Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole
The question of how exactly the universe began is the motivation for this work. Based on the discoveries of the cosmic expansion and of the cosmic microwave background (CMB) radiation, humans have learned of the Big Bang origin of the universe. However, what exactly happened in the first moments of...
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ftcdlib:qt6b98h32b 2023-05-15T13:57:18+02:00 Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole Takahashi, Yuki David 105 2010-01-01 application/pdf http://www.escholarship.org/uc/item/6b98h32b http://n2t.net/ark:/13030/m5125xnz en eng eScholarship, University of California http://www.escholarship.org/uc/item/6b98h32b qt6b98h32b http://n2t.net/ark:/13030/m5125xnz public Takahashi, Yuki David. (2010). Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole. UC Berkeley: Physics. Retrieved from: http://www.escholarship.org/uc/item/6b98h32b Astrophysics Physics Antarctica calibration CMB cosmology inflation telescope dissertation 2010 ftcdlib 2016-09-23T22:54:54Z The question of how exactly the universe began is the motivation for this work. Based on the discoveries of the cosmic expansion and of the cosmic microwave background (CMB) radiation, humans have learned of the Big Bang origin of the universe. However, what exactly happened in the first moments of the Big Bang? A scenario of initial exponential expansion called "inflation" was proposed in the 1980s, explaining several important mysteries about the universe. Inflation would have generated gravitational waves that would have left a unique imprint in the polarization of the CMB. To search for this evidence for inflation, a team gathered in 2002 to design a telescope experiment called BICEP. Sited at the South Pole, BICEP was a novel 25-cm aperture refractor with 49 pairs of polarization-sensitive bolometers. We completed 3 years of successful observations from February 2006 to December 2008. To constrain the amplitude of polarization resulting from inflation, expected to be at least 7 orders of magnitude fainter than the 3 K CMB intensity, precise control of systematic effects is essential. A crucial challenge is preventing systematic errors from introducing false polarization anisotropy signal at the level corresponding to ~0.1 μK in amplitude. One main focus of this thesis is the characterization of systematic effects for BICEP. We developed a simulation framework for propagating instrumental systematic effects to the final polarization results. Based on these simulations, we established benchmarks for the characterization of critical instrumental properties including bolometer relative gains, beam mismatch, polarization orientation, telescope pointing, sidelobes, thermal stability, and timestream noise model. Guided by these benchmarks, we carefully measured these properties and have shown that we have characterized the instrument adequately to ensure that systematic errors do not limit BICEP's current cosmology results. We have analyzed the first 2 years of data, lowering the upper limits on the gravitational-wave induced polarization by an order of magnitude over all previous experiments. The systematic error analysis has identified what future refinements are likely necessary to probe CMB polarization down to levels corresponding to inflationary energy scales below 2 × 10 16 GeV. Doctoral or Postdoctoral Thesis Antarc* Antarctica South pole South pole University of California: eScholarship South Pole |
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University of California: eScholarship |
op_collection_id |
ftcdlib |
language |
English |
topic |
Astrophysics Physics Antarctica calibration CMB cosmology inflation telescope |
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Astrophysics Physics Antarctica calibration CMB cosmology inflation telescope Takahashi, Yuki David Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole |
topic_facet |
Astrophysics Physics Antarctica calibration CMB cosmology inflation telescope |
description |
The question of how exactly the universe began is the motivation for this work. Based on the discoveries of the cosmic expansion and of the cosmic microwave background (CMB) radiation, humans have learned of the Big Bang origin of the universe. However, what exactly happened in the first moments of the Big Bang? A scenario of initial exponential expansion called "inflation" was proposed in the 1980s, explaining several important mysteries about the universe. Inflation would have generated gravitational waves that would have left a unique imprint in the polarization of the CMB. To search for this evidence for inflation, a team gathered in 2002 to design a telescope experiment called BICEP. Sited at the South Pole, BICEP was a novel 25-cm aperture refractor with 49 pairs of polarization-sensitive bolometers. We completed 3 years of successful observations from February 2006 to December 2008. To constrain the amplitude of polarization resulting from inflation, expected to be at least 7 orders of magnitude fainter than the 3 K CMB intensity, precise control of systematic effects is essential. A crucial challenge is preventing systematic errors from introducing false polarization anisotropy signal at the level corresponding to ~0.1 μK in amplitude. One main focus of this thesis is the characterization of systematic effects for BICEP. We developed a simulation framework for propagating instrumental systematic effects to the final polarization results. Based on these simulations, we established benchmarks for the characterization of critical instrumental properties including bolometer relative gains, beam mismatch, polarization orientation, telescope pointing, sidelobes, thermal stability, and timestream noise model. Guided by these benchmarks, we carefully measured these properties and have shown that we have characterized the instrument adequately to ensure that systematic errors do not limit BICEP's current cosmology results. We have analyzed the first 2 years of data, lowering the upper limits on the gravitational-wave induced polarization by an order of magnitude over all previous experiments. The systematic error analysis has identified what future refinements are likely necessary to probe CMB polarization down to levels corresponding to inflationary energy scales below 2 × 10 16 GeV. |
format |
Doctoral or Postdoctoral Thesis |
author |
Takahashi, Yuki David |
author_facet |
Takahashi, Yuki David |
author_sort |
Takahashi, Yuki David |
title |
Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole |
title_short |
Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole |
title_full |
Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole |
title_fullStr |
Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole |
title_full_unstemmed |
Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole |
title_sort |
measurement of the cosmic microwave background polarization with the bicep telescope at the south pole |
publisher |
eScholarship, University of California |
publishDate |
2010 |
url |
http://www.escholarship.org/uc/item/6b98h32b http://n2t.net/ark:/13030/m5125xnz |
op_coverage |
105 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
Antarc* Antarctica South pole South pole |
genre_facet |
Antarc* Antarctica South pole South pole |
op_source |
Takahashi, Yuki David. (2010). Measurement of the Cosmic Microwave Background Polarization with the BICEP Telescope at the South Pole. UC Berkeley: Physics. Retrieved from: http://www.escholarship.org/uc/item/6b98h32b |
op_relation |
http://www.escholarship.org/uc/item/6b98h32b qt6b98h32b http://n2t.net/ark:/13030/m5125xnz |
op_rights |
public |
_version_ |
1766264893681434624 |