activity
19922005
most citedNon-gaussianity from the second-order cosmological perturbation

145 citations · 153 across the 5 of their papers we have counts for

collaborators

12 papers

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-ph2005145 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…

hep-ph20042 cited

Note about leptogenesis from gravity waves in models of inflation

David H. Lyth, Yeinzon Rodriguez, Carlos Quimbay

We show how the mechanism recently proposed by Alexander, Peskin, and Sheikh-Jabbari, in which the observed cosmic matter-antimatter asymmetry comes from the contribution of the co…

hep-th20034 cited

Which is the best inflation model?

David H. Lyth

Reasonable-looking models of inflation are compared, taking into account the possibility that the curvature perturbation might originate from some "curvaton" field different from t…

hep-ph20022 cited

Generating the primordial curvature perturbation from inflation

David H. Lyth

The scale--independence of the primordial curvature perturbation suggests that it comes from the vacuum fluctuation during inflation of a light scalar field. This field may be the…

hep-ph2000

Observational constraints on models of inflation from the density perturbation and gravitino production

David H. Lyth

Present data require a spectral index $n\gsim 0.95$ at something like 1- level. If this lower bound survives it will constrain `new' and `modular' inflation models, while raisin…