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20002026
most citedCosmology with the Laser Interferometer Space Antenna

359 citations · 2.7k across the 60 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 31 cited

On the degeneracy between primordial tensor modes and cosmic strings in future CMB data from Planck

Jon Urrestilla, Pia Mukherjee, Andrew R. Liddle +3

While observations indicate that the predominant source of cosmic inhomogeneities are adiabatic perturbations, there are a variety of candidates to provide auxiliary trace effects,…

astro-ph2007★ 58 cited

Cosmic microwave anisotropies from BPS semilocal strings

Jon Urrestilla, Neil Bevis, Mark Hindmarsh +2

We present the first ever calculation of cosmic microwave background CMB anisotropy power spectra from semilocal cosmic strings, obtained via simulations of a classical field theor…

astro-ph2007★ 87 cited

CMB polarization power spectra contributions from a network of cosmic strings

Neil Bevis, Mark Hindmarsh, Martin Kunz +1

We present the first calculation of the possible (local) cosmic string contribution to the cosmic microwave background polarization spectra from simulations of a string network (ra…

astro-ph2007★ 195 cited

Fitting CMB data with cosmic strings and inflation

Neil Bevis, Mark Hindmarsh, Martin Kunz +1

We perform a multiparameter likelihood analysis to compare measurements of the cosmic microwave background (CMB) power spectra with predictions from models involving cosmic strings…

astro-ph2006★ 202 cited

CMB power spectrum contribution from cosmic strings using field-evolution simulations of the Abelian Higgs model

Neil Bevis, Mark Hindmarsh, Martin Kunz +1

We present the first field-theoretic calculations of the contribution made by cosmic strings to the temperature power spectrum of the cosmic microwave background (CMB). Unlike prev…

astro-ph2005★ 28 cited

Semilocal Cosmic String Networks

A. Achucarro, P. Salmi, J. Urrestilla

We report on a large scale numerical study of networks of semilocal cosmic strings in flat space in the parameter regime in which they are perturbatively stable. We find a populati…