Task Force on Cosmic Microwave Background Research
arXiv:astro-ph/0604101
Abstract
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.
This is the final report of the DoE/NASA/NSF interagency task force on CMB research chaired by Rai Weiss. 87 pages
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- A Microscopic Limit on Gravitational Waves from D-brane Inflation
- New Sources of Gravitational Waves during Inflation
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- Analytic approach to the CMB polarizations generated by relic gravitational waves
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- Detecting Relic Gravitational Waves by Pulsar Timing Arrays: Effects of Cosmic Phase Transitions and Relativistic Free-Streaming Gases
- Non-Gaussianity and large-scale structure in a two-field inflationary model
- The Quijote CMB Experiment
- Natural Inflation: the status after WMAP 3-year data
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- The Primordial Inflation Polarization Explorer (PIPER)
- A CubeSat for Calibrating Ground-Based and Sub-Orbital Millimeter-Wave Polarimeters (CalSat)
- Antenna-coupled TES Bolometer Arrays for BICEP2/Keck and SPIDER
- A Back-reaction Induced Lower Bound on the Tensor-to-Scalar Ratio
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- Statistical imprints of CMB B-type polarization leakage in an incomplete sky survey analysis
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- The CMB polarization: status and prospects
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