The coupling of baryons and photons by Thomson scattering in the early universe leads to a rich structure in the power spectra of the cosmic microwave background photons and the matter. The study of the former has revolutionized cosmology and allowed precise measurement of a host of important cosmological parameters. The study of the latter is still in its infancy, but holds the potential to constrain the nature of the dark energy believed to be causing the accelerated expansion of the universe. I will discuss how we can measure this cosmic sound, and the theoretical developments that need to be made before we can realize the promise of future experiments.

--------------------------------------------------------------------------------------
For more information, contact:

Adil Hassam
hassam@umd.edu
301-405- 1417

Arthur LaPorta
alaporta@umd.edu
301-405-3291