A (giant) void is not mandatory to explain away dark energy with a Lemaître- Tolman model
- Author
- CELERIER, M.-N1 ; BOLEJKO, K2 3 ; KRASINSKI, A3
[1] Laboratoire Univers et Théories (LUTH), Observatoire de Paris, CNRS, Université Paris-Diderot, 5 place Jules Janssen, 92190 Meudon, France
[2] Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch 7701, South Africa
[3] Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, Bartycka 18, 00 716 Warszawa, Poland - Source
Astronomy and astrophysics (Berlin. Print). 2010, Vol 518, Num 2 ; A21.1-A21.10 ; ref : 1/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- cosmology: dark energy cosmology: miscellaneous
- Keyword (fr)
- Algorithme Constante temps Cosmologie Cône lumière Densité courant Diamètre angulaire Distribution masse Déplacement vers le rouge Energie sombre Equation évolution Espace temps Modèle Métrique Tolman Observable
- Keyword (en)
- Algorithms Time constant Cosmology Light cones Current density Angular diameter Mass distribution Red shift Dark energy Evolution equation Space-time Models Tolman metric Observables
- Keyword (es)
- Constante tiempo Diamétro angular Ecuación evolución Modelo Métrico Tolman
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 23691796
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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