Physical Society Colloquium
The Cosmic Microwave Background and Neutrinos
Department of Physics Princeton University
The remarkably simple standard model of cosmology has passed many tests
and its basic parameters have been well constrained. A new generation of
measurements now uses the CMB along with other cosmic probes such as galaxy
surveys to interrogate the volume of the universe between us and the surface
of last scattering to push beyond the standard model. We can, for example,
use the CMB to address such questions as “What is the sum of the
neutrino masses?” and “How many relativistic species
of particles were there in the early universe?” We review the
status of observations and present what we might hope to learn in the next
half decade of observations.
Friday, February 23rd 2018, 15:30
Ernest Rutherford Physics Building, Keys Auditorium (room 112)
|