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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Main Author: Mohamed Soliman, Ahmed
Format: Thesis
Language:English
Published: California Institute of Technology 2023
Subjects:
Online Access:https://dx.doi.org/10.7907/srdx-w019
https://resolver.caltech.edu/CaltechTHESIS:05232023-174453276
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spelling 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
institution 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
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