The multipole expansion of the local expansion rate
Résumé
We design a new observable, the expansion rate fluctuation $\eta$, to characterize deviations from the linear relation between redshift and distance in the local universe. We also show how to compress the resulting signal into spherical harmonic coefficients in order to better decipher the structure and symmetries of the anisotropies in the local expansion rate. We apply this analysis scheme to several public catalogs of redshift-independent distances, the Cosmicflows-3 and Pantheon data sets, covering the redshift range $0.01
Domaines
Astrophysique [astro-ph]INSPIRE HEP : Connectez-vous pour contacter le contributeur
https://hal.science/hal-03838356
Soumis le : jeudi 3 novembre 2022-15:00:35
Dernière modification le : lundi 6 mai 2024-18:58:02
Dates et versions
Identifiants
- HAL Id : hal-03838356 , version 1
- ARXIV : 2210.11333
- DOI : 10.1103/PhysRevD.107.023507
- INSPIRE : 2168171
Citer
Basheer Kalbouneh, Christian Marinoni, Julien Bel. The multipole expansion of the local expansion rate. Physical Review D, 2023, 107 (2), pp.023507. ⟨10.1103/PhysRevD.107.023507⟩. ⟨hal-03838356⟩
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