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Generalized disformal Horndeski theories: cosmological perturbations and consistent matter coupling

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arxiv 2209.02176 v2 pith:ZYQ2PTA3 submitted 2022-09-06 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords theoriesdisformalhorndeskiperturbationsclassconditionscosmologicalgeneralized
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Invertible disformal transformations are a useful tool to investigate ghost-free scalar-tensor theories. By performing a higher-derivative generalization of the invertible disformal transformation on Horndeski theories, we construct a novel class of ghost-free scalar-tensor theories, which we dub generalized disformal Horndeski theories. Specifically, these theories lie beyond the quadratic/cubic DHOST class. We explore cosmological perturbations to identify a subclass where gravitational waves propagate at the speed of light and clarify the conditions for the absence of ghost/gradient instabilities for tensor and scalar perturbations. We also investigate the conditions under which a matter field can be consistently coupled to these theories without introducing unwanted extra degrees of freedom.

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Cited by 4 Pith papers

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

  1. Disformal Maps: Classification and Singular Dynamics

    gr-qc 2026-08 conditional novelty 7.0 of 10

    Disformal transformations are classified by a Cayley-Hamilton degree and Hawking-Ellis type, and the mimetic energy-momentum tensor's type follows from a polynomial map of the original tensor.

  2. A New Definition of Horndeski Theory and the Possibility of Multiple Scalar Field Extensions

    gr-qc 2025-11 conditional novelty 6.0 of 10

    Horndeski theory is re-characterized as the disformally-closed class anchored to a minimal seed action, reproducing the known single-field action and generating multi-field antisymmetric terms, with full multi-field v...

  3. Primordial black hole dark matter from ultra-slow-roll inflation in Horndeski gravity

    gr-qc 2025-12 conditional novelty 5.0 of 10

    A kinetic cubic Horndeski coupling creates an ultra-slow-roll phase that amplifies curvature perturbations enough to produce asteroid-mass primordial black holes, potentially 90% of dark matter.

  4. Stealth black hole solutions in higher-order Maxwell-Einstein theories

    gr-qc 2025-06 conditional novelty 5.0 of 10

    Under specific algebraic conditions on the coupling functions, Reissner-Nordström and Schwarzschild-(A)dS solutions persist in higher-order Maxwell-Einstein theories, including stealth solutions and dyonic solutions i...

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