Motivated by the gauge theory of gravity with local scaling symmetry proposed recently in [1,2], we investigate whether the scalar field therein can be responsible for the inflation. We show that the classical theory would suffer from the difficulty that inflation can start but will never stop. We explore possible solutions by invoking the symmetry breaking through quantum effects. The effective potential of the scalar field is shown to have phenomenologically interesting forms to give viable inflation models. The predictions of physical observables agree well with current cosmological measurements and can be further tested in future experiments searching for primordial gravitational waves
In scale-invariant models of fundamental physics all mass scales are generated via spontaneous symme...
We consider inflation within a model framework where the Higgs boson arises as a pseudo-Goldstone bo...
When inflation is driven by a pseudoscalar field χ coupled to vectors as α4χFF˜, this coupling may l...
A scale-invariant universe can have a period of accelerated expansion at early times: inflation. We ...
Inflation is studied in the context of induced gravity (IG) γσ2R, where R is the Ricci sca...
We investigate the inflationary implications of extensions of Poincare symmetry. The simplest constr...
Abstract We propose a new inflation scenario in flux compactification, where a zero mode scalar fiel...
Cosmic inflation not only sets the initial conditions for the evolution of the universe but also pro...
We construct a model of inflation based on a low-energy effective theory of spontaneously broken glo...
AbstractWe examine the role of using symmetry and effective field theory in inflationary model build...
We argue, at a very basic effective field theory level, that higher dimension operators in scalar th...
We examine the role of using symmetry and effective field theory in inflationary model building. We ...
We point out that a successful inflationary magnetogenesis could be realised if we break the local U...
We investigate models in which inflation is driven by an ultraviolet safe and interacting scalar sec...
We study the Wheeler-DeWitt equation for a class of induced gravity models in the minisuperspace app...
In scale-invariant models of fundamental physics all mass scales are generated via spontaneous symme...
We consider inflation within a model framework where the Higgs boson arises as a pseudo-Goldstone bo...
When inflation is driven by a pseudoscalar field χ coupled to vectors as α4χFF˜, this coupling may l...
A scale-invariant universe can have a period of accelerated expansion at early times: inflation. We ...
Inflation is studied in the context of induced gravity (IG) γσ2R, where R is the Ricci sca...
We investigate the inflationary implications of extensions of Poincare symmetry. The simplest constr...
Abstract We propose a new inflation scenario in flux compactification, where a zero mode scalar fiel...
Cosmic inflation not only sets the initial conditions for the evolution of the universe but also pro...
We construct a model of inflation based on a low-energy effective theory of spontaneously broken glo...
AbstractWe examine the role of using symmetry and effective field theory in inflationary model build...
We argue, at a very basic effective field theory level, that higher dimension operators in scalar th...
We examine the role of using symmetry and effective field theory in inflationary model building. We ...
We point out that a successful inflationary magnetogenesis could be realised if we break the local U...
We investigate models in which inflation is driven by an ultraviolet safe and interacting scalar sec...
We study the Wheeler-DeWitt equation for a class of induced gravity models in the minisuperspace app...
In scale-invariant models of fundamental physics all mass scales are generated via spontaneous symme...
We consider inflation within a model framework where the Higgs boson arises as a pseudo-Goldstone bo...
When inflation is driven by a pseudoscalar field χ coupled to vectors as α4χFF˜, this coupling may l...