BICEP Array Detectors and Instrumentation at 30/40 GHz: Design, Performance, and Deployment to the South Pole for Constraining Primordial Gravitational Waves ...
The discovery of the Cosmic Microwave Background (CMB) in the 1960s has provided strong observational evidence for the Big Bang cosmological model to describe the origin and evolution of the universe. The theory of cosmic inflation was developed in the 1980s to account for the initial density pertur...
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ftdatacite:10.7907/srdx-w019 2023-06-11T04:03:37+02:00 BICEP Array Detectors and Instrumentation at 30/40 GHz: Design, Performance, and Deployment to the South Pole for Constraining Primordial Gravitational Waves ... Mohamed Soliman, Ahmed 2023 PDF https://dx.doi.org/10.7907/srdx-w019 https://resolver.caltech.edu/CaltechTHESIS:05232023-174453276 en eng California Institute of Technology No commercial reproduction, distribution, display or performance rights in this work are provided. Inflation detectors. cosmology cryogenic instrumentation Galactic Foregrounds, telescopes BICEP Array Big Bang CMB polarimeters Cosmic Microwave Background primordial gravitational waves Applied Physics Thesis Text thesis Dissertation 2023 ftdatacite https://doi.org/10.7907/srdx-w019 2023-06-01T12:13:17Z The discovery of the Cosmic Microwave Background (CMB) in the 1960s has provided strong observational evidence for the Big Bang cosmological model to describe the origin and evolution of the universe. The theory of cosmic inflation was developed in the 1980s to account for the initial density perturbations by a period of exponential expansion in the early Universe to solve the horizon, flatness and monopole problems. Many inflation models predict potentially detectable primordial gravitational-waves (PGWs) background that imprint a B-mode polarization pattern in the CMB. The amplitude of the inflationary B-mode polarization depends on the energy scale of inflation and is parameterized by the tensor-to-scalar ratio r. The detection of a B-mode pattern would open a new window to probe the energy scale at the beginning of time when the universe was a mere fraction of a second old after the Big Bang. The BICEP/Keck collaboration is building a series of experiments located at the Amundsen-Scott South Pole Station ... Thesis Amundsen-Scott South pole DataCite Metadata Store (German National Library of Science and Technology) Amundsen Scott South Pole Station ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen-Scott ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen-Scott South Pole Station ENVELOPE(139.273,139.273,-89.998,-89.998) South Pole |
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Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
English |
topic |
Inflation detectors. cosmology cryogenic instrumentation Galactic Foregrounds, telescopes BICEP Array Big Bang CMB polarimeters Cosmic Microwave Background primordial gravitational waves Applied Physics |
spellingShingle |
Inflation detectors. cosmology cryogenic instrumentation Galactic Foregrounds, telescopes BICEP Array Big Bang CMB polarimeters Cosmic Microwave Background primordial gravitational waves Applied Physics Mohamed Soliman, Ahmed BICEP Array Detectors and Instrumentation at 30/40 GHz: Design, Performance, and Deployment to the South Pole for Constraining Primordial Gravitational Waves ... |
topic_facet |
Inflation detectors. cosmology cryogenic instrumentation Galactic Foregrounds, telescopes BICEP Array Big Bang CMB polarimeters Cosmic Microwave Background primordial gravitational waves Applied Physics |
description |
The discovery of the Cosmic Microwave Background (CMB) in the 1960s has provided strong observational evidence for the Big Bang cosmological model to describe the origin and evolution of the universe. The theory of cosmic inflation was developed in the 1980s to account for the initial density perturbations by a period of exponential expansion in the early Universe to solve the horizon, flatness and monopole problems. Many inflation models predict potentially detectable primordial gravitational-waves (PGWs) background that imprint a B-mode polarization pattern in the CMB. The amplitude of the inflationary B-mode polarization depends on the energy scale of inflation and is parameterized by the tensor-to-scalar ratio r. The detection of a B-mode pattern would open a new window to probe the energy scale at the beginning of time when the universe was a mere fraction of a second old after the Big Bang. The BICEP/Keck collaboration is building a series of experiments located at the Amundsen-Scott South Pole Station ... |
format |
Thesis |
author |
Mohamed Soliman, Ahmed |
author_facet |
Mohamed Soliman, Ahmed |
author_sort |
Mohamed Soliman, Ahmed |
title |
BICEP Array Detectors and Instrumentation at 30/40 GHz: Design, Performance, and Deployment to the South Pole for Constraining Primordial Gravitational Waves ... |
title_short |
BICEP Array Detectors and Instrumentation at 30/40 GHz: Design, Performance, and Deployment to the South Pole for Constraining Primordial Gravitational Waves ... |
title_full |
BICEP Array Detectors and Instrumentation at 30/40 GHz: Design, Performance, and Deployment to the South Pole for Constraining Primordial Gravitational Waves ... |
title_fullStr |
BICEP Array Detectors and Instrumentation at 30/40 GHz: Design, Performance, and Deployment to the South Pole for Constraining Primordial Gravitational Waves ... |
title_full_unstemmed |
BICEP Array Detectors and Instrumentation at 30/40 GHz: Design, Performance, and Deployment to the South Pole for Constraining Primordial Gravitational Waves ... |
title_sort |
bicep array detectors and instrumentation at 30/40 ghz: design, performance, and deployment to the south pole for constraining primordial gravitational waves ... |
publisher |
California Institute of Technology |
publishDate |
2023 |
url |
https://dx.doi.org/10.7907/srdx-w019 https://resolver.caltech.edu/CaltechTHESIS:05232023-174453276 |
long_lat |
ENVELOPE(0.000,0.000,-90.000,-90.000) ENVELOPE(0.000,0.000,-90.000,-90.000) ENVELOPE(139.273,139.273,-89.998,-89.998) |
geographic |
Amundsen Scott South Pole Station Amundsen-Scott Amundsen-Scott South Pole Station South Pole |
geographic_facet |
Amundsen Scott South Pole Station Amundsen-Scott Amundsen-Scott South Pole Station South Pole |
genre |
Amundsen-Scott South pole |
genre_facet |
Amundsen-Scott South pole |
op_rights |
No commercial reproduction, distribution, display or performance rights in this work are provided. |
op_doi |
https://doi.org/10.7907/srdx-w019 |
_version_ |
1768380694382247936 |