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Extended Cuscuton as Dark Energy

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arxiv 2003.01934 v2 pith:CUEUMTFG submitted 2020-03-04 gr-qc astro-ph.CO

classification gr-qcastro-ph.CO
keywords cuscutonextendedcosmologydarkenergyadmittinganalyticargue
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abstract

Late-time cosmology in the extended cuscuton theory is studied, in which gravity is modified while one still has no extra dynamical degrees of freedom other than two tensor modes. We present a simple example admitting analytic solutions for the cosmological background evolution that mimics $\Lambda$CDM cosmology. We argue that the extended cuscuton as dark energy can be constrained, like usual scalar-tensor theories, by the growth history of matter density perturbations and the time variation of Newton's constant.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cosmological constraints and standard sirens forecasts for non-dynamical dark energy in Horndeski gravity

    astro-ph.CO 2026-08 conditional novelty 5.0 of 10

    Standard sirens from third-generation detectors could measure H0 to 0.21% in Extended Cuscuton models, but the forecast omits the modified GW luminosity distance.

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