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Cosmology and fundamental physics with the ELT-ANDES spectrograph.
Martins, C J A P; Cooke, R; Liske, J; Murphy, M T; Noterdaeme, P; Schmidt, T M; Alcaniz, J S; Alves, C S; Balashev, S; Cristiani, S; Di Marcantonio, P; Génova Santos, R; Gonçalves, R S; González Hernández, J I; Maiolino, R; Marconi, A; Marques, C M J; Melo E Sousa, M A F; Nunes, N J; Origlia, L; Péroux, C; Vinzl, S; Zanutta, A.
Afiliação
  • Martins CJAP; Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal.
  • Cooke R; Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal.
  • Liske J; Centre for Extragalactic Astronomy, Durham University, Science Site, South Road, DH1 3LE Durham, UK.
  • Murphy MT; Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany.
  • Noterdaeme P; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122 Australia.
  • Schmidt TM; Institut d'Astrophysique de Paris, UMR 7095, CNRS-SU, 98bis bd Arago, 75014 Paris, France.
  • Alcaniz JS; French-Chilean Laboratory for Astronomy, IRL 3386, CNRS and U. de Chile, Casilla 36-D, Santiago, Chile.
  • Alves CS; Observatoire Astronomique de l'Université de Genève, Chemin Pegasi 51, Sauverny, CH-1290 Switzerland.
  • Balashev S; Observatório Nacional, 20921-400 Rio de Janeiro, RJ Brazil.
  • Cristiani S; Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal.
  • Di Marcantonio P; Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT UK.
  • Génova Santos R; Ioffe Institute, Polyteknicheskaya 26, 194021 Saint-Petersburg, Russia.
  • Gonçalves RS; INAF-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo, 11, I-34143 Trieste, Italy.
  • González Hernández JI; IFPU-Institute for Fundamental Physics of the Universe, via Beirut 2, I-34151 Trieste, Italy.
  • Maiolino R; INFN-National Institute for Nuclear Physics, via Valerio 2, I-34127 Trieste, Italy.
  • Marconi A; INAF-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo, 11, I-34143 Trieste, Italy.
  • Marques CMJ; Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife Spain.
  • Melo E Sousa MAF; Universidad de La Laguna, Department Astrofísica, E-38206 La Laguna, Tenerife Spain.
  • Nunes NJ; Observatório Nacional, 20921-400 Rio de Janeiro, RJ Brazil.
  • Origlia L; Departamento de Física, Universidade Federal Rural do Rio de Janeiro, 23897-000 Seropédica, RJ Brazil.
  • Péroux C; Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife Spain.
  • Vinzl S; Universidad de La Laguna, Department Astrofísica, E-38206 La Laguna, Tenerife Spain.
  • Zanutta A; Cavendish Laboratory, University of Cambridge, 19 J.J. Thomson Ave., Cambridge, CB3 0HE UK.
Exp Astron (Dordr) ; 57(1): 5, 2024.
Article em En | MEDLINE | ID: mdl-39308933
ABSTRACT
State-of-the-art 19th century spectroscopy led to the discovery of quantum mechanics, and 20th century spectroscopy led to the confirmation of quantum electrodynamics. State-of-the-art 21st century astrophysical spectrographs, especially ANDES at ESO's ELT, have another opportunity to play a key role in the search for, and characterization of, the new physics which is known to be out there, waiting to be discovered. We rely on detailed simulations and forecast techniques to discuss four important examples of this point big bang nucleosynthesis, the evolution of the cosmic microwave background temperature, tests of the universality of physical laws, and a real-time model-independent mapping of the expansion history of the universe (also known as the redshift drift). The last two are among the flagship science drivers for the ELT. We also highlight what is required for the ESO community to be able to play a meaningful role in 2030s fundamental cosmology and show that, even if ANDES only provides null results, such 'minimum guaranteed science' will be in the form of constraints on key cosmological paradigms these are independent from, and can be competitive with, those obtained from traditional cosmological probes.
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Exp Astron (Dordr) Ano de publicação: 2024 Tipo de documento: Article País de afiliação: Portugal País de publicação: Holanda

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Exp Astron (Dordr) Ano de publicação: 2024 Tipo de documento: Article País de afiliação: Portugal País de publicação: Holanda