We present a minimal axion inflation model which can generate a large tensor-to-scalar ratio while remaining sub-Planckian. The modulus of a complex scalar field Phi with a lambda vertical bar Phi vertical bar(4) potential couples directly to the gauge field of a strongly-coupled sector via a term of the form (vertical bar Phi vertical bar/M-Pl)(m) F (F) over tilde . This generates a minimum of the potential which is aperiodic in the phase. The resulting inflation model is equivalent to a phi(4/(m+1)) chaotic inflation model. For the natural case of a leading-order portal-like interaction of the form Phi dagger Phi F (F) over tilde, the model is equivalent to a phi(4/3) chaotic inflation model and predicts a tensor-to-scalar ratio r = 16/3N...
We reexamine inflation due to a constrained inflaton in the model of a complex scalar. Inflaton evol...
The BICEP2 observation of a large tensor-to-scalar ratio, r = 0.20+0.07-0.05, implies that the infla...
We reexamine inflation due to a constrained inflaton in the model of a complex scalar. Inflaton evol...
The minimal sub-Planckian axion inflation model accounts for a large scalar-to-tensor ratio via a sp...
The BICEP2 observation of a large tensor-to-scalar ratio, r = 0.20(-0.05)(+0.07), implies that the i...
The minimal sub-Planckian axion inflation model accounts for a large scalar-to-tensor ratio via a sp...
We propose a novel scenario of primordial inflation in which the inflaton goes through a spiral moti...
We propose a novel scenario of primordial inflation in which the inflaton goes through a spiral moti...
In this paper my prime objective is to explain the generation of large tensor-to-scalar ratio from t...
In this paper we provide an accurate bound on primordial gravitational waves, i.e. tensor-to-scalar ...
In this paper my prime objective is to explain the generation of large tensor-to-scalar ratio from t...
AbstractIn this paper my prime objective is to explain the generation of large tensor-to-scalar rati...
We use the PLANCK 2018 and the WMAP data to constraint inflation models driven by a scalar field $\p...
AbstractIn this paper we provide an accurate bound on primordial gravitational waves, i.e. tensor-to...
We construct a family of simple single-field inflation models consistent with Planck / BICEP Keck bo...
We reexamine inflation due to a constrained inflaton in the model of a complex scalar. Inflaton evol...
The BICEP2 observation of a large tensor-to-scalar ratio, r = 0.20+0.07-0.05, implies that the infla...
We reexamine inflation due to a constrained inflaton in the model of a complex scalar. Inflaton evol...
The minimal sub-Planckian axion inflation model accounts for a large scalar-to-tensor ratio via a sp...
The BICEP2 observation of a large tensor-to-scalar ratio, r = 0.20(-0.05)(+0.07), implies that the i...
The minimal sub-Planckian axion inflation model accounts for a large scalar-to-tensor ratio via a sp...
We propose a novel scenario of primordial inflation in which the inflaton goes through a spiral moti...
We propose a novel scenario of primordial inflation in which the inflaton goes through a spiral moti...
In this paper my prime objective is to explain the generation of large tensor-to-scalar ratio from t...
In this paper we provide an accurate bound on primordial gravitational waves, i.e. tensor-to-scalar ...
In this paper my prime objective is to explain the generation of large tensor-to-scalar ratio from t...
AbstractIn this paper my prime objective is to explain the generation of large tensor-to-scalar rati...
We use the PLANCK 2018 and the WMAP data to constraint inflation models driven by a scalar field $\p...
AbstractIn this paper we provide an accurate bound on primordial gravitational waves, i.e. tensor-to...
We construct a family of simple single-field inflation models consistent with Planck / BICEP Keck bo...
We reexamine inflation due to a constrained inflaton in the model of a complex scalar. Inflaton evol...
The BICEP2 observation of a large tensor-to-scalar ratio, r = 0.20+0.07-0.05, implies that the infla...
We reexamine inflation due to a constrained inflaton in the model of a complex scalar. Inflaton evol...