UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data

Lodha, K; Shafieloo, A; Calderon, R; Linder, E; Sohn, W; Cervantes-Cota, JL; De Mattia, A; ... Zou, H; + view all (2025) DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data. Physical Review D , 111 (2) , Article 023532. 10.1103/PhysRevD.111.023532. Green open access

[thumbnail of PhysRevD.111.023532.pdf]
Preview
Text
PhysRevD.111.023532.pdf - Published Version

Download (1MB) | Preview

Abstract

Baryon acoustic oscillation data from the first year of the Dark Energy Spectroscopic Instrument (DESI) provide near percent-level precision of cosmic distances in seven bins over the redshift range z=0.1-4.2. This paper is the follow-up to the original DESI BAO cosmology paper [A. G. Adame (DESI Collaboration), arXiv:2404.03002], which considered the conventional w0wa cold dark matter (CDM) model. We use the novel DESI data, together with other cosmic probes, to constrain the background expansion history using some well-motivated physical classes of dark energy. In particular, we explore three physics-focused behaviors of dark energy from the equation of state and energy density perspectives: the thawing class (matching many simple quintessence potentials), emergent class (where dark energy comes into being recently, as in phase transition models), and mirage class [where phenomenologically the distance to cosmic microwave background (CMB) last scattering is close to that from a cosmological constant Λ despite dark energy dynamics]. All three classes fit the data at least as well as ΛCDM, and indeed can improve on it by Δχ2≈-5 to -17 for the combination of DESI BAO with CMB and supernova data while having one more parameter. The mirage class does essentially as well as w0waCDM and exhibits moderate to strong Bayesian evidence preference with respect to ΛCDM. These classes of dynamical behaviors highlight worthwhile avenues for further exploration into the nature of dark energy.

Type: Article
Title: DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data
Open access status: An open access version is available from UCL Discovery
DOI: 10.1103/PhysRevD.111.023532
Publisher version: https://doi.org/10.1103/physrevd.111.023532
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10205459
Downloads since deposit
Loading...
20Downloads
Download activity - last month
Loading...
Download activity - last 12 months
Loading...
Downloads by country - last 12 months
Loading...

Archive Staff Only

View Item View Item