Add to ORKGWe consider cosmic microwave background (CMB) anisotropy in models with quintessence taking into account of isocurvature fluctuation in the quintessence. It is shown that, if the primordial fluctuation of the quintessence has a correlation with the adiabatic density fluctuations, CMB angular power spectrum C_l at low multipoles can be suppressed without affecting C_l at high multipoles. Possible scenario of generating correlated mixture of the quintessence and adiabatic fluctuations is also discussed
AbstractWe study the cosmic microwave background (CMB) anisotropy in the scenario where the baryon a...
We study the anisotropy of the cosmic microwave background (CMB) in cold and mixed dark matter (CDM ...
AbstractWe discuss cosmic microwave background anisotropies in models with an unconventional primord...
We consider cosmic microwave background (CMB) anisotropy in models with quintessence, taking into ac...
We examine the cosmic microwave background (CMB) anisotropy for signatures of early quintessence dar...
If the Universe is flat, as predicted by inflationary cosmology, then the vast majority of the cosmi...
We use cosmic microwave background (CMB) and large-scale structure data to constrain cosmological mo...
AbstractWe consider effects of the isocurvature perturbation in the framework of the tracker-type qu...
We analyze the evolution of energy density fluctuations in cosmological scenarios with a mixture of ...
18 pages, 20 figuresRecent high precision measurements of the CMB anisotropies performed by the BOOM...
The Cosmic Microwave Background (CMB) anisotropy power on the largest angular scales observed both b...
We describe the observable features of the recently proposed Extended Quintessence scenarios on the ...
We perform a detailed comparison of the Wilkinson Microwave Anisotropy Probe (WMAP) measurements of ...
Prompted by the recent MAXIMA-1 and BOOMERANG-98 measurements of the cosmic microwave background (CM...
We examine the cosmic microwave background (CMB) anisotropy for signatures of early quintessence dar...
AbstractWe study the cosmic microwave background (CMB) anisotropy in the scenario where the baryon a...
We study the anisotropy of the cosmic microwave background (CMB) in cold and mixed dark matter (CDM ...
AbstractWe discuss cosmic microwave background anisotropies in models with an unconventional primord...
We consider cosmic microwave background (CMB) anisotropy in models with quintessence, taking into ac...
We examine the cosmic microwave background (CMB) anisotropy for signatures of early quintessence dar...
If the Universe is flat, as predicted by inflationary cosmology, then the vast majority of the cosmi...
We use cosmic microwave background (CMB) and large-scale structure data to constrain cosmological mo...
AbstractWe consider effects of the isocurvature perturbation in the framework of the tracker-type qu...
We analyze the evolution of energy density fluctuations in cosmological scenarios with a mixture of ...
18 pages, 20 figuresRecent high precision measurements of the CMB anisotropies performed by the BOOM...
The Cosmic Microwave Background (CMB) anisotropy power on the largest angular scales observed both b...
We describe the observable features of the recently proposed Extended Quintessence scenarios on the ...
We perform a detailed comparison of the Wilkinson Microwave Anisotropy Probe (WMAP) measurements of ...
Prompted by the recent MAXIMA-1 and BOOMERANG-98 measurements of the cosmic microwave background (CM...
We examine the cosmic microwave background (CMB) anisotropy for signatures of early quintessence dar...
AbstractWe study the cosmic microwave background (CMB) anisotropy in the scenario where the baryon a...
We study the anisotropy of the cosmic microwave background (CMB) in cold and mixed dark matter (CDM ...
AbstractWe discuss cosmic microwave background anisotropies in models with an unconventional primord...