Abstract We present a new mechanism for inflation which exhibits a speed limit on scalar motion, generating accelerated expansion even on a steep potential. This arises from explicitly integrating out the short modes of additional fields coupled to the inflaton ϕ via a dimension six operator, yielding an expression for the effective action which includes a nontrivial (logarithmic) function of (∂ϕ)2. The speed limit appears at the branch cut of this logarithm arising in a large flavor expansion, similarly to the square root branch cut in DBI inflation arising in a large color expansion. Finally, we describe observational constraints on the parameters of this model
Observations of the cosmic microwave background do not yet determine whether inflation was driven by...
We re-examine large scalar fields within effective field theory, in particular focussing on the issu...
Observations of the cosmic microwave background do not yet determine whetherinflation was driven by ...
The viability of a given model for inflation is determined not only by the form of the inflaton pote...
We examine inflationary universe models driven by scalar fields with logarithmic potentials of the f...
International audienceSlow-roll inflation is studied as an effective field theory. We find that the ...
We suggest a new type of hill-top inflation originating from the initial conditions in the form of t...
14 pages, no figures, version to appear in Phys Rev DSlow-roll inflation is studied as an effective ...
14 pages, no figures, version to appear in Phys Rev DSlow-roll inflation is studied as an effective ...
AbstractWe propose a new class of inflation models in which the coefficient of the inflaton kinetic ...
International audienceSlow-roll inflation is studied as an effective field theory. We find that the ...
14 pages, no figures, version to appear in Phys Rev DSlow-roll inflation is studied as an effective ...
International audienceSlow-roll inflation is studied as an effective field theory. We find that the ...
We re-examine large scalar fields within effective field theory, in particular focussing on the issu...
International audienceSlow-roll inflation is studied as an effective field theory. We find that the ...
Observations of the cosmic microwave background do not yet determine whether inflation was driven by...
We re-examine large scalar fields within effective field theory, in particular focussing on the issu...
Observations of the cosmic microwave background do not yet determine whetherinflation was driven by ...
The viability of a given model for inflation is determined not only by the form of the inflaton pote...
We examine inflationary universe models driven by scalar fields with logarithmic potentials of the f...
International audienceSlow-roll inflation is studied as an effective field theory. We find that the ...
We suggest a new type of hill-top inflation originating from the initial conditions in the form of t...
14 pages, no figures, version to appear in Phys Rev DSlow-roll inflation is studied as an effective ...
14 pages, no figures, version to appear in Phys Rev DSlow-roll inflation is studied as an effective ...
AbstractWe propose a new class of inflation models in which the coefficient of the inflaton kinetic ...
International audienceSlow-roll inflation is studied as an effective field theory. We find that the ...
14 pages, no figures, version to appear in Phys Rev DSlow-roll inflation is studied as an effective ...
International audienceSlow-roll inflation is studied as an effective field theory. We find that the ...
We re-examine large scalar fields within effective field theory, in particular focussing on the issu...
International audienceSlow-roll inflation is studied as an effective field theory. We find that the ...
Observations of the cosmic microwave background do not yet determine whether inflation was driven by...
We re-examine large scalar fields within effective field theory, in particular focussing on the issu...
Observations of the cosmic microwave background do not yet determine whetherinflation was driven by ...