Constraints on Horndeski gravity with phantom crossing
- 1Institute of Cosmology and Gravitation, University of Portsmouth , Burnaby Road, Portsmouth PO1 3FX ,
- 2Max-Planck-Institut für Astronomie , Königstuhl 17, D-69117 Heidelberg ,
Abstract
Gravity models in which the dark energy equation of state crosses w=−1, also known as the phantom divide, have received extensive interest due to recent analyses favouring this behaviour. We introduce a new subclass of Horndeski scalar–tensor models capable of generating phantom crossing, whilst remaining minimally coupled to matter: the Asymptotic Cubic Galileon (ACG) models. We show that ACG models can jointly fit the expansion history inferred from observations of the Planck cosmic microwave background, baryon acoustic oscillation measurements from the Dark Energy Spectroscopic Instrument, and distance-ladder supernovae measurements from the Dark Energy Survey. We then demonstrate that requiring a positive galaxy–Integrated Sachs–Wolfe cross-correlation, together with physically viable screening behaviour, substantially restricts the viable ACG parameter space. Model comparison metrics, including χ 2 and Bayesian evidence, favour both ACG and w0waCDM (cold dark matter) models over ΛCDM, with ACG providing a fit of comparable quality to w0waCDM. Crucially, ACG models ground the observationally preferred w0waCDM behaviour in a robust Lagrangian formulation. This enables interpretation beyond mere phenomenological fits, and motivates further tests of these models on non-linear scales.
Versions
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BibTeX
@article{naidoo2026constraints,
title = {{Constraints on Horndeski gravity with phantom crossing}},
author = {Krishna Naidoo and James Hallam and Tessa Baker and Sergi Sirera},
journal = {Monthly Notices of the Royal Astronomical Society},
year = {2026},
month = oct,
doi = {10.1093/mnras/stag1958},
url = {https://academic.oup.com/mnras/article/doi/10.1093/mnras/stag1958/8916634},
note = {CC BY 4.0},
}
RIS
TY - JOUR
TI - Constraints on Horndeski gravity with phantom crossing
AU - Krishna Naidoo
AU - James Hallam
AU - Tessa Baker
AU - Sergi Sirera
PY - 2026
DA - 2026/10/14
JO - Monthly Notices of the Royal Astronomical Society
DO - 10.1093/mnras/stag1958
UR - https://academic.oup.com/mnras/article/doi/10.1093/mnras/stag1958/8916634
AB - Gravity models in which the dark energy equation of state crosses w=−1, also known as the phantom divide, have received extensive interest due to recent analyses favouring this behaviour. We introduce a new subclass of Horndeski scalar–tensor models capable of generating phantom crossing, whilst remaining minimally coupled to matter: the Asymptotic Cubic Galileon (ACG) models. We show that ACG models can jointly fit the expansion history inferred from observations of the Planck cosmic microwave background, baryon acoustic oscillation measurements from the Dark Energy Spectroscopic Instrument, and distance-ladder supernovae measurements from the Dark Energy Survey. We then demonstrate that requiring a positive galaxy–Integrated Sachs–Wolfe cross-correlation, together with physically viable screening behaviour, substantially restricts the viable ACG parameter space. Model comparison metrics, including χ ^2 and Bayesian evidence, favour both ACG and w_0w_aCDM (cold dark matter) models over ΛCDM, with ACG providing a fit of comparable quality to w_0w_aCDM. Crucially, ACG models ground the observationally preferred w_0w_aCDM behaviour in a robust Lagrangian formulation. This enables interpretation beyond mere phenomenological fits, and motivates further tests of these models on non-linear scales.
SN - 0035-8711
SN - 1365-2966
ER -