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20002026
most citedPlanck 2013 results. XXV. Searches for cosmic strings and other topological defects

346 citations · 4.2k across the 73 of their papers we have counts for

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astro-ph2008★ 44 cited

Constraints on Kinetically Modified Inflation from WMAP5

Larissa Lorenz, Jerome Martin, Christophe Ringeval

Single field inflationary models with a non-minimal kinetic term (also called k-inflationary models) can be characterised by the so-called sound flow functions, which complete the…

astro-ph2008★ 61 cited

K-inflationary Power Spectra in the Uniform Approximation

Larissa Lorenz, Jerome Martin, Christophe Ringeval

The advent of explicit Dirac-Born-Infeld (DBI) inflationary models within string theory has drawn renewed interest to the cosmological role of unusual scalar field dynamics, usuall…

astro-ph2007★ 114 cited

Small-Angle CMB Temperature Anisotropies Induced by Cosmic Strings

Aurélien A. Fraisse, Christophe Ringeval, David N. Spergel +1

We use Nambu-Goto numerical simulations to compute the cosmic microwave background (CMB) temperature anisotropies induced at arcminute angular scales by a network of cosmic strings…

astro-ph2007★ 65 cited

The exact numerical treatment of inflationary models

Christophe Ringeval

The precision reached by the recent CMB measurements gives new insights into the shape of the primordial power spectra of the cosmological perturbations. In the context of inflatio…

astro-ph2006★ 245 cited

Inflation after WMAP3: Confronting the Slow-Roll and Exact Power Spectra with CMB Data

Jerome Martin, Christophe Ringeval

The implications of the WMAP (Wilkinson Microwave Anisotropy Probe) third year data for inflation are investigated using both the slow-roll approximation and an exact numerical int…

astro-ph2005★ 293 cited

Cosmological evolution of cosmic string loops

Christophe Ringeval, Mairi Sakellariadou, Francois Bouchet

The existence of a scaling evolution for cosmic string loops in an expanding universe is demonstrated for the first time by means of numerical simulations. In contrast with what is…