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Modeling nonlinear dark energy fluctuations
Ronaldo Carlotto Batista IF-USP
Raul Abramo, Rogério Rosenfeld,
Lamartine Liberato
I Workshop: “Challanges of New Physics in the Space”Campos do Jordão, 30/04/2009
Dark Energy Models
Cosmological Constant
Canonical Scalar Field
Perfect Fluid
e.g. Chaplygin Gas
K-essence
e.g. Tachyon, Born-Infeld
Dark Energy Linear Perturbations
For quintessence
Order of Hubble radius ~ Gpc
Hwang & Noh 2001
Spherical Collapse with DE fluctuations
Mota & van de Bruck 2004
For quintessence:
Spherical Collapse with DE fluctuations
Lima et. al. 1997Pseudo-newtonian Cosmology
Linear Comparison PN - GR PRD arxiv 0902.3226
With pressure gradient
Spherical Collapse App.
Relativistic Spherical Collapse
For perfect fluids:
Linear Nonlinear
Relativistic Spherical Collapse
For quintessence
Relativistic Spherical Collapse
For Dark Matter in EdS
For small scales
Relativistic Spherical Collapse
Dark Matter evolution in EdS
Thanks
This work is supported by FAPESP