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Four direct measurements of the fine-structure constant 13 billion years ago
Observations of the redshift z = 7.085 quasar J1120+0641 are used to search for variations of the fine structure constant, α, over the redshift range 5:5 to 7:1. Observations at z = 7:1 probe the physics of the universe at only 0.8 billion years old. These are the most distant direct measurements of...
Autores principales: | , , , , , , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
American Association for the Advancement of Science
2020
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7182409/ https://www.ncbi.nlm.nih.gov/pubmed/32917582 http://dx.doi.org/10.1126/sciadv.aay9672 |
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author | Wilczynska, Michael R. Webb, John K. Bainbridge, Matthew Barrow, John D. Bosman, Sarah E. I. Carswell, Robert F. Dąbrowski, Mariusz P. Dumont, Vincent Lee, Chung-Chi Leite, Ana Catarina Leszczyńska, Katarzyna Liske, Jochen Marosek, Konrad Martins, Carlos J. A. P. Milaković, Dinko Molaro, Paolo Pasquini, Luca |
author_facet | Wilczynska, Michael R. Webb, John K. Bainbridge, Matthew Barrow, John D. Bosman, Sarah E. I. Carswell, Robert F. Dąbrowski, Mariusz P. Dumont, Vincent Lee, Chung-Chi Leite, Ana Catarina Leszczyńska, Katarzyna Liske, Jochen Marosek, Konrad Martins, Carlos J. A. P. Milaković, Dinko Molaro, Paolo Pasquini, Luca |
author_sort | Wilczynska, Michael R. |
collection | PubMed |
description | Observations of the redshift z = 7.085 quasar J1120+0641 are used to search for variations of the fine structure constant, α, over the redshift range 5:5 to 7:1. Observations at z = 7:1 probe the physics of the universe at only 0.8 billion years old. These are the most distant direct measurements of α to date and the first measurements using a near-IR spectrograph. A new AI analysis method is employed. Four measurements from the x-shooter spectrograph on the Very Large Telescope (VLT) constrain changes in a relative to the terrestrial value (α(0)). The weighted mean electromagnetic force in this location in the universe deviates from the terrestrial value by Δα/α = (α(z) − α(0))/α(0) = (−2:18 ± 7:27) × 10(−5), consistent with no temporal change. Combining these measurements with existing data, we find a spatial variation is preferred over a no-variation model at the 3:9σ level. |
format | Online Article Text |
id | pubmed-7182409 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2020 |
publisher | American Association for the Advancement of Science |
record_format | MEDLINE/PubMed |
spelling | pubmed-71824092020-05-18 Four direct measurements of the fine-structure constant 13 billion years ago Wilczynska, Michael R. Webb, John K. Bainbridge, Matthew Barrow, John D. Bosman, Sarah E. I. Carswell, Robert F. Dąbrowski, Mariusz P. Dumont, Vincent Lee, Chung-Chi Leite, Ana Catarina Leszczyńska, Katarzyna Liske, Jochen Marosek, Konrad Martins, Carlos J. A. P. Milaković, Dinko Molaro, Paolo Pasquini, Luca Sci Adv Research Articles Observations of the redshift z = 7.085 quasar J1120+0641 are used to search for variations of the fine structure constant, α, over the redshift range 5:5 to 7:1. Observations at z = 7:1 probe the physics of the universe at only 0.8 billion years old. These are the most distant direct measurements of α to date and the first measurements using a near-IR spectrograph. A new AI analysis method is employed. Four measurements from the x-shooter spectrograph on the Very Large Telescope (VLT) constrain changes in a relative to the terrestrial value (α(0)). The weighted mean electromagnetic force in this location in the universe deviates from the terrestrial value by Δα/α = (α(z) − α(0))/α(0) = (−2:18 ± 7:27) × 10(−5), consistent with no temporal change. Combining these measurements with existing data, we find a spatial variation is preferred over a no-variation model at the 3:9σ level. American Association for the Advancement of Science 2020-04-24 /pmc/articles/PMC7182409/ /pubmed/32917582 http://dx.doi.org/10.1126/sciadv.aay9672 Text en Copyright © 2020 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC). http://creativecommons.org/licenses/by-nc/4.0/ This is an open-access article distributed under the terms of the Creative Commons Attribution-NonCommercial license (http://creativecommons.org/licenses/by-nc/4.0/) , which permits use, distribution, and reproduction in any medium, so long as the resultant use is not for commercial advantage and provided the original work is properly cited. |
spellingShingle | Research Articles Wilczynska, Michael R. Webb, John K. Bainbridge, Matthew Barrow, John D. Bosman, Sarah E. I. Carswell, Robert F. Dąbrowski, Mariusz P. Dumont, Vincent Lee, Chung-Chi Leite, Ana Catarina Leszczyńska, Katarzyna Liske, Jochen Marosek, Konrad Martins, Carlos J. A. P. Milaković, Dinko Molaro, Paolo Pasquini, Luca Four direct measurements of the fine-structure constant 13 billion years ago |
title | Four direct measurements of the fine-structure constant 13 billion years ago |
title_full | Four direct measurements of the fine-structure constant 13 billion years ago |
title_fullStr | Four direct measurements of the fine-structure constant 13 billion years ago |
title_full_unstemmed | Four direct measurements of the fine-structure constant 13 billion years ago |
title_short | Four direct measurements of the fine-structure constant 13 billion years ago |
title_sort | four direct measurements of the fine-structure constant 13 billion years ago |
topic | Research Articles |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7182409/ https://www.ncbi.nlm.nih.gov/pubmed/32917582 http://dx.doi.org/10.1126/sciadv.aay9672 |
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