Task Force on Cosmic Microwave Background Research

Adrian Lee (Berkeley/LBNL); Andrew Lange (Caltech); Bruce Partridge (Haverford); Bruce Winstein (Chicago); chair); Gary Hinshaw (GSFC); James Bock (Caltech/JPL); John Ruhl (Case Western); Lyman Page (Princeton); Mark Devlin (Penn)

Task Force on Cosmic Microwave Background Research

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arxiv astro-ph/0604101 v1 pith:NNCCBA5I submitted 2006-04-05 astro-ph gr-qchep-th

Task Force on Cosmic Microwave Background Research

James Bock (Caltech/JPL) , Sarah Church (Stanford) , Mark Devlin (Penn) , Gary Hinshaw (GSFC) , Andrew Lange (Caltech) , Adrian Lee (Berkeley/LBNL) , Lyman Page (Princeton) , Bruce Partridge (Haverford)

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John Ruhl (Case Western) Max Tegmark (MIT) Peter Timbie (Wisconsin) Rainer Weiss (MIT chair) Bruce Winstein (Chicago) Matias Zaldarriaga (Harvard)

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One of the most spectacular scientific breakthroughs in past decades was using measurements of the fluctuations in the cosmic microwave background (CMB) to test precisely our understanding of the history and composition of the Universe. This report presents a roadmap for leading CMB research to its logical next step, using precision polarization measurements to learn about ultra-high-energy physics and the Big Bang itself.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz
astro-ph.GA 2026-05 unverdicted novelty 3.0

Comparison of Galactic magnetic field models to polarized synchrotron observations shows good agreement on angles but poor match on intensity, indicating local foreground structures must be incorporated.