Self tuning scalar tensor black holes
arXiv:1501.05167 · doi:10.1088/1742-6596/600/1/012003
Abstract
Studying a certain sub class of higher order Horndeski (scalar-tensor) theories we discuss a method discovered recently permitting analytic black hole solutions with a non trivial and regular scalar field. One of the solutions found has de Sitter asymptotics and self tunes the bulk cosmological constant. Using the aforementioned method we find and analyse new black hole solutions which can also have de Sitter asymptotics. By looking at small deviations of the integration constant responsible for self tuning we discuss the robustness of the self tuning mechanism. We find that neighboring solutions to the one previously found present also self tuning properties with unaltered effective cosmological constant.
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References in corpus (35)
- An Alternative to Compactification
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- f(R) Theories Of Gravity
- Modified Gravity and Cosmology
- 4D Gravity on a Brane in 5D Minkowski Space
- Quantum Gravity at a Lifshitz Point
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- The galileon as a local modification of gravity
- From k-essence to generalised Galileons
- Covariant Galileon
- Gravity with a dynamical preferred frame
- Membranes at Quantum Criticality
- Generalized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress tensors
- A healthy extension of Horava gravity
- Avoiding Dark Energy with 1/R Modifications of Gravity
- Black hole hair in generalized scalar-tensor gravity
- General second order scalar-tensor theory, self tuning, and the Fab Four
- Dressing a black hole with a time-dependent Galileon
- An introduction to the Vainshtein mechanism
- A no-hair theorem for the galileon
- Black holes with non-minimal derivative coupling
- de Sitter black hole with a conformally coupled scalar field in four dimensions
- Self-tuning and the derivation of the Fab Four
- Sequestering the Standard Model Vacuum Energy
- Comment on `Strong coupling in extended Horava-Lifshitz gravity'
- Galileons from Lovelock actions
- Black Holes in Bi-scalar Extensions of Horndeski Theories
- Higher order gravity theories and their black hole solutions
- Chameleon Field Theories
- New Charged Black Holes with Conformal Scalar Hair
- Purely Kinetic Coupled Gravity
- Gravity and Scalar Fields
- Hairy black holes in theories with massive gravitons
- Construction and physical properties of Kerr black holes with scalar hair
- From Lovelock to Horndeski's generalised scalar-tensor theory
Cited by in corpus (37)
- Asymptotically flat black holes in Horndeski theory and beyond
- Black holes and stars in Horndeski theory
- Neutron stars in general second order scalar-tensor theory: the case of non-minimal derivative coupling
- Lectures on the Cosmological Constant Problem
- Charged Galileon black holes
- Cosmological self-tuning and local solutions in generalized Horndeski theories
- Hamiltonian vs stability and application to Horndeski theory
- Black holes in a cubic Galileon universe
- Black holes and solitons in an extended Proca theory
- Black holes with primary scalar hair
- Compact objects in Horndeski gravity
- The Well-Tempered Cosmological Constant
- A no-hair theorem for stars in Horndeski theories
- Metric-Affine Gravity and Cosmology/Aspects of Torsion and non-Metricity in Gravity Theories
- Axial quasinormal modes of static neutron stars in the nonminimal derivative coupling sector of Horndeski gravity: spectrum and universal relations for realistic equations of state
- On Lovelock galileons and black holes
- Hairy Taub-NUT/Bolt-AdS solutions in Horndeski theory
- Self Tuning Scalar Fields in Spherically Symmetric Spacetimes
- Compact objects of spherical symmetry in beyond Horndeski theories
- Beyond Fab Four
- Compact objects with primary hair in shift and parity symmetric beyond Horndeski gravities
- Conformally coupled theories and their deformed compact objects: from black holes, radiating spacetimes to eternal wormholes
- Asymptotically flat black holes with scalar hair: a review
- Stable black holes in shift-symmetric Horndeski theories
- Selecting Horndeski theories without apparent symmetries and their black hole solutions
- Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations
- Novel exact ultra-compact and ultra-sparse hairy black holes emanating from regular and phantom scalar fields
- Warped-AdS3 black holes with scalar halo
- Black holes in massive conformal gravity
- Black holes in new massive conformal gravity
- Compact astrophysical objects in modified gravity
- Scalar-tensor black holes in an expanding universe
- Stealth Ellis Wormholes In Horndeski theories
- Stealth black holes in Aether Scalar Tensor theory
- Extension of Buchdahl's Theorem on Reciprocal Solutions
- Theoretical filters for shift-symmetric Horndeski gravities
- Effective Field Theory of Hairy Black Holes and Their flat/dS limit