A vector curvaton model with a Maxwell kinetic term and varying kinetic function and mass during inflation is studied. It is shown that, if light until the end of inflation, the vector field can generate statistical anisotropy in the curvature perturbation spectrum and bispectrum, with the latter being predominantly anisotropic. If by the end of inflation the vector field becomes heavy, then particle production is isotropic and the vector curvaton can alone generate the curvature perturbation. The model does not suffer from instabilities such as ghosts and is the only concrete model, to date, which can produce the curvature perturbation without direct involvement of fundamental scalar fields
I discuss the possibility of using a massive vector field to generate the density perturbation in th...
We suppose that a vector field perturbation causes part of the primordial curvature perturbation. Th...
Light vector fields during inflation obtain a superhorizon perturbation spectrum when their conforma...
A new model realization of the vector curvaton paradigm is presented and analyzed. The model consist...
We analyze a massive vector field with a non-canonical kinetic term in the action, minimally coupled...
It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing d...
The \delta N formalism is extended to include the perturbation of the vector field. The latter is qu...
It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing d...
The δN formula for the primordial curvature perturbation ζ is extended to include vector as well as ...
We present a mechanism for the origin of the large-scale curvature perturbation in our Universe by t...
We present a mechanism for the origin of the large-scale curvature perturbation in our Universe by t...
I investigate the possibility that the observed curvature perturbation is due to a massive vector fi...
In a model of an Abelian vector boson with a Maxwell kinetic term and non-negative mass-squared it i...
It is shown that a massive Abelian vector boson field can generate the curvature perturbation in the...
In a model of an Abelian vector boson with a Maxwell kinetic term and non-negative mass-squared it i...
I discuss the possibility of using a massive vector field to generate the density perturbation in th...
We suppose that a vector field perturbation causes part of the primordial curvature perturbation. Th...
Light vector fields during inflation obtain a superhorizon perturbation spectrum when their conforma...
A new model realization of the vector curvaton paradigm is presented and analyzed. The model consist...
We analyze a massive vector field with a non-canonical kinetic term in the action, minimally coupled...
It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing d...
The \delta N formalism is extended to include the perturbation of the vector field. The latter is qu...
It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing d...
The δN formula for the primordial curvature perturbation ζ is extended to include vector as well as ...
We present a mechanism for the origin of the large-scale curvature perturbation in our Universe by t...
We present a mechanism for the origin of the large-scale curvature perturbation in our Universe by t...
I investigate the possibility that the observed curvature perturbation is due to a massive vector fi...
In a model of an Abelian vector boson with a Maxwell kinetic term and non-negative mass-squared it i...
It is shown that a massive Abelian vector boson field can generate the curvature perturbation in the...
In a model of an Abelian vector boson with a Maxwell kinetic term and non-negative mass-squared it i...
I discuss the possibility of using a massive vector field to generate the density perturbation in th...
We suppose that a vector field perturbation causes part of the primordial curvature perturbation. Th...
Light vector fields during inflation obtain a superhorizon perturbation spectrum when their conforma...