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- Clifford Cheung, Paolo Creminelli, A. Liam Fitzpatrick, Jared Kaplan, Leonardo Senatore
- 2008

We study the effective field theory of inflation, i.e. the most general theory describing the fluctuations around a quasi de Sitter background, in the case of single field models. The scalar mode can be eaten by the metric by going to unitary gauge. In this gauge, the most general theory is built with the lowest dimension operators invariant under spatial… (More)

- Paolo Creminelli
- 2003

We study the impact of higher dimension operators in the inflaton Lagrangian on the non-gaussianity of the scalar spectrum. These terms can strongly enhance the effect without spoiling slow-roll, though it is difficult to exceed f NL ∼ 1, because the scale which suppresses the operators cannot be too low, if we want the effective field theory description to… (More)

- Nima Arkani-Hamed, Paolo Creminelli, Shinji Mukohyama, Matias Zaldarriaga
- 2003

We propose a new scenario for early cosmology, where an inflationary de Sitter phase is obtained with a ghost condensate. The transition to radiation dominance is triggered by the ghost itself, without any slow-roll potential. Density perturbations are generated by fluctuations around the ghost condensate and can be reliably computed in the effective field… (More)

- Daniel Babich, Paolo Creminelli, Matias Zaldarriaga
- 2004

We study the dependence on configuration in momentum space of the primordial 3-point function of density perturbations in several different scenarios: standard slow-roll inflation, curvaton and variable decay models, ghost inflation, models with higher derivative operators and the DBI model of inflation. We define a cosine between the distributions using a… (More)

- Paolo Creminelli, Markus A. Luty, Alberto Nicolis, Leonardo Senatore
- 2006

We present a consistent effective theory that violates the null energy condition (NEC) without developing any instabilities or other pathological features. The model is the ghost condensate with the global shift symmetry softly broken by a potential. We show that this system can drive a cosmological expansion with ˙ H > 0. Demanding the absence of… (More)

- Paolo Creminelli, Leonardo Senatore
- 2007

We present a bouncing cosmology which evolves from the contracting to the expanding phase in a smooth way, without developing instabilities or pathologies and remaining in the regime of validity of 4d effective field theory. A nearly scale invariant spectrum of perturbations is generated during the contracting phase by an isocurvature scalar with a negative… (More)

- Paolo Creminelli, Alberto Nicolis, Leonardo Senatore, Max Tegmark, Matias Zaldarriaga
- 2005

We develop a method to constrain the level of non-Gaussianity of density perturbations when the 3-point function is of the " equilateral " type. Departures from Gaussianity of this form are produced by single field models such as ghost or DBI inflation and in general by the presence of higher order derivative operators in the effective Lagrangian of the… (More)

For bouncing cosmologies such as the ekpyrotic/cyclic scenarios we show that it is possible to make predictions for density perturbations which are independent of the details of the bouncing phase. This can be achieved, as in inflationary cosmology, thanks to the existence of a dynamical attractor, which makes local observables equal to the unperturbed… (More)

- Paolo Creminelli, Alberto Nicolis, Riccardo Rattazzi
- 2008

We study through holography the compact Randall-Sundrum (RS) model at finite temperature. In the presence of radius stabilization, the system is described at low enough temperature by the RS solution. At high temperature it is described by the AdS-Schwarzschild solution with an event horizon replacing the TeV brane. We calculate the transition temperature T… (More)

- Riccardo Barbieri, Paolo Creminelli, Alessandro Strumia, Nikolaos Tetradis
- 1999

Baryogenesis by heavy-neutrino decay and sphaleron reprocessing of both baryon and lepton number is reconsidered, paying special attention to the flavour structure of the general evolution equations and developing an approximate but sufficiently accurate analytic solution to the prototype evolution equation. Two different models of neutrino masses are… (More)