Time-Delay Cosmography: Measuring the Hubble Constant and Other Cosmological Parameters with Strong Gravitational Lensing.

Cosmology Dark energy Gravitational lensing Hubble constant

Journal

Space science reviews
ISSN: 0038-6308
Titre abrégé: Space Sci Rev
Pays: Netherlands
ID NLM: 100971458

Informations de publication

Date de publication:
2024
Historique:
received: 03 04 2023
accepted: 08 05 2024
medline: 20 6 2024
pubmed: 20 6 2024
entrez: 20 6 2024
Statut: ppublish

Résumé

Multiply lensed images of a same source experience a relative time delay in the arrival of photons due to the path length difference and the different gravitational potentials the photons travel through. This effect can be used to measure absolute distances and the Hubble constant (

Identifiants

DOI: 10.1007/s11214-024-01079-w PMID: 38899030 PMC: PMC11182856
pubmed: 38899030
doi: 10.1007/s11214-024-01079-w
pii: 1079
pmc: PMC11182856
doi:

Types de publication

Journal Article Review

Langues

eng

Pagination

48

Informations de copyright

© The Author(s) 2024.

Déclaration de conflit d'intérêts

Competing InterestsThe authors declare no competing interests.

Auteurs

S Birrer (S)

Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 USA.
Kavli Institute for Particle Astrophysics and Cosmology and Department of Physics, Stanford University, Stanford, CA 94305 USA.
ORCID: 0000-0003-3195-5507

M Millon (M)

Kavli Institute for Particle Astrophysics and Cosmology and Department of Physics, Stanford University, Stanford, CA 94305 USA.
Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland.

D Sluse (D)

STAR Institute, Quartier Agora - Allée du six Août, 19c B-4000 Liège, Belgium.

A J Shajib (AJ)

Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 USA.
Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637 USA.

F Courbin (F)

Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland.
ICC-UB Institut de Ciències del Cosmos, University of Barcelona, Martí Franquès, 1, E-08028 Barcelona, Spain.
ICREA, Pg. Lluís Companys 23, Barcelona, E-08010 Spain.

S Erickson (S)

Kavli Institute for Particle Astrophysics and Cosmology and Department of Physics, Stanford University, Stanford, CA 94305 USA.

L V E Koopmans (LVE)

Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700AV Groningen, The Netherlands.

S H Suyu (SH)

Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748 Garching, Germany.
TUM School of Natural Sciences, Physics Department, Technical University of Munich, James-Franck-Straße 1, 85748 Garching, Germany.
Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), 11F of ASMAB, No.1, Sect. 4, Roosevelt Road, Taipei, 10617 Taiwan.

T Treu (T)

Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 USA.

Classifications MeSH