DOIAbstract
Observational constraints on standard CDM spectra and perturbation spectra with broken scale invariance are discussed
Observational constraints on standard CDM spectra and perturbation spectra with broken scale invariance are discussed
The most general homogeneous statistical ensemble of linear scalar perturbations which are regular a...
A brief account is given of large-scale structure modelling based on the assumption that the initial...
International audienceCMB temperature fluctuation observations provide a precise measurement of the ...
Cosmological models predict transfer functions by which primordial density perturbations develop int...
We study linear power spectra and formation of large scale structures in flat cosmological models wi...
In this Masterthesis the structure formation process in the early universe is considered. At the end...
We have simulated the formation of large-scale structure arising from COBE-normalized spectra comput...
We investigate the performance of Lagrangian perturbation theory up to the second order for two scen...
We consider the most general primordial cosmological perturbation in a universe filled with photons,...
The combined analysis of the cosmic microwave background on large scales and Lyman alpha forest on s...
The shape of the primordial fluctuation spectrum is probed by cosmic microwave background fluctuatio...
We describe an attempt to reconstruct the initial conditions for the formation of cosmological large...
International audienceCMB temperature fluctuation observations provide a precise measurement of the ...
International audienceCMB temperature fluctuation observations provide a precise measurement of the ...
We constrain the form of the primordial power spectrum using Wilkinson Microwave Anisotropy Probe (W...
The most general homogeneous statistical ensemble of linear scalar perturbations which are regular a...
A brief account is given of large-scale structure modelling based on the assumption that the initial...
International audienceCMB temperature fluctuation observations provide a precise measurement of the ...
Cosmological models predict transfer functions by which primordial density perturbations develop int...
We study linear power spectra and formation of large scale structures in flat cosmological models wi...
In this Masterthesis the structure formation process in the early universe is considered. At the end...
We have simulated the formation of large-scale structure arising from COBE-normalized spectra comput...
We investigate the performance of Lagrangian perturbation theory up to the second order for two scen...
We consider the most general primordial cosmological perturbation in a universe filled with photons,...
The combined analysis of the cosmic microwave background on large scales and Lyman alpha forest on s...
The shape of the primordial fluctuation spectrum is probed by cosmic microwave background fluctuatio...
We describe an attempt to reconstruct the initial conditions for the formation of cosmological large...
International audienceCMB temperature fluctuation observations provide a precise measurement of the ...
International audienceCMB temperature fluctuation observations provide a precise measurement of the ...
We constrain the form of the primordial power spectrum using Wilkinson Microwave Anisotropy Probe (W...
The most general homogeneous statistical ensemble of linear scalar perturbations which are regular a...
A brief account is given of large-scale structure modelling based on the assumption that the initial...
International audienceCMB temperature fluctuation observations provide a precise measurement of the ...
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