Physical Society Colloquium
Looking for cracks in the cosmological model
Department of Physics and Department of Astrophysical
Sciences Princeton University
Recent observations of the cosmic microwave background are allowing us to
scrutinize the ‘Lambda - Cold Dark Matter’ cosmological model, and to
weigh in on possible cracks in this model that may be appearing from
different astronomical observations. I will describe recent results from the
Atacama Cosmology Telescope, and show how the relic CMB light can be used as
a backlight to weigh cosmic structures, and to map out the dark matter and
cosmic gas over half the sky. I will also describe prospects for an improved
view of the physics of the early universe from these data, and from the
upcoming Simons Observatory.
Friday, March 1st 2024, 15:30
Ernest Rutherford Physics Building, Keys Auditorium (room 112)
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