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20022009
most citedObservational Signatures and Non-Gaussianities of General Single Field Inflation

978 citations · 2k across the 10 of their papers we have counts for

collaborators

16 papers

astro-ph.CO200915 cited

The Origin of the Universe as Revealed Through the Polarization of the Cosmic Microwave Background

S. Dodelson, R. Easther, S. Hanany +61

Modern cosmology has sharpened questions posed for millennia about the origin of our cosmic habitat. The age-old questions have been transformed into two pressing issues primed for…

astro-ph.CO200936 cited

Non-Gaussianity as a Probe of the Physics of the Primordial Universe and the Astrophysics of the Low Redshift Universe

E. Komatsu, N. Afshordi, N. Bartolo +58

A new and powerful probe of the origin and evolution of structures in the Universe has emerged and been actively developed over the last decade. In the coming decade, non-Gaussiani…

astro-ph2008303 cited

CMBPol Mission Concept Study: Probing Inflation with CMB Polarization

Daniel Baumann, Mark G. Jackson, Peter Adshead +56

We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measu…

hep-th200825 cited

Fine-Tuning in DBI Inflationary Mechanism

Xingang Chen

We show a model-independent fine-tuning issue in the DBI inflationary mechanism. DBI inflation requires a warp factor h small enough to sufficiently slow down the inflaton. On the…

astro-ph2008298 cited

Generation and Characterization of Large Non-Gaussianities in Single Field Inflation

Xingang Chen, Richard Easther, Eugene A. Lim

Inflation driven by a single, minimally coupled, slowly rolling field generically yields a negligible primordial non-Gaussianity. We discuss two distinct mechanisms by which a non-…

hep-th2007102 cited

Comparing Infrared Dirac-Born-Infeld Brane Inflation to Observations

Rachel Bean, Xingang Chen, Hiranya V. Peiris +1

We compare the Infrared Dirac-Born-Infeld (IR DBI) brane inflation model to observations using a Bayesian analysis. The current data cannot distinguish it from the \LambdaCDM model…