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19942022
most citedEverything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)

918 citations · 10.5k across the 126 of their papers we have counts for

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Showing 2002Show all

11 papers · 1 filter

hep-th2002★ 10 cited

Trans-Planckian Dark Energy?

Martin Lemoine, Jerome Martin, Jean-Philippe Uzan

It has recently been proposed by Mersini et al. 01, Bastero-Gil and Mersini 02 that the dark energy could be attributed to the cosmological properties of a scalar field with a non-…

astro-ph2002★ 2 cited

Quintessence and the accelerating universe

Philippe Brax, Jerome Martin

Observations seem to indicate that our universe is presently accelerating due to the presence of dark energy. Quintessence represents a possible way to model the dark energy. In th…

astro-ph2002★ 120 cited

WKB approximation for inflationary cosmological perturbations

Jerome Martin, Dominik J. Schwarz

A new method for predicting inflationary cosmological perturbations, based on the Wentzel-Kramers-Brillouin (WKB) approximation, is presented. A general expression for the WKB scal…

astro-ph2002★ 1 cited

Non-vacuum initial states for the cosmological perturbations and the back-reaction problem of inflation

Alejandro Gangui, Jerome Martin, Mairi Sakellariadou

In the framework of Inflationary theory, the assumption that the quantum state of the perturbations is a non-vacuum state leads to a difficulty: non-vacuum initial states imply, in…

astro-ph2002★ 55 cited

Inflation and non--Gaussianity

Alejandro Gangui, Jerome Martin, Mairi Sakellariadou

We study non-Gaussian signatures on the cosmic microwave background (CMB) radiation predicted within inflationary models with non-vacuum initial states for cosmological perturbatio…

hep-th2002★ 45 cited

Comment on "Density perturbations in the ekpyrotic scenario"

Jerome Martin, Patrick Peter, Nelson Pinto-Neto +1

In the paper ``Density perturbations in the ekpyrotic scenario'', it is argued that the expected spectrum of primordial perturbations should be scale invariant in this scenario. He…