A primordial gravitational wave background with positive(blue) spectral index is expected in several non-standard inflationary cosmologies where the stress-energy tensor violates the null energy condition. Here we show that a sizable amount of blue gravitational waves is compatible with current cosmological and astrophysical data. So far most of the works on parameter estimation from cosmic microwave background data have assumed a negative or negligible spectral index. The present limits on cosmological parameters, especially on the scalar spectral index, widen up considerably when one allows also for blue tilts of the tensor spectrum. Since the amplitude of the CMB B-mode polarization is larger in these models, future data from Planck are ...
We study a theory of massive tensor gravitons which predicts blue-tilted and largely amplified primo...
In this paper we constrain the cosmological parameters, in particular the tilt of tensor power spect...
We present new constraints on the spectral index n(T) of tensor fluctuations from the recent data ob...
A primordial gravitational wave background with positive(blue) spectral index is expected in several...
We study the tilt of the primordial gravitational waves spectrum. A hint of blue tilt is shown from ...
In some classes of inflationary models, a violation of the null energy condition (NEC) is expected d...
In some classes of inflationary models, a violation of the null energy condition (NEC) is expected d...
Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produ...
Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produ...
In this paper we constrain the cosmological parameters, in particular the tilt of tensor power spect...
Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produ...
Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produ...
We evaluate our capability to constrain the abundance of primordial tensor perturbations (primordial...
The BICEP-2 team has recently reported the positive detection of cosmic microwave background Bmode p...
We evaluate our capability to constrain the abundance of primordial tensor perturbations (primordial...
We study a theory of massive tensor gravitons which predicts blue-tilted and largely amplified primo...
In this paper we constrain the cosmological parameters, in particular the tilt of tensor power spect...
We present new constraints on the spectral index n(T) of tensor fluctuations from the recent data ob...
A primordial gravitational wave background with positive(blue) spectral index is expected in several...
We study the tilt of the primordial gravitational waves spectrum. A hint of blue tilt is shown from ...
In some classes of inflationary models, a violation of the null energy condition (NEC) is expected d...
In some classes of inflationary models, a violation of the null energy condition (NEC) is expected d...
Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produ...
Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produ...
In this paper we constrain the cosmological parameters, in particular the tilt of tensor power spect...
Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produ...
Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produ...
We evaluate our capability to constrain the abundance of primordial tensor perturbations (primordial...
The BICEP-2 team has recently reported the positive detection of cosmic microwave background Bmode p...
We evaluate our capability to constrain the abundance of primordial tensor perturbations (primordial...
We study a theory of massive tensor gravitons which predicts blue-tilted and largely amplified primo...
In this paper we constrain the cosmological parameters, in particular the tilt of tensor power spect...
We present new constraints on the spectral index n(T) of tensor fluctuations from the recent data ob...