Precision Cosmology with the CMB

Details Precision Cosmology with the CMB Precision Cosmology with the CMB

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aps..apr.j3002k&link_type=abstract

American Physical Society, April Meeting, 2004, May 1-4, 2004, Denver, Colorado April 2004, MEETING ID: APR04, abstract #J3.002

Physics

Scientific paper

I will cover what we have learned from WMAP and what we can expect to learn in about 2009 from Planck and on through 2016 from dedicated CMB polarization missions. These future missions are probes of Big Bang Inhomogenesis (BBI); i.e., the production of the initial departures from homogeneity that have led to all the structures we see in the Universe today. They will provide the most precise possible measurements of the scalar and tensor metric perturbations and can potentially determine the energy scale of inflation. Combined with cosmic shear observations, future CMB missions will be highly sensitive to the mass of relic neutrinos and the time evolution of the dark energy.

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