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Jones, William Claude (2005-04-29) A Measurement of the temperature and polarization anisotropies of the cosmic microwave background radiation. http://resolver.caltech.edu/CaltechETD:etd-05102005-102535


Type of Document Dissertation
Author Jones, William Claude
URN etd-05102005-102535
Persistent URL http://resolver.caltech.edu/CaltechETD:etd-05102005-102535
Title A Measurement of the temperature and polarization anisotropies of the cosmic microwave background radiation
Degree PhD
Option Physics
Advisory Committee
Advisor Name Title
Andrew E. Lange Committee Chair
Marc Kamionkowski Committee Member
Sunil Golwala Committee Member
Tony Readhead Committee Member
Keywords
  • bolometers
  • optics
  • Cosmology
  • CMB
Date of Defense 2005-04-29
Availability unrestricted
Abstract
We describe the design and performance of the Boomerang experiment,

and report on measurements of the temperature and polarization

anisotropies of the Cosmic Microwave Background (CMB) obtained during

the January 2003 flight of Boomerang (B2K). To enable these studies, we have

developed a bolometric detector which is intrinsically sensitive to

linear polarization. The receiver consists of a pair of co-located

silicon nitride micromesh absorbers which couple anisotropically to

linearly polarized radiation through a corrugated waveguide

structure. This system allows simultaneous background limited

measurements of the Stokes I and Q parameters over ~30%

bandwidths at frequencies from ~60 to 400 GHz.

The science results reported here are derived from 195

hours of observation with four 145 GHz Polarization Sensitive

Bolometer (PSB) pairs. The data include 75 hours of observations

distributed over 1.8% of the sky with an additional 120 hours concentrated on the central portion of the field, itself representing

0.22% of the full sky. The B2K data improve significantly on existing

measurements of the CMB temperature power spectrum at angular scales of

500 < l < 1100. In addition we have measured a

spectrum of curl-free polarization anisotropies which, in the context of the

most simple adiabatic inflationary models, are consistent with the

predictions of the currently favored LCDM cosmology

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