Abstract. We present new observational constraints on inhomogeneous models based on ob-servables independent of the CMB and large-scale structure. Using Bayesian evidence we find very strong evidence for the homogeneous LCDM model, thus disfavouring inhomoge-neous models. Our new constraints are based on quantities independent of the growth of perturbations and rely on cosmic clocks based on atomic physics and on the local density of matter. ar X i
The search for the physical mechanism underlying the observational evidence for the acceleration of ...
Cosmological models for structure formation are severely constrained by several of the recent observ...
Measurements of the SNe Ia Hubble diagram which suggest that the universe is accelerating due to the...
We present new observational constraints on inhomogeneous models based on observables independent of...
Abstract. It has been proposed that the observed dark energy can be explained away by the effect of ...
We find that if we live at the center of an inhomogeneity with total density contrast |δ0 | ' ...
International audienceRecently, spatially inhomogeneous cosmological models have been proposed as an...
Do current observational data confirm the assumptions of the cosmological principle, or is there sta...
Do current observational data confirm the assumptions of the cosmological principle, or is there sta...
Cosmological observables could be used to construct cosmological models; however, a fixed number of ...
We review observational tests for the homogeneity of the Universe on large scales. Redshift and pecu...
We explore how local, cosmology-independent measurements of the Hubble constant and the age of the U...
We study metric-affine gravity (MAG) inspired cosmological models. Those models were statistically e...
Telescopes all around the World are daily collecting huge amounts of data from the sky. However, thi...
We pursue a program to confront observations with inhomogeneous extensions of the FLRW metric. The m...
The search for the physical mechanism underlying the observational evidence for the acceleration of ...
Cosmological models for structure formation are severely constrained by several of the recent observ...
Measurements of the SNe Ia Hubble diagram which suggest that the universe is accelerating due to the...
We present new observational constraints on inhomogeneous models based on observables independent of...
Abstract. It has been proposed that the observed dark energy can be explained away by the effect of ...
We find that if we live at the center of an inhomogeneity with total density contrast |δ0 | ' ...
International audienceRecently, spatially inhomogeneous cosmological models have been proposed as an...
Do current observational data confirm the assumptions of the cosmological principle, or is there sta...
Do current observational data confirm the assumptions of the cosmological principle, or is there sta...
Cosmological observables could be used to construct cosmological models; however, a fixed number of ...
We review observational tests for the homogeneity of the Universe on large scales. Redshift and pecu...
We explore how local, cosmology-independent measurements of the Hubble constant and the age of the U...
We study metric-affine gravity (MAG) inspired cosmological models. Those models were statistically e...
Telescopes all around the World are daily collecting huge amounts of data from the sky. However, thi...
We pursue a program to confront observations with inhomogeneous extensions of the FLRW metric. The m...
The search for the physical mechanism underlying the observational evidence for the acceleration of ...
Cosmological models for structure formation are severely constrained by several of the recent observ...
Measurements of the SNe Ia Hubble diagram which suggest that the universe is accelerating due to the...