We investigate the one loop effective potential of inflation in a standard model of chaotic inflation. The leading one loop corrections to the effective inflaton potential are evaluated in the quasi de Sitter background, and we estimate the one loop correction to the two-point function of the inflaton perturbations in the Hartree approximation. In this approximation, the one loop corrections depends on the total number of e-foldings of inflation and the maximal effect is estimated to be a correction to the power spectrum of a few percent. However, such a correction may be difficult to disentangle from the background in the simplest scenario
The precision reached by the recent CMB measurements gives new insights into the shape of the primor...
We present the status of our study into the feasibility of estimating the parameters of inflation fr...
Slow-roll inflation can be studied as an effective field theory. The form of the inflaton potential ...
In this paper we extend our previous treatment of the one-loop corrections to inflation. Previously ...
An estimate of the one-loop correction to the power spectrum of the primordial curvature perturbatio...
We compute one-loop corrections to the power spectrum of the curvature perturbation in single-field ...
In loop quantum cosmology, the universe avoids a big bang singularity and undergoes an early and sho...
International audienceWe obtain the effective inflaton potential during slow-roll inflation by inclu...
The observed power spectrum of the cosmic microwave background (CMB) is consistent with inflationary...
International audienceInflation is today a part of the Standard Model of the Universe supported by t...
We calculate one-loop correction to the two-point functions of curvature perturbation in single-fiel...
Quantum theory of cosmological fluctuations with other matters is studied to higher order to unders...
The most widely studied formation mechanism of a primordial black hole (PBH) is collapse of large-am...
A novel inflection-point inflation model is analysed. The model considers a massless scalar field, w...
We study loop corrections to correlation functions of inflationary perturbations. Previous calculati...
The precision reached by the recent CMB measurements gives new insights into the shape of the primor...
We present the status of our study into the feasibility of estimating the parameters of inflation fr...
Slow-roll inflation can be studied as an effective field theory. The form of the inflaton potential ...
In this paper we extend our previous treatment of the one-loop corrections to inflation. Previously ...
An estimate of the one-loop correction to the power spectrum of the primordial curvature perturbatio...
We compute one-loop corrections to the power spectrum of the curvature perturbation in single-field ...
In loop quantum cosmology, the universe avoids a big bang singularity and undergoes an early and sho...
International audienceWe obtain the effective inflaton potential during slow-roll inflation by inclu...
The observed power spectrum of the cosmic microwave background (CMB) is consistent with inflationary...
International audienceInflation is today a part of the Standard Model of the Universe supported by t...
We calculate one-loop correction to the two-point functions of curvature perturbation in single-fiel...
Quantum theory of cosmological fluctuations with other matters is studied to higher order to unders...
The most widely studied formation mechanism of a primordial black hole (PBH) is collapse of large-am...
A novel inflection-point inflation model is analysed. The model considers a massless scalar field, w...
We study loop corrections to correlation functions of inflationary perturbations. Previous calculati...
The precision reached by the recent CMB measurements gives new insights into the shape of the primor...
We present the status of our study into the feasibility of estimating the parameters of inflation fr...
Slow-roll inflation can be studied as an effective field theory. The form of the inflaton potential ...