activity
19992015
most citedA Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration

2k citations · 6.7k across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.CO2015★ 2 cited

On the Scale of Inflation

C. Armendariz-Picon

Because the scale of inflation is conformal frame dependent, in order to fully characterize it one should quote its value in terms of all the independent equal-time dimensionless r…

astro-ph2008★ 31 cited

Bayesian Limits on Primordial Isotropy Breaking

C. Armendariz-Picon, Larne Pekowsky

It is often assumed that primordial perturbations are statistically isotropic, which implies, among other properties, that their power spectrum is invariant under rotations. In thi…

astro-ph2007★ 44 cited

Creating Statistically Anisotropic and Inhomogeneous Perturbations

C. Armendariz-Picon

In almost all structure formation models, primordial perturbations are created within a homogeneous and isotropic universe, like the one we observe. Because their ensemble averages…

astro-ph2006★ 21 cited

Why should primordial perturbations be in a vacuum state?

C. Armendariz-Picon

In order to calculate the power spectrum generated during a stage of inflation, we have to specify the quantum state of the inflaton perturbations, which is conventionally assumed…

astro-ph2006★ 42 cited

Near Scale Invariance with Modified Dispersion Relations

C. Armendariz-Picon

We describe a novel mechanism to seed a nearly scale invariant spectrum of adiabatic perturbations during a non-inflationary stage. It relies on a modified dispersion relation that…

astro-ph2005★ 35 cited

Footprints of Statistical Anisotropies

C. Armendariz-Picon

We propose and develop a formalism to describe and constrain statistically anisotropic primordial perturbations. Starting from a decomposition of the primordial power spectrum in s…