An exact black hole spacetime with scalar field and its shadow together with quasinormal modes

Abstract

We find an exact black hole solution with a minimally coupled scalar field. The corresponding spacetime has two horizons and one of the them is the black hole event horizon and the other is the cosmic horizon. In this sense, the solution is analogous to the Schwarzschild-de Sitter (or anti-de Sitter) spacetime. We investigate the thermodynamics and construct the first law of thermodynamics. At the same time, we make a study on the shadow and quasinormal modes of this black hole solution.

arXiv comment9 pages, 4 figures

References in corpus (71)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
• Thermodynamics of Spacetime: The Einstein Equation of State
• Quasinormal modes of black holes and black branes
• Quasi-Normal Modes of Stars and Black Holes
• Quasinormal modes of black holes: from astrophysics to string theory
• First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
• Thermodynamical Aspects of Gravity: New insights
• Kerr black holes with scalar hair
• General Laws of Black-Hole Dynamics
• Unified first law of black-hole dynamics and relativistic thermodynamics
• Gravity and the Thermodynamics of Horizons
• Classical and Quantum Thermodynamics of horizons in spherically symmetric spacetimes
• Black hole hair in generalized scalar-tensor gravity
• Non-equilibrium Thermodynamics of Spacetime
• Unified First Law and Thermodynamics of Apparent Horizon in FRW Universe
• Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
• Shadow of a black hole surrounded by dark matter
• Thermodynamic route to Field equations in Lanczos-Lovelock Gravity
• A new method for shadow calculations: application to parameterised axisymmetric black holes
• The Current Ability to Test Theories of Gravity with Black Hole Shadows
• Black hole shadow in an asymptotically-flat, stationary, and axisymmetric spacetime: The Kerