The BICEP1 and BICEP2 telescopes studied the temperature and polarization of the Cosmic Microwave Background (CMB) from 2006 – 2008 and 2010 – 2012, respectively, producing the deepest maps of polarization created to date. From BICEP2 three-year data, we detect B-mode polarization at the degree-scale above the expectation from lensed-ΛCDM to greater than 5σ significance, consistent with that expected from gravitational waves created during Inflation. Instrumental systematic effects have been characterized and ruled out, and galactic foreground contamination is disfavored by the data.
Additionally, correlations between temperature and B-mode polarization and between E-mode and B-mode polarization show evidence of polarization rotation of –1° to 5σ significance; however, adding systematic uncertainty reduces this significance to ∼ 2σ. These measurements, combined with other CMB and astrophysical measurements, point to possible parity violating physics like cosmic birefringence, but more precise calibration techniques are required to break the degeneracy between cosmic polarization rotation and systematic effects. Improved calibration is possible with current generation technology and may be achieved within the next few years.
In this work, I present experimental and analysis techniques employed for BICEP1 and BICEP2 to measure B-mode polarization and temperature and polarization correlations, as well as the scientific motivation, results, and a path forward for future measurements.
|Commitee:||Greist, Kim, Paar, Hans, Rebeiz, Gabriel, Thiemens, Mark|
|School:||University of California, San Diego|
|School Location:||United States -- California|
|Source:||DAI-B 75/10(E), Dissertation Abstracts International|
|Keywords:||B-modes, Birefringence, Cosmic microwave background, Cosmology, Gravitational waves, Inflation|
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