Fundamental physics with ESPRESSO

Detalhes bibliográficos
Autor(a) principal: da Fonseca, Vítor
Data de Publicação: 2022
Outros Autores: Barreiro, Tiago, Nunes, Nelson J., Cristiani, Stefano, Cupani, Guido, D'Odorico, Valentina, Leite, Ana C. O., Marques, Catarina M. J., Martins, Carlos J. A. P., Milaković, Dinko, Molaro, Paolo, Murphy, Michael T., Schmidt, Tobias M., Abreu, Manuel, Adibekyan, Vardan, Cabral, Alexandre, Di Marcantonio, Paolo, González Hernández, Jonay I., Palle, Enric, Pepe, Francesco A., Rebolo, Rafael, Santos, Nuno C., Sousa, Sérgio G., Sozzetti, Alessandro, Mascareño, Alejandro Suárez, Osorio, Maria Rosa Zapatero
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10362/150645
Resumo: This work was financed by FEDER–Fundo Europeu de Desenvolvimento Regional funds through the COMPETE 2020–Operational Programme for Competitiveness and Internationalisation (POCI), and by Portuguese funds through FCT – Fundação para a Ciência e a Tecnologia under projects POCI-01-0145-FEDER-028987. MTM acknowledges the support of the Australian Research Council through Future Fellowship grant FT180100194. The INAF authors acknowledge financial support of the Italian Ministry of Education, University, and Research with PRIN 201278X4FL and the “Progetti Premiali” funding scheme. TMS also acknowledges the support from the Swiss National Science Foundation (SNSF) and the University of Geneva. M-RZO acknowledges funding under project PID2019-109522GB-C51 of the Spanish Ministerio de Ciencia e Investigación. ASM and JIGH acknowledge financial support from the Spanish Ministry of Science and Innovation (MICIN) project PID2020-117493GB-I00. ASM also acknowledges financial support from the Spanish Ministry of Science and Innovation (MICINN) under 2018 Juan de la Cierva program IJC2018-035229-I, as well as from the Government of the Canary Islands project ProID2020010129. Publisher Copyright: ©
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spelling Fundamental physics with ESPRESSOConstraining a simple parametrisation for varyingDark energyAstronomy and AstrophysicsSpace and Planetary ScienceThis work was financed by FEDER–Fundo Europeu de Desenvolvimento Regional funds through the COMPETE 2020–Operational Programme for Competitiveness and Internationalisation (POCI), and by Portuguese funds through FCT – Fundação para a Ciência e a Tecnologia under projects POCI-01-0145-FEDER-028987. MTM acknowledges the support of the Australian Research Council through Future Fellowship grant FT180100194. The INAF authors acknowledge financial support of the Italian Ministry of Education, University, and Research with PRIN 201278X4FL and the “Progetti Premiali” funding scheme. TMS also acknowledges the support from the Swiss National Science Foundation (SNSF) and the University of Geneva. M-RZO acknowledges funding under project PID2019-109522GB-C51 of the Spanish Ministerio de Ciencia e Investigación. ASM and JIGH acknowledge financial support from the Spanish Ministry of Science and Innovation (MICIN) project PID2020-117493GB-I00. ASM also acknowledges financial support from the Spanish Ministry of Science and Innovation (MICINN) under 2018 Juan de la Cierva program IJC2018-035229-I, as well as from the Government of the Canary Islands project ProID2020010129. Publisher Copyright: ©Context. The spectrograph ESPRESSO recently obtained a limit on the variation of the fine-structure constant, α, through measurements along the line of sight of a bright quasar with a precision of 1.36 ppm at 1σ level. This imposes new constraints on cosmological models with a varying α. We assume such a model where the electromagnetic sector is coupled to a scalar field dark energy responsible for the current acceleration of the Universe. We parametrise the variation