activity
19922026
most citedBig-Bang nucleosynthesis (Particle Data Group mini-review)

4.1k citations · 31.4k across the 275 of their papers we have counts for

collaborators
Showing 2009 · astro-ph.COShow all

7 papers · 2 filters

astro-ph.CO2009★ 56 cited

Unified dark energy and dark matter from a scalar field different from quintessence

Changjun Gao, Martin Kunz, Andrew R Liddle +1

We explore unification of dark matter and dark energy in a theory containing a scalar field of non-Lagrangian type, obtained by direct insertion of a kinetic term into the energy-m…

astro-ph.CO2009★ 41 cited

Constraining the dark fluid

Martin Kunz, Andrew R Liddle, David Parkinson +1

Cosmological observations are normally fit under the assumption that the dark sector can be decomposed into dark matter and dark energy components. However, as long as the probes r…

astro-ph.CO2009★ 33 cited

An Evolutionary Paradigm for Dusty Active Galaxies at Low Redshift

D. Farrah, B. Connolly, N. Connolly +7

We apply methods from Bayesian inferencing and graph theory to a dataset of 102 mid-infrared spectra, and archival data from the optical to the millimeter, to construct an evolutio…

astro-ph.CO2009★ 24 cited

Optimizing baryon acoustic oscillation surveys II: curvature, redshifts, and external datasets

David Parkinson, Martin Kunz, Andrew R. Liddle +3

We extend our study of the optimization of large baryon acoustic oscillation (BAO) surveys to return the best constraints on the dark energy, building on Paper I of this series (Pa…

astro-ph.CO2009★ 12 cited

Viable inflationary models ending with a first-order phase transition

Marina Cortês, Andrew R. Liddle

We investigate the parameter space of hybrid inflation models where inflation terminates via a first-order phase transition causing nucleation of bubbles. Such models experience a…

astro-ph.CO2009★ 164 cited

Early assembly of the most massive galaxies

Chris A. Collins, John P. Stott, Matt Hilton +15

The current consensus is that galaxies begin as small density fluctuations in the early Universe and grow by in situ star formation and hierarchical merging. Stars begin to form re…

astro-ph.CO2009★ 4 cited

Observing the Evolution of the Universe

James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…