The Next Generation Cosmic Microwave Background Measurements and What We Hope to Learn About the Early Universe

Details The Next Generation Cosmic Microwave Background Measurements and What We Hope to Learn About the Early Universe The Next Generation Cosmic Microwave Background Measurements and What We Hope to Learn About the Early Universe

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998kcs..confe..12l&link_type=abstract

Presented at the KITP: Colloquium Series, Mar 4, 1998, Kavli Institute for Theoretical Physics, University of California, Santa

Physics

Scientific paper

The next generation of CMB measurements promises to greatlyincrease ourknowledge of the CMB angular power spectrum. This should enable us todetermine many of the cosmological parameters that define our universe suchas the overall mass and baryon density, if there is a significant vacuumenergy component, the Hubble parameter, spectral tilt and reionizationhistory, among others. Whether nature is kind to us or whether foregroundcontamination and systematics prevent the full realization of these goalsremains to be seen.

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