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Prospects for Inflationary B-Mode DetectionMeasurements of the linear polarization of the cosmic microwave background provide a direct window into the physics of inflation. The experimental challenges are daunting: not only is the predicted signal faint compared to the photon noise limit, but it is hidden behind competing foregrounds from both local and cosmic sources. I will discuss the experimental response to these challenges and the prospects for eventual detection and characterization of the inflationary signal.
Document ID
20110020767
Acquisition Source
Goddard Space Flight Center
Document Type
Abstract
Authors
Kogut, Alan J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 25, 2013
Publication Date
October 5, 2011
Subject Category
Astrophysics
Report/Patent Number
GSFC.ABS.5186.2011
Report Number: GSFC.ABS.5186.2011
Meeting Information
Meeting: Pre-Planckian Inflation
Location: Minneapolis, MN
Country: United States
Start Date: October 5, 2011
End Date: October 9, 2011
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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