We present some results concerning the large volume limit of loop quantum cosmology in the flat homogeneous and isotropic case. We derive the Wheeler-De Witt equation in this limit. Looking for the action from which this equation can also be obtained, we then address the problem of the modifications to be brought to the Friedman's equation of motion and to the equation of motion of the scalar field, in the classical limit
Loop quantum cosmology corrections to Wheeler-DeWitt's equation for Friedmann's model have been cons...
8 pagesInternational audienceWe compute the transition amplitude between coherent quantum-states of ...
8 pagesInternational audienceWe compute the transition amplitude between coherent quantum-states of ...
In loop quantum cosmology, a difference equation for the wave function describes the evolution of a ...
In loop quantum cosmology, a difference equation for the wave function describes the evolution of a ...
We develop an action principle for those models arising from isotropic loop quantum cosmology, and s...
The flat, homogeneous, and isotropic universe with a massless scalar field is a paradigmatic model i...
Quantum gravity is expected to be necessary in order to understand situations where classical genera...
The use of techniques from loop quantum gravity for cosmological models may solve some difficult pro...
Quantum gravity is expected to be necessary in order to understand situations in which classical gen...
Quantum gravity is expected to be necessary in order to understand situations in which classical gen...
Quantum gravity is expected to be necessary in order to understand situations where classical genera...
Isotropic models in loop quantum cosmology allow explicit calculations, thanks largely to a complete...
The cosmological application of the low energy effective action of string theory with perfect fluid ...
To derive loop quantum cosmology from loop quantum gravity, I apply the model given in [48] to a sys...
Loop quantum cosmology corrections to Wheeler-DeWitt's equation for Friedmann's model have been cons...
8 pagesInternational audienceWe compute the transition amplitude between coherent quantum-states of ...
8 pagesInternational audienceWe compute the transition amplitude between coherent quantum-states of ...
In loop quantum cosmology, a difference equation for the wave function describes the evolution of a ...
In loop quantum cosmology, a difference equation for the wave function describes the evolution of a ...
We develop an action principle for those models arising from isotropic loop quantum cosmology, and s...
The flat, homogeneous, and isotropic universe with a massless scalar field is a paradigmatic model i...
Quantum gravity is expected to be necessary in order to understand situations where classical genera...
The use of techniques from loop quantum gravity for cosmological models may solve some difficult pro...
Quantum gravity is expected to be necessary in order to understand situations in which classical gen...
Quantum gravity is expected to be necessary in order to understand situations in which classical gen...
Quantum gravity is expected to be necessary in order to understand situations where classical genera...
Isotropic models in loop quantum cosmology allow explicit calculations, thanks largely to a complete...
The cosmological application of the low energy effective action of string theory with perfect fluid ...
To derive loop quantum cosmology from loop quantum gravity, I apply the model given in [48] to a sys...
Loop quantum cosmology corrections to Wheeler-DeWitt's equation for Friedmann's model have been cons...
8 pagesInternational audienceWe compute the transition amplitude between coherent quantum-states of ...
8 pagesInternational audienceWe compute the transition amplitude between coherent quantum-states of ...