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A brief analysis of self-gravitating polytropic models with a non-zero cosmological constant (Research Note)

Author
MERAFINA, M1 ; BISNOVATYI-KOGAN, G. S2 ; TARASOV, S. O3
[1] University of Rome La Sapienza, Department of Physics, Piazzale Aldo Moro 2, 00185 Rome, Italy
[2] Space Research Institute (IKI) Profsoyuznaya 84/32, 117997 Moscow, Russian Federation
[3] National Research Nuclear University MEPHI, Kashirskoe Shosse 31, 115409 Moscow, Russian Federation
Source

Astronomy and astrophysics (Berlin. Print). 2012, Vol 541 ; L13.1-L13.4 ; 2 ; 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
Russian
Author keyword
dark energy dark matter galaxies: clusters: general
Keyword (fr)
Amas galaxies Constante cosmologique Cosmologie Energie sombre Equation état Etat équilibre Matière sombre Modèle Polytrope Sphère Stabilité dynamique Système autogravitant Valeur critique
Keyword (en)
Galaxy clusters Cosmological constant Cosmology Dark energy Equations of state Equilibrium state Dark matter Models Polytropes Spheres Dynamic stability Self-gravitating systems Critical value
Keyword (es)
Estado equilibrio Modelo Valor crítico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
26196419

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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