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most citedNon-gaussianity from the second-order cosmological perturbation

145 citations · 1.2k across the 20 of their papers we have counts for

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7 papers · 1 filter

astro-ph200668 cited

Generating the Curvature Perturbation at the End of Inflation in String Theory

D. H. Lyth, A. Riotto

In brane inflationary scenarios, the cosmological perturbations are supposed to originate from the vacuum fluctuations of the inflaton field corresponding to the position of the br…

astro-ph200651 cited

Classicality of the primordial perturbations

David H. Lyth, David Seery

We show that during inflation, a quantum fluctuation becomes classical at all orders if it becomes classical at first order. Implications are discussed.

astro-ph200670 cited

Curvature perturbation from symmetry breaking the end of inflation

Laila Alabidi, David Lyth

We consider a two-field hybrid inflation model, in which the curvature perturbation is predominantly generated at the end of inflation. By finely tuning the coupling of the fields…

astro-ph2006131 cited

A numerical study of non-gaussianity in the curvaton scenario

Karim A. Malik, David H. Lyth

We study the curvaton scenario using gauge-invariant second order perturbation theory and solving the governing equations numerically. Focusing on large scales we calculate the non…

astro-ph200655 cited

Inflation models after WMAP year three

Laila Alabidi, David H. Lyth

The survey of models in astro-ph/0510441 is updated.For the first time, a large fraction of the models is ruled out at more than .

astro-ph200685 cited

Non-gaussianity and cosmic uncertainty in curvaton-type models

D. H. Lyth

In curvaton-type models, observable non-gaussianity of the curvature perturbation would come from a contribution of the form , where is gaussian. I analyse this situat…