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Quintessential Quartic Quasi-topological Quartet

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arxiv 1703.11007 v2 pith:SFVIJPYQ submitted 2017-03-31 hep-th gr-qc

Quintessential Quartic Quasi-topological Quartet

classification hep-th gr-qc
keywords quasi-topologicalsolutionsdimensionsfourgravitypropertiesquartictheories
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We construct the quartic version of generalized quasi-topological gravity, which was recently constructed to cubic order in arXiv: 1703.01631. This class of theories includes Lovelock gravity and a known form of quartic quasi-topological gravity as special cases and possess a number of remarkable properties: (i) In vacuum, or in the presence of suitable matter, there is a single independent field equation which is a total derivative. (ii) At the linearized level, the equations of motion on a maximally symmetric background are second order, coinciding with the linearized Einstein equations up to a redefinition of Newton's constant. Therefore, these theories propagate only the massless, transverse graviton on a maximally symmetric background. (iii) While the Lovelock and quasi-topological terms are trivial in four dimensions, there exist four new generalized quasi-topological terms (the quartet) that are nontrivial, leading to interesting higher curvature theories in $d \geq 4$ dimensions that appear well suited for holographic study. We construct four dimensional black hole solutions to the theory and study their properties. A study of black brane solutions in arbitrary dimensions reveals that these solutions are modified from the `universal' properties these solutions have. This result may lead to interesting consequences for the dual CFTs.

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Cited by 6 Pith papers

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

  1. Regular Black Holes in Nonlocal Quasitopological Gravity

    gr-qc 2026-07 accept novelty 7.0

    Infinite-derivative completions of quasitopological gravities are ghost-free, avoid strong coupling, and admit exact spherically symmetric vacuum regular black holes obeying a perturbative Birkhoff theorem.

  2. Cosmic Inflation From Regular Black Holes

    gr-qc 2026-04 unverdicted novelty 7.0

    Regular black holes in the bulk of quasi-topological gravity drive a de Sitter inflationary phase on the brane at small scales, with e-fold number set by the ratio of black hole radius to higher-curvature scale.

  3. Regular Vaidya solutions of effective gravitational theories

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    gr-qc 2026-07 accept novelty 6.0

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  5. Off-shell Hessian thermodynamic stability of higher-curvature black holes

    gr-qc 2026-06 unverdicted novelty 6.0

    An off-shell Hessian criterion H = S'_W(r_h) T'(r_h) governs thermodynamic stability of higher-curvature black holes, recovering the temperature-slope rule on physical branches and producing mean-field critical exponents.

  6. From Ringdown to Lensing: Analytic Eikonal Modes of Quasi-Topological Regular Black Holes

    gr-qc 2026-04 unverdicted novelty 5.0

    Analytic quasinormal-mode expressions and explicit QNM-shadow-lensing correspondence for four-dimensional quasi-topological regular black holes.