We perform an analytical study of the integrated Sachs\u2013Wolfe (ISW) effect within the framework of unified dark matter models based on a scalar field which aim at a unified description of dark energy and dark matter. Computing the temperature power spectrum of the cosmic microwave background anisotropies we are able to isolate those contributions that can potentially lead to strong deviations from the usual ISW effect occurring in a \u39bCDM universe. This helps to highlight the crucial role played by the sound speed in the unified dark matter models. Our treatment is completely general in that all the results depend only on the speed of sound of the dark component and thus it can be applied to a variety of unified models, including tho...
Interacting dark matter-dark energy (IDMDE) models can be taken to account as one of the present cha...
Context. One of the main challenges of modern cosmology is to understand the nature of the mysteriou...
CMB photons redshift and blueshift as they move through gravitational potentials $\Phi$ while propag...
We perform an analytical study of the Integrated Sachs-Wolfe (ISW) effect within the framework of Un...
In this thesis I have investigated the possibility that the dynamics of a single scalar field can ...
Dark energy perturbations are normally either neglected or else included in a purely numerical way, ...
5 pages, 5 figuresInternational audienceWe study the integrated Sachs-Wolfe (ISW) effect using a mod...
We outline a gauge-invariant framework to calculate cosmological perturbations in dark energy models...
Artículo de publicación ISICosmological fluids are commonly assumed to be distributed in a spatially...
This capstone develops tools usable for the detection of the Integrated Sachs-Wolfe Effect within th...
Using a directional spherical wavelet analysis we detect the integrated Sachs-Wolfe (ISW) effect, in...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographica...
15 pages, 17 figures. Added discussion, references, 2 new figures. Minor errors fixed in the calcula...
We use scalar field Lagrangians with a non-canonical kinetic term to obtain unified dark matter mode...
International audienceThe late integrated Sachs-Wolfe (ISW) effect correlates the cosmic microwave b...
Interacting dark matter-dark energy (IDMDE) models can be taken to account as one of the present cha...
Context. One of the main challenges of modern cosmology is to understand the nature of the mysteriou...
CMB photons redshift and blueshift as they move through gravitational potentials $\Phi$ while propag...
We perform an analytical study of the Integrated Sachs-Wolfe (ISW) effect within the framework of Un...
In this thesis I have investigated the possibility that the dynamics of a single scalar field can ...
Dark energy perturbations are normally either neglected or else included in a purely numerical way, ...
5 pages, 5 figuresInternational audienceWe study the integrated Sachs-Wolfe (ISW) effect using a mod...
We outline a gauge-invariant framework to calculate cosmological perturbations in dark energy models...
Artículo de publicación ISICosmological fluids are commonly assumed to be distributed in a spatially...
This capstone develops tools usable for the detection of the Integrated Sachs-Wolfe Effect within th...
Using a directional spherical wavelet analysis we detect the integrated Sachs-Wolfe (ISW) effect, in...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographica...
15 pages, 17 figures. Added discussion, references, 2 new figures. Minor errors fixed in the calcula...
We use scalar field Lagrangians with a non-canonical kinetic term to obtain unified dark matter mode...
International audienceThe late integrated Sachs-Wolfe (ISW) effect correlates the cosmic microwave b...
Interacting dark matter-dark energy (IDMDE) models can be taken to account as one of the present cha...
Context. One of the main challenges of modern cosmology is to understand the nature of the mysteriou...
CMB photons redshift and blueshift as they move through gravitational potentials $\Phi$ while propag...