Einstein-Horndeski gravity and the ultra slowly evaporating black hole
arXiv:2411.03785 · doi:10.1016/j.physletb.2025.139303
Abstract
In this work, we study the evaporation behaviors of asymptotically flat charged black holes in the Einstein-Horndeski gravity theory. Based on the thermodynamics of the Horndeski black hole, we present a physical understanding of the scalar charge of the Horndeski black hole and also clarify its connection to the Einstein vector theory. As the presence of non-minimal coupling, the evaporating behaviors of the Horndeski black hole are vastly different from the Reissner-Nordstrom (RN) black hole case. Due to the different spacetime and electric field structures, the evaporation rate of the Horndeski black hole will slow down at the late stage of evaporation and thus gain a lifetime much longer than the RN black hole. These results illuminate the effect of non-minimally coupled matters on the black hole evaporation and provide clues to search for these matter fields in future observations.
9 pages 3 figures
References in corpus (38)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Observation of Gravitational Waves from a Binary Black Hole Merger
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- Complexity Equals Action
- A no-hair theorem for the galileon
- Exact cosmological solutions with nonminimal derivative coupling
- Quintessence and phantom cosmology with non-minimal derivative coupling
- Asymptotically locally AdS and flat black holes in the presence of an electric field in the Horndeski scenario
- UV-Protected Inflation
- Black Hole Entropy and Viscosity Bound in Horndeski Gravity
- Investigating shadow images and rings of the charged Horndeski black hole illuminated by various thin accretions
- Lifshitz black holes with a time-dependent scalar field in Horndeski theory
- Thermodynamics of Charged Black Holes in Einstein-Horndeski-Maxwell Theory
- Non-Perturbative Quark-Antiquark Production From a Constant Chromo-Electric Field via the Schwinger Mechanism
- Einstein-Vector Gravity, Emerging Gauge Symmetry and de Sitter Bounce
- Building a Holographic Superconductor with a Scalar Field Coupled Kinematically to Einstein Tensor
- Scalar Charges in Asymptotic AdS Geometries
- Hawking evaporation of Einstein-Gauss-Bonnet AdS black holes in dimensions
- DC Conductivities with Momentum Dissipation in Horndeski Theories
- Holographic Complexity Growth Rate in Horndeski Theory
- P-V criticality in the extended phase space of black holes in Einstein-Horndeski gravity
- Black hole evaporation in Lovelock gravity with diverse dimensions
- Finite Upper Bound for the Hawking Decay Time of an Arbitrarily Large Black Hole in Anti-de Sitter Spacetime
- On Thermodynamics of AdS Black Holes with Scalar Hair
- Black hole evaporation in de Sitter space
- Cosmic Censorship and the Evolution of d-Dimensional Charged Evaporating Black Holes
- Thermodynamics of Horndeski black holes with non-minimal derivative coupling
- Black Hole Evaporation in Hořava-Lifshitz Gravity
- Hawking Evaporation of Black Holes in Massive Gravity
- Thermodynamics and evaporation of perfect fluid dark matter black hole in phantom background
- Notes on thermodynamics of Schwarzschild-like bumblebee black hole
- Superradiant energy extraction from rotating hairy Horndeski black holes
- AdS/BCFT correspondence and Horndeski gravity in the presence of gauge fields: holographic paramagnetism/ferromagnetism phase transition
- Magnetized AdS/BCFT Correspondence in Horndeski Gravity
- Transport properties in the Horndeski holographic two-currents model
Cited by in corpus (6)
- Particle creation and evaporation in Kalb-Ramond gravity
- Particle production induced by a Lorentzian non-commutative spacetime
- A Non-Commutative Kalb-Ramond Black Hole
- Particle production, absorption, scattering, and geodesics in a Schwarzschild-Hernquist black hole
- Spin effects on particle creation and evaporation in gravity
- Kiselev black hole and the ultra-slow evaporating behavior