Thermodynamics of black holes featuring primary scalar hair
arXiv:2404.07522 · doi:10.1103/PhysRevD.110.L101502
Abstract
In this work, we embark on the thermodynamic investigation concerning a family of primary charged black holes within the context of shift and parity symmetric Beyond Horndeski gravity. Employing the Euclidean approach, we derive the functional expression for the free energy and derive the first thermodynamic law, offering a methodology to address the challenge of extracting the thermal quantities in shift-symmetric scalar tensor theories characterized by linear time dependence in the scalar field. Following the formal analysis, we provide some illustrative examples focusing on the thermal evaporation of these fascinating objects.
8 pages, 1 figure, typos corrected
References in corpus (15)
- Healthy theories beyond Horndeski
- Horndeski theory and beyond: a review
- Black Hole Solutions as Topological Thermodynamic Defects
- Regular black holes: A short topic review
- Corrected form of the first law of thermodynamics for regular black holes
- Charged Galileon black holes
- Linear stability analysis of hairy black holes in quadratic degenerate higher-order scalar-tensor theories: Odd-parity perturbations
- Thermodynamics of a BTZ black hole solution with an Horndeski source
- On Rotating Black Holes in DHOST Theories
- Disforming the Kerr metric
- Black holes with primary scalar hair
- Astrophysical constraints on compact objects in 4D Einstein-Gauss-Bonnet gravity
- Extended black hole thermodynamics from extended Iyer-Wald formalism
- On Thermal Stability of Hairy Black Holes
- Compact objects with primary hair in shift and parity symmetric beyond Horndeski gravities
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- A First-Order Eikonal Framework for Quasinormal Modes, Shadows, Strong Lensing, and Grey-Body Factors in a Scalarized Black-Hole Metric
- Smarr formula for black holes with primary and secondary scalar hair
- Regular black holes and reductions of thermodynamic phase spaces
- Theoretical filters for shift-symmetric Horndeski gravities
- Thermodynamically massless Simpson-Visser black holes
- Effect of primary scalar hair on black hole's strong lensing in Beyond Horndeski Gravity