of α with two extra parameters, one defining the cosmological evolution of the quintessence component and the other fixing the coupling with the electromagnetic field. Aims. The objective of this work is to constrain these parameters with both astrophysical and local probes. We also carried out a comparative analysis of how each data probe may constrain our parametrisation. Methods. We performed a Bayesian analysis by comparing the predictions of the model with observations. The astrophysical datasets are composed of quasar spectra measurements, including the latest ESPRESSO data point, as well as Planck observations of the cosmic microwave background. We combined these with local results from atomic clocks and the MICROSCOPE experiment. Results. The constraints placed on the quintessence parameter are consistent with a null variation of the field, and are therefore compatible with a δ CDM cosmology. The constraints on the coupling to the electromagnetic sector are dominated by the Eötvös parameter local bound. Conclusions. More precise measurements with ESPRESSO will be extremely important to study the cosmological evolution of α as it probes an interval of redshift not accessible to other types of observations. However, for this particular model, current available data favour a null variation of α resulting mostly from the strong MICROSCOPE limits.DF – Departamento de FísicaRUNda Fonseca, VítorBarreiro, TiagoNunes, Nelson J.Cristiani, StefanoCupani, GuidoD'Odorico, ValentinaLeite, Ana C. O.Marques, Catarina M. J.Martins, Carlos J. A. P.Milaković, DinkoMolaro, PaoloMurphy, Michael T.Schmidt, Tobias M.Abreu, ManuelAdibekyan, VardanCabral, AlexandreDi Marcantonio, PaoloGonzález Hernández, Jonay I.Palle, EnricPepe, Francesco A.Rebolo, RafaelSantos, Nuno C.Sousa, Sérgio G.Sozzetti, AlessandroMascareño, Alejandro SuárezOsorio, Maria Rosa Zapatero2023-03-15T22:33:40Z2022-102022-10-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article9application/pdfhttp://hdl.handle.net/10362/150645engda Fonseca, V., Barreiro, T., Nunes, N. J., Cristiani, S., Cupani, G., D'Odorico, V., Leite, A. C. O., Marques, C. M. J., Martins, C. J. A. P., Milaković, D., Molaro, P., Murphy, M. T., Schmidt, T. M., Abreu, M., Adibekyan, V., Cabral, A., Di Marcantonio, P., González Hernández, J. I., Palle, E., ... Osorio, M. R. Z. (2022). Fundamental physics with ESPRESSO: Constraining a simple parametrisation for varying. Astronomy and Astrophysics, 666, [A57]. https://doi.org/10.1051/0004-6361/2022437950004-6361PURE: 55894238https://doi.org/10.1051/0004-6361/202243795info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2023-07-10T16:12:51ZPortal AgregadorONG
dc.title.none.fl_str_mv Fundamental physics with ESPRESSO
Constraining a simple parametrisation for varying
title Fundamental physics with ESPRESSO
spellingShingle Fundamental physics with ESPRESSO
da Fonseca, Vítor
Dark energy
Astronomy and Astrophysics
Space and Planetary Science
title_short Fundamental physics with ESPRESSO
title_full Fundamental physics with ESPRESSO
title_fullStr Fundamental physics with ESPRESSO
title_full_unstemmed Fundamental physics with ESPRESSO
title_sort Fundamental physics with ESPRESSO
author da Fonseca, Vítor
author_facet da Fonseca, Vítor
Barreiro, Tiago
Nunes, Nelson J.
Cristiani, Stefano
Cupani, Guido
D'Odorico, Valentina
Leite, Ana C. O.
Marques, Catarina M. J.
Martins, Carlos J. A. P.
Milaković, Dinko
Molaro, Paolo
Murphy, Michael T.
Schmidt, Tobias M.
Abreu, Manuel
Adibekyan, Vardan
Cabral, Alexandre
Di Marcantonio, Paolo
González Hernández, Jonay I.
Palle, Enric
Pepe, Francesco A.
Rebolo, Rafael
Santos, Nuno C.
Sousa, Sérgio G.
Sozzetti, Alessandro
Mascareño, Alejandro Suárez
Osorio, Maria Rosa Zapatero
author_role author
author2 Barreiro, Tiago
Nunes, Nelson J.
Cristiani, Stefano
Cupani, Guido
D'Odorico, Valentina
Leite, Ana C. O.
Marques, Catarina M. J.
Martins, Carlos J. A. P.
Milaković, Dinko
Molaro, Paolo
Murphy, Michael T.
Schmidt, Tobias M.
Abreu, Manuel
Adibekyan, Vardan
Cabral, Alexandre
Di Marcantonio, Paolo
González Hernández, Jonay I.
Palle, Enric
Pepe, Francesco A.
Rebolo, Rafael
Santos, Nuno C.
Sousa, Sérgio G.
Sozzetti, Alessandro
Mascareño, Alejandro Suárez
Osorio, Maria Rosa Zapatero
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv DF – Departamento de Física
RUN
dc.contributor.author.fl_str_mv da Fonseca, Vítor
Barreiro, Tiago
Nunes, Nelson J.
Cristiani, Stefano
Cupani, Guido
D'Odorico, Valentina
Leite, Ana C. O.
Marques, Catarina M. J.
Martins, Carlos J. A. P.
Milaković, Dinko
Molaro, Paolo
Murphy, Michael T.
Schmidt, Tobias M.
Abreu, Manuel
Adibekyan, Vardan
Cabral, Alexandre
Di Marcantonio, Paolo
González Hernández, Jonay I.
Palle, Enric
Pepe, Francesco A.
Rebolo, Rafael
Santos, Nuno C.
Sousa, Sérgio G.
Sozzetti, Alessandro
Mascareño, Alejandro Suárez
Osorio, Maria Rosa Zapatero
dc.subject.por.fl_str_mv Dark energy
Astronomy and Astrophysics
Space and Planetary Science
topic Dark energy
Astronomy and Astrophysics
Space and Planetary Science
description This work was financed by FEDER–Fundo Europeu de Desenvolvimento Regional funds through the COMPETE 2020–Operational Programme for Competitiveness and Internationalisation (POCI), and by Portuguese funds through FCT – Fundação para a Ciência e a Tecnologia under projects POCI-01-0145-FEDER-028987. MTM acknowledges the support of the Australian Research Council through Future Fellowship grant FT180100194. The INAF authors acknowledge financial support of the Italian Ministry of Education, University, and Research with PRIN 201278X4FL and the “Progetti Premiali” funding scheme. TMS also acknowledges the support from the Swiss National Science Foundation (SNSF) and the University of Geneva. M-RZO acknowledges funding under project PID2019-109522GB-C51 of the Spanish Ministerio de Ciencia e Investigación. ASM and JIGH acknowledge financial support from the Spanish Ministry of Science and Innovation (MICIN) project PID2020-117493GB-I00. ASM also acknowledges financial support from the Spanish Ministry of Science and Innovation (MICINN) under 2018 Juan de la Cierva program IJC2018-035229-I, as well as from the Government of the Canary Islands project ProID2020010129. Publisher Copyright: ©
publishDate 2022
dc.date.none.fl_str_mv 2022-10
2022-10-01T00:00:00Z
2023-03-15T22:33:40Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10362/150645
url http://hdl.handle.net/10362/150645
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv da Fonseca, V., Barreiro, T., Nunes, N. J., Cristiani, S., Cupani, G., D'Odorico, V., Leite, A. C. O., Marques, C. M. J., Martins, C. J. A. P., Milaković, D., Molaro, P., Murphy, M. T., Schmidt, T. M., Abreu, M., Adibekyan, V., Cabral, A., Di Marcantonio, P., González Hernández, J. I., Palle, E., ... Osorio, M. R. Z. (2022). Fundamental physics with ESPRESSO: Constraining a simple parametrisation for varying. Astronomy and Astrophysics, 666, [A57]. https://doi.org/10.1051/0004-6361/202243795
0004-6361
PURE: 55894238
https://doi.org/10.1051/0004-6361/202243795
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
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