp 1267-1281, 15 p ; ref : 1/4 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- cosmology: theory hydrodynamics methods: numerical
- Keyword (fr)
- Cosmologie Explosion supernova Gradient densité Lagrangien Modèle hydrodynamique Méthode Lagrange Méthode numérique Onde acoustique Onde choc Sphère
- Keyword (en)
- Cosmology Supernovae explosion Density gradient Lagrangian Hydrodynamic model Lagrangian method Numerical method Acoustic waves Shock waves Spheres
- Keyword (es)
- Explosión supernova Gradiente densidad Lagrangiano Método Lagrange Método numérico
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20781452
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1111/j.1365-2966.2008.13836.x 
https://dx.doi.org/10.1111/j.1365-2966.2008.13836.x
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