We present new observational constraints on inhomogeneous models based on observables independent of the CMB and large-scale structure. Using Bayesian evidence we find very strong evidence for the homogeneous LCDM model, thus disfavouring inhomogeneous 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
AbstractWe explore how local, cosmology-independent measurements of the Hubble constant and the age ...
Cosmological observables could be used to construct cosmological models; however, a fixed number of ...
AbstractAs is well known, one can explain the current cosmic acceleration by considering an inhomoge...
We present new observational constraints on inhomogeneous models based on observables independent of...
In this paper, instead of invoking Dark Energy, we try and fit various cosmological observations wit...
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...
Abstract. We present new observational constraints on inhomogeneous models based on ob-servables ind...
The apparent accelerating expansion of the Universe, determined from observations of distant superno...
We explore how local, cosmology-independent measurements of the Hubble constant and the age of the U...
We present the first cosmological constraints derived from the analysis of the void size function. T...
As is well known, one can explain the current cosmic acceleration by considering an inhomogeneous an...
As is well known, one can explain the current cosmic acceleration by considering an inhomogeneous an...
A suggested solution to the dark energy problem is the void model, where accelerated expansion is r...
If the voids that we see today in the distribution of galaxies existed at recombination, they will l...
AbstractWe explore how local, cosmology-independent measurements of the Hubble constant and the age ...
Cosmological observables could be used to construct cosmological models; however, a fixed number of ...
AbstractAs is well known, one can explain the current cosmic acceleration by considering an inhomoge...
We present new observational constraints on inhomogeneous models based on observables independent of...
In this paper, instead of invoking Dark Energy, we try and fit various cosmological observations wit...
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...
Abstract. We present new observational constraints on inhomogeneous models based on ob-servables ind...
The apparent accelerating expansion of the Universe, determined from observations of distant superno...
We explore how local, cosmology-independent measurements of the Hubble constant and the age of the U...
We present the first cosmological constraints derived from the analysis of the void size function. T...
As is well known, one can explain the current cosmic acceleration by considering an inhomogeneous an...
As is well known, one can explain the current cosmic acceleration by considering an inhomogeneous an...
A suggested solution to the dark energy problem is the void model, where accelerated expansion is r...
If the voids that we see today in the distribution of galaxies existed at recombination, they will l...
AbstractWe explore how local, cosmology-independent measurements of the Hubble constant and the age ...
Cosmological observables could be used to construct cosmological models; however, a fixed number of ...
AbstractAs is well known, one can explain the current cosmic acceleration by considering an inhomoge...