A universal relation among Euclidean integrals for black holes in higher-derivative gravity theories
arXiv:2508.05326 · doi:10.1103/njlp-rm1c
Abstract
In this paper, we establish a universal equality governing Euclidean integrals of gravitational actions in higher-derivative theories. This relation is shown to hold universally for asymptotically flat black holes in pure gravity, and is generalized to asymptotically anti-de Sitter (AdS) spacetimes through appropriate regularization. We further examine its validity in systems with matter-gravity coupling, identifying that violations occur only when matter fields exhibit pathological behaviors: divergence at the horizon or non-decaying profiles at infinity. These findings reveal fundamental constraints on gravitational thermodynamics and provide diagnostic tools for identifying ill-behaved matter configurations.
10 papges, no figures, accepted version
References in corpus (12)
- Modified Gravity and Cosmology
- Lorentz violation with an antisymmetric tensor
- Black holes in an Effective Field Theory extension of GR
- Generalized ghost-free quadratic curvature gravity
- Black Hole Entropy and Viscosity Bound in Horndeski Gravity
- Classification of Six Derivative Lagrangians of Gravity and Static Spherically Symmetric Solutions
- Thermodynamics of Charged Black Holes in Einstein-Horndeski-Maxwell Theory
- The minus sign in the first law of de Sitter horizons
- On Euclidean and Noetherian Entropies in AdS Space
- Extended black hole thermodynamics from extended Iyer-Wald formalism
- On the first order corrections to the black hole thermodynamics in higher curvature theories of gravity
- Black hole entropy contributions from Euclidean cores