Cosmologists at Perimeter Institute seek to help pin down the constituents and history of our universe, and the rules governing its origin and evolution. Many of the most interesting clues about physics beyond the standard model (e.g., dark matter, dark energy, the matter/anti-matter asymmetry, and the spectrum of primordial density perturbations], come from cosmological observations, and cosmological observations are often the best way to test or constrain a proposed modification of the laws of nature, since such observations can probe length scales, time scales, and energy scales that are beyond the reach of terrestrial laboratories.
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Format results
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Institute of Space Sciences
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Imprints of primordial non-gaussianity on large-scale structure
University of Michigan–Ann Arbor -
Scale Dependent Non-Gaussianity in Large-Scale Structure
University of Washington -
Primordial Non-Gaussianities in Kahler Moduli Inflation
Queen's University -
Probing local non--Gaussianities in CMB within a Bayesian framework
Max Planck Institute for Astrophysics Munich Germany -
Secondary Anistropy Contributions to the Bispectrum
University of California, Irvine -
Point Source Contamination of f_NL Estimators
California Institute of Technology -
WMAP 5-year Results: Measurement of f_NL
Max-Planck-Institut für Astrophysik (MPA), Garching -
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Aspects of Hagedorn Holography
Hebrew University of Jerusalem -
Gauge Theory Duals of Cosmological Singularities
University of Kentucky -