activity
19942009
most citedCMBPol Mission Concept Study: Probing Inflation with CMB Polarization

303 citations · 2k across the 35 of their papers we have counts for

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16 papers · 1 filter

astro-ph200682 cited

The evolution of clusters in the CLEF cosmological simulation: X-ray structural and scaling properties

Scott T. Kay, Antonio C. da Silva, Nabila Aghanim +5

We present results from a study of the X-ray cluster population that forms within the CLEF cosmological hydrodynamics simulation, a large N-body/SPH simulation of the Lambda CDM co…

astro-ph200666 cited

Quintessence reconstructed: new constraints and tracker viability

Martin Sahlén, Andrew R Liddle, David Parkinson

We update and extend our previous work reconstructing the potential of a quintessence field from current observational data. We extend the cosmological dataset to include new super…

astro-ph2006101 cited

Intermediate inflation in light of the three-year WMAP observations

John D Barrow, Andrew R Liddle, Cédric Pahud

The three-year observations from the Wilkinson Microwave Anisotropy Probe have been hailed as giving the first clear indication of a spectral index n_s<1. We point out that the dat…

astro-ph2006101 cited

Present and future evidence for evolving dark energy

Andrew R Liddle, Pia Mukherjee, David Parkinson +1

We compute the Bayesian evidences for one- and two-parameter models of evolving dark energy, and compare them to the evidence for a cosmological constant, using current data from T…

astro-ph200671 cited

Nflation: non-gaussianity in the horizon-crossing approximation

Soo A. Kim, Andrew R. Liddle

We analyze the cosmic non-gaussianity produced in inflation models with multiple uncoupled fields with monomial potentials, such as Nflation. Using the horizon-crossing approximati…

astro-ph20065 cited

Cosmological model selection

Andrew R. Liddle, Pia Mukherjee, David Parkinson

Model selection aims to determine which theoretical models are most plausible given some data, without necessarily asking about the preferred values of the model parameters. A comm…