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19962009
most citedThe cosmological gravitational wave background from primordial density perturbations

695 citations · 2.3k across the 22 of their papers we have counts for

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14 papers · 1 filter

hep-th200819 cited

Generalised perturbation equations in bouncing cosmologies

Antonio Cardoso, David Wands

We consider linear perturbation equations for long-wavelength scalar metric perturbations in generalised gravity, applicable to non-singular cosmological models including a bounce…

hep-th2007111 cited

Non-Gaussianities from ekpyrotic collapse with multiple fields

Kazuya Koyama, Shuntaro Mizuno, Filippo Vernizzi +1

We compute the non-Gaussianity of the curvature perturbation generated by ekpyrotic collapse with multiple fields. The transition from the multi-field scaling solution to a single-…

hep-th200772 cited

Diagrammatic approach to non-Gaussianity from inflation

Christian T. Byrnes, Kazuya Koyama, Misao Sasaki +1

We present Feynman type diagrams for calculating the n-point function of the primordial curvature perturbation in terms of scalar field perturbations during inflation. The diagrams…

hep-th200770 cited

Curvature perturbations from ekpyrotic collapse with multiple fields

Kazuya Koyama, Shuntaro Mizuno, David Wands

A scale-invariant spectrum of isocurvature perturbations is generated during collapse in the ekpyrotic scaling solution in models where multiple fields have steep negative exponent…

hep-th200617 cited

Coupled bulk and brane fields about a de Sitter brane

Antonio Cardoso, Kazuya Koyama, Andrew Mennim +2

We consider the evolution of a bulk scalar field in anti-de Sitter (AdS) spacetime linearly coupled to a scalar field on a de Sitter boundary brane. We present results of a spectra…

hep-th200610 cited

Low-energy effective theory for a Randall-Sundrum scenario with a moving bulk brane

Ludovica Cotta-Ramusino, David Wands

We derive the low-energy effective theory of gravity for a generalized Randall-Sundrum scenario, allowing for a third self-gravitating brane to live in the 5D bulk spacetime. At ze…