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Disformal Transformations, Veiled General Relativity and Mimetic Gravity

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it
abstract

In this Note we show that Einstein's equations for gravity are generically invariant under 'disformations'. We also show that the particular subclass when this is not true yields the equations of motion of 'Mimetic Gravity'. Finally we give the 'mimetic' generalization of the Schwarzschild solution.

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Fragility of stealth solutions in mimetic gravity

gr-qc · 2026-06-30 · unverdicted · novelty 7.0

Stealth solutions in mimetic gravity decouple from background dynamics on the lambda=0 branch but impose an infinite hierarchy of constraints on perturbations, rendering the screening limit non-uniform and pathological.

Imperfect dark matter with higher derivatives

gr-qc · 2025-10-27 · unverdicted · novelty 6.0

Higher-derivative extension of dark matter yields an imperfect fluid that matches pressureless dust on homogeneous backgrounds but generates acceleration and vorticity to avoid caustic singularities in inhomogeneous cosmologies.

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Showing 3 of 3 citing papers after filters.

  • Fragility of stealth solutions in mimetic gravity gr-qc · 2026-06-30 · unverdicted · none · ref 17 · internal anchor

    Stealth solutions in mimetic gravity decouple from background dynamics on the lambda=0 branch but impose an infinite hierarchy of constraints on perturbations, rendering the screening limit non-uniform and pathological.

  • Gravitational wave constraints on the Paneitz operator gr-qc · 2026-04-30 · unverdicted · none · ref 27

    The Paneitz operator in 4D belongs to extended mimetic gravity and is constrained by gravitational wave propagation speed.

  • Imperfect dark matter with higher derivatives gr-qc · 2025-10-27 · unverdicted · none · ref 18 · internal anchor

    Higher-derivative extension of dark matter yields an imperfect fluid that matches pressureless dust on homogeneous backgrounds but generates acceleration and vorticity to avoid caustic singularities in inhomogeneous cosmologies.