Physical Society Colloquium
Beyond the Standard Cosmological Model
Department of Physics & Astronomy University of Pennsylvania
Observational advances in cosmology have led to the emergence of a standard
model that explains the accelerated expansion of the universe and the
distribution and dynamics of galaxies. Cold dark matter and dark energy are
considered the leading components of the energy density of the universe.
Ideas that provide alternatives to the minimal standard model include the
possibility that gravity on large scales deviates from the predictions of
general relativity. I will describe how cosmological measurements are used to
pursue such new physics. I will show gravitational lensing results from the
Sloan Digital Sky Survey and the Dark Energy Survey. New methods to measure
the mass distributon cosmic voids and the shapes of galaxy halos can test
theories of gravity and dark matter. Lensing by large-scale structure from
galaxy surveys and the cosmic microwave background provides tests of both
dark energy and gravity.
Friday, February 12th 2016, 15:30
Ernest Rutherford Physics Building, Keys Auditorium (room 112)
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