Constraining the inflationary universe from the South Pole ...
The standard model of cosmology (ΛCDM ) is able to statistically describe the observable Universe with a small set of parameters that have been mea- sured to a percent level precision through observations of the Cosmic Mi- crowave Background (CMB) [Aghanim et al. 2020]. While this model shows a rema...
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ftdatacite:10.14288/1.0427409 2024-04-28T08:38:49+00:00 Constraining the inflationary universe from the South Pole ... Fatigoni, Sofia 2023 https://dx.doi.org/10.14288/1.0427409 https://doi.library.ubc.ca/10.14288/1.0427409 en eng University of British Columbia article-journal Text ScholarlyArticle 2023 ftdatacite https://doi.org/10.14288/1.0427409 2024-04-02T09:31:21Z The standard model of cosmology (ΛCDM ) is able to statistically describe the observable Universe with a small set of parameters that have been mea- sured to a percent level precision through observations of the Cosmic Mi- crowave Background (CMB) [Aghanim et al. 2020]. While this model shows a remarkable agreement with the data, it still can’t explain all the features we observe in the CMB. One of the biggest mysteries resides on the fact that CMB radiation sky is extremely uniform in temperature, despite that it was generated when the Universe was so young that just small patches of sky could be in causal contact. As an add on to the Standard Cosmological Model the theory of inflation [Guth 1981] was introduced, to solve this set of puzzles. One prediction from Inflation is the presence of a background of gravitational waves, in the primordial Universe, that would have produced a unique parity-odd pattern in the polarization of the CMB, also known as B-Modes. Until now no CMB experiment was able to find ... Text South pole DataCite Metadata Store (German National Library of Science and Technology) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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description |
The standard model of cosmology (ΛCDM ) is able to statistically describe the observable Universe with a small set of parameters that have been mea- sured to a percent level precision through observations of the Cosmic Mi- crowave Background (CMB) [Aghanim et al. 2020]. While this model shows a remarkable agreement with the data, it still can’t explain all the features we observe in the CMB. One of the biggest mysteries resides on the fact that CMB radiation sky is extremely uniform in temperature, despite that it was generated when the Universe was so young that just small patches of sky could be in causal contact. As an add on to the Standard Cosmological Model the theory of inflation [Guth 1981] was introduced, to solve this set of puzzles. One prediction from Inflation is the presence of a background of gravitational waves, in the primordial Universe, that would have produced a unique parity-odd pattern in the polarization of the CMB, also known as B-Modes. Until now no CMB experiment was able to find ... |
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Text |
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Fatigoni, Sofia |
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Fatigoni, Sofia Constraining the inflationary universe from the South Pole ... |
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Fatigoni, Sofia |
author_sort |
Fatigoni, Sofia |
title |
Constraining the inflationary universe from the South Pole ... |
title_short |
Constraining the inflationary universe from the South Pole ... |
title_full |
Constraining the inflationary universe from the South Pole ... |
title_fullStr |
Constraining the inflationary universe from the South Pole ... |
title_full_unstemmed |
Constraining the inflationary universe from the South Pole ... |
title_sort |
constraining the inflationary universe from the south pole ... |
publisher |
University of British Columbia |
publishDate |
2023 |
url |
https://dx.doi.org/10.14288/1.0427409 https://doi.library.ubc.ca/10.14288/1.0427409 |
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South pole |
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South pole |
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https://doi.org/10.14288/1.0427409 |
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