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19932026
most citedExponential potentials and cosmological scaling solutions

1.5k citations · 22.2k across the 177 of their papers we have counts for

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Showing 2014Show all

10 papers · 1 filter

astro-ph.CO2014★ 24 cited

Expected dipole asymmetry in CMB polarization

M. H. Namjoo, A. A. Abolhasani, H. Assadullahi +3

We explore the hemispherical asymmetry predicted in cosmic microwave background polarization when there is an asymmetry in temperature anisotropies due to primordial perturbations.…

astro-ph.CO2014★ 18 cited

CMB hemispherical asymmetry from non-linear isocurvature perturbations

Hooshyar Assadullahi, Hassan Firouzjahi, Mohammad Hossein Namjoo +1

We investigate whether non-adiabatic perturbations from inflation could produce an asymmetric distribution of temperature anisotropies on large angular scales in the cosmic microwa…

astro-ph.CO2014★ 70 cited

Generalised tensor fluctuations and inflation

Dario Cannone, Gianmassimo Tasinato, David Wands

Using an effective field theory approach to inflation, we examine novel properties of the spectrum of inflationary tensor fluctuations, that arise when breaking some of the symmetr…

astro-ph.CO2014★ 29 cited

Impact of polarisation on the intrinsic CMB bispectrum

Guido W. Pettinari, Christian Fidler, Robert Crittenden +3

We compute the bispectrum induced in the cosmic microwave background (CMB) temperature and polarisation by the evolution of the primordial density perturbations using the second-or…

astro-ph.CO2014★ 309 cited

Indications of a late-time interaction in the dark sector

Valentina Salvatelli, Najla Said, Marco Bruni +2

We show that a general late-time interaction between cold dark matter and vacuum energy is favoured by current cosmological datasets. We characterize the strength of the coupling b…

astro-ph.CO2014★ 36 cited

Einstein's signature in cosmological large-scale structure

Marco Bruni, Juan Carlos Hidalgo, David Wands

We show how the non-linearity of general relativity generates a characteristic non-Gaussian signal in cosmological large-scale structure that we calculate at all perturbative order…