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New tests of dark sector interactions from the full-shape galaxy power spectrum
dc.contributor.author | Nunes, Rafael da Costa | pt_BR |
dc.contributor.author | Vagnozzi, Sunny | pt_BR |
dc.contributor.author | Kumar, Suresh | pt_BR |
dc.contributor.author | Di Valentino, Eleonora | pt_BR |
dc.contributor.author | Mena Requejo, Olga | pt_BR |
dc.date.accessioned | 2022-10-03T04:48:38Z | pt_BR |
dc.date.issued | 2022 | pt_BR |
dc.identifier.issn | 0556-2821 | pt_BR |
dc.identifier.uri | http://hdl.handle.net/10183/249553 | pt_BR |
dc.description.abstract | We explore the role of redshift-space galaxy clustering data in constraining nongravitational interactions between dark energy (DE) and dark matter (DM), for which state-of-the-art limits have so far been obtained from late-time background measurements. We use the joint likelihood for prereconstruction full-shape (FS) galaxy power spectrum and postreconstruction Baryon Acoustic Oscillation (BAO) measurements from the BOSS DR12 sample, alongside Cosmic Microwave Back ground (CMB) data from Planck: from this dataset combination we infer H0 ¼ 68.02þ0.49 −0.60 km=s=Mpc and the 2σ lower limit ξ > −0.12, among the strongest limits ever reported on the DM-DE coupling strength ξ for the particular model considered. Contrary to what has been observed for the ΛCDM model and simple extensions thereof, we find that the CMB þ FS combination returns tighter constraints compared to the CMB þ BAO one, suggesting that there is valuable additional information contained in the broadband of the power spectrum. We test this finding by running additional CMB-free analyses and removing sound horizon information, and discuss the important role of the equality scale in setting constraints on DM-DE interactions. Our results reinforce the critical role played by redshift-space galaxy clustering measurements in the epoch of precision cosmology, particularly in relation to tests of nonminimal dark sector extensions of the ΛCDM model. | en |
dc.format.mimetype | application/pdf | pt_BR |
dc.language.iso | eng | pt_BR |
dc.relation.ispartof | Physical Review. D, Particles and fields. Woodbury. Vol. 105, no. 12 (June 2022), 123506, 18 p. | pt_BR |
dc.rights | Open Access | en |
dc.subject | Aglomerados de galaxias | pt_BR |
dc.subject | Deslocamento para o vermelho | pt_BR |
dc.subject | Energia escura | pt_BR |
dc.subject | Matéria escura | pt_BR |
dc.title | New tests of dark sector interactions from the full-shape galaxy power spectrum | pt_BR |
dc.type | Artigo de periódico | pt_BR |
dc.identifier.nrb | 001145718 | pt_BR |
dc.type.origin | Estrangeiro | pt_BR |
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