Kerr-Schild perturbations in higher derivative gravity theories in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>D</mml:mi> </mml:math> dimensions

We study Kerr-Schild perturbations of a ghost-free, generic nonlocal gravity theory constructed from an infinite series of higher-derivative terms in $D$ dimensions. The infinite series of higher-derivative terms are encoded by form factors, the forms of which can be restricted by requiring that the action remains perturbatively free of ghosts and tachyons around maximally symmetric backgrounds for transverse-traceless fluctuations. To demonstrate this, we obtain field equations for the anti--de Sitter plane-wave metric in Kerr-Schild form, which yield linearized field equations for transverse-traceless spin-2 field. Using unitarity and consistency requirements, we obtain, as an example, the explicit derivation of nonlocal form factors in $D$ dimensions.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-11-25
DOI
https://doi.org/10.1103/y57m-rwpv
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
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article

Kerr-Schild perturbations in higher derivative gravity theories in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>D</mml:mi> </mml:math> dimensions

Karl J. Friston
Physical review. D/Physical review. D.
Black Holes and Theoretical Physics
article

Kerr-Schild perturbations in higher derivative gravity theories in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mi>D</mml:mi> </mml:math> dimensions

Karl J. Friston
article en

Abstract

We study Kerr-Schild perturbations of a ghost-free, generic nonlocal gravity theory constructed from an infinite series of higher-derivative terms in $D$ dimensions. The infinite series of higher-derivative terms are encoded by form factors, the forms of which can be restricted by requiring that the action remains perturbatively free of ghosts and tachyons around maximally symmetric backgrounds for transverse-traceless fluctuations. To demonstrate this, we obtain field equations for the anti--de Sitter plane-wave metric in Kerr-Schild form, which yield linearized field equations for transverse-traceless spin-2 field. Using unitarity and consistency requirements, we obtain, as an example, the explicit derivation of nonlocal form factors in $D$ dimensions.

Physical review. D/Physical review. D.Vol. 112(12)
Usak University (TR)
Openalex Percentile: Top 82%
Black Holes and Theoretical Physics
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