Cargando…

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...

Descripción completa

Detalles Bibliográficos
Autores principales: 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
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2020
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
_version_ 1783526234395770880
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
work_keys_str_mv AT wilczynskamichaelr fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT webbjohnk fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT bainbridgematthew fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT barrowjohnd fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT bosmansarahei fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT carswellrobertf fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT dabrowskimariuszp fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT dumontvincent fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT leechungchi fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT leiteanacatarina fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT leszczynskakatarzyna fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT liskejochen fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT marosekkonrad fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT martinscarlosjap fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT milakovicdinko fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT molaropaolo fourdirectmeasurementsofthefinestructureconstant13billionyearsago
AT pasquiniluca fourdirectmeasurementsofthefinestructureconstant13billionyearsago