activity
19962008
most citedA discriminating probe of gravity at cosmological scales

403 citations · 580 across the 9 of their papers we have counts for

collaborators
Showing 2008 · astro-phShow all

6 papers · 2 filters

astro-ph20086 cited

Backgrounds and Projected Limits from Dark Matter Direct Detection Experiments

Scott Dodelson

A simple formula is introduced which indicates the amount by which projections of dark matter direct detection experiments are expected to be degraded due to backgrounds.

astro-ph200815 cited

CMBPol Mission Concept Study: A Mission to Map our Origins

Daniel Baumann, Asantha Cooray, Scott Dodelson +7

Quantum mechanical metric fluctuations during an early inflationary phase of the universe leave a characteristic imprint in the polarization of the cosmic microwave background (CMB…

astro-ph2008303 cited

CMBPol Mission Concept Study: Probing Inflation with CMB Polarization

Daniel Baumann, Mark G. Jackson, Peter Adshead +56

We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measu…

astro-ph20085 cited

Weighing the spatial and temporal fluctuations of the dark universe

Pengjie Zhang, Rachel Bean, Michele Liguori +1

A generic prediction of the standard cosmology, based on general relativity (GR), dark matter and the cosmological constant (and more generally, smooth dark energy), is that, the t…

astro-ph200815 cited

Universal Weak Lensing Distortion of Cosmological Correlation Functions

Scott Dodelson, Fabian Schmidt, Alberto Vallinotto

Gravitational lensing affects observed cosmological correlation functions because observed images do not coincide with true source locations. We treat this universal effect in a ge…

astro-ph200819 cited

Weak Lensing Effects on the Galaxy Three-Point Correlation Function

Fabian Schmidt, Alberto Vallinotto, Emiliano Sefusatti +1

We study the corrections to the galaxy three-point correlation function (3PCF) induced by weak lensing magnification due to the matter distribution along the line of sight. We cons…