Observation of Cosmic Microwave Background Polarization with BICEP

Background Imaging of Cosmic Extragalactic Polarization (BICEP) is a bolometric polarimeter that has been optimized to target the B-mode of the cosmic microwave background (CMB) polarization at degree angular scales, which is a sensitive probe of the energy scale of inflation. The instrument's...

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Bibliographic Details
Main Author: Chiang, Hsin Cynthia
Format: Thesis
Language:English
Published: California Institute of Technology 2009
Subjects:
bolometers
Physics
inflation
b-mode
cosmic microwave background
gravitational wave background
polarization
South Pole
South pole
Online Access:https://dx.doi.org/10.7907/ra1d-v074
https://resolver.caltech.edu/CaltechETD:etd-10052008-101916
Description
Summary:Background Imaging of Cosmic Extragalactic Polarization (BICEP) is a bolometric polarimeter that has been optimized to target the B-mode of the cosmic microwave background (CMB) polarization at degree angular scales, which is a sensitive probe of the energy scale of inflation. The instrument's focal plane comprises 49 pairs of polarization-sensitive bolometers operating at 100 and 150 GHz, and the 25-cm aperture refractive optics provide degree-scale resolution over a 17 degree instantaneous field of view. The compact design enables sufficient control of instrumental polarization systematics to attain a projected final sensitivity corresponding to a tensor-to-scalar ratio of 0.1. This thesis describes the design, performance, and preliminary science results from BICEP, which has been observing the CMB from the South Pole since January 2006. After the first two seasons of operation, the EE, TE, and TT power spectra are measured with high precision at 30 < ell < 300, and BB is consistent with zero. BICEP has also observed the Galactic plane, and polarized emission is mapped with high signal-to-noise.

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