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Structure formation in a variable dark energy model and observational constraints

Arbabi Bidgoli, S ; Sharif University of Technology | 2008

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  1. Type of Document: Article
  2. DOI: 10.1007/978-3-540-74713-0_1
  3. Publisher: 2008
  4. Abstract:
  5. The interpretation of a vast number of cosmological observations in the framework of FRW models suggests that the major part of the energy density of the universe is in form of dark energy with still unknown physical nature. In some models for dark energy, which are motivated by particle physics theory, the equation of state and the contribution of dark energy to the energy density of the universe can be variable. Here we study structure formation in a parameterized dark energy model, and compare its predictions with recent observational data, from the Supernova Ia gold sample and the parameters of large scale structure determined by the 2-degree Field Galaxy Redshift Survey (2dFGRS), and put some constraints on the free parameters of this model. © 2008 Springer-Verlag Berlin Heidelberg
  6. Keywords:
  7. Dark energy large scale ; Cold dark matter ; Dark energy model ; Structure growth index
  8. Source: ESO Astrophysics Symposia ; Volume 2008 , 2008 , Pages 3-7 ; 14312433 (ISSN); 3540747125 (ISBN); 9783540747123 (ISBN)
  9. URL: https://link.springer.com/chapter/10.1007/978-3-540-74713-0_1