
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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Primordial non-Gaussianity, statistics of collapsed objects, and the ISW effect
Niayesh Afshordi University of Waterloo
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Optimal Non-Gaussian Estimators
Ue-Li Pen Canadian Institute for Theoretical Astrophysics (CITA)
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Primordial non-Gaussianity: Two "shapes" to look for
Kendrick Smith Perimeter Institute for Theoretical Physics
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Characterizing all possible primordial bispectrums from single field models
Xingang Chen University of Cambridge
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Analytic Form of Inflationary Actions and Non-Gaussianity
Daniel Chung University of Wisconsin–Madison
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Scale dependent non-Gaussianity
Sarah Shandera Pennsylvania State University
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Reconstruction of the primordial density PDF
Ravi Sheth University of Pennsylvania
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The effect of primordial non gaussianity on large scale structure
Licia Verde Institute of Space Sciences
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Imprints of primordial non-gaussianity on large-scale structure
Dragan Huterer University of Michigan–Ann Arbor
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Scale Dependent Non-Gaussianity in Large-Scale Structure
Marilena LoVerde University of Washington