activity
19922014
most citedParticle Physics Models of Inflation and the Cosmological Density Perturbation

1.9k citations · 16.3k across the 107 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

8 papers · 2 filters

astro-ph2005★ 139 cited

Inflation models and observation

Laila Alabidi, David Lyth

We consider small-field models which invoke the usual framework for the effective field theory, and large-field models which go beyond that. Present and future possibilities for di…

astro-ph2005★ 206 cited

Generating the curvature perturbation at the end of inflation

David H. Lyth

The dominant contribution to the primordial curvature perturbation may be generated at the end of inflation. Taking the end of inflation to be sudden, formulas are presented for th…

astro-ph2005★ 40 cited

Forming sub-horizon black holes at the end of inflation

David. H Lyth, Karim A. Malik, Misao Sasaki +1

Previous authors have calculated the mass function of primordial black holes only on scales which are well outside the horizon at the end of inflation. Here we extend the calculati…

astro-ph2005

The bound on the primordial tensor perturbation

David H. Lyth

I recall the well-known sufficient conditions for the bound on the spectrum of the primordial tensor perturbation. Two recent papers claim a violation of this bound, withou…

astro-ph2005★ 58 cited

A Bound Concerning Primordial Non-Gaussianity

David H. Lyth, Ignacio Zaballa

Seery and Lidsey have calculated the three-point correlator of the light scalar fields, a few Hubble times after horizon exit during inflation. Lyth and Rodriguez have calculated t…

astro-ph2005★ 202 cited

Detecting a small perturbation through its non-Gaussianity

Lotfi Boubekeur, David. H. Lyth

A highly non-gaussian cosmological perturbation with a flat spectrum has unusual stochastic properties. We show that they depend on the size of the box within which the perturbatio…

astro-ph2005★ 629 cited

The inflationary prediction for primordial non-gaussianity

David H. Lyth, Yeinzon Rodriguez

We extend the δN formalism so that it gives all of the stochastic properties of the primordial curvature perturbation ζif the initial field perturbations are gaussian. The calculat…

astro-ph2005★ 145 cited

Non-gaussianity from the second-order cosmological perturbation

David H. Lyth, Yeinzon Rodriguez

Several conserved and/or gauge invariant quantities described as the second-order curvature perturbation have been given in the literature. We revisit various scenarios for the gen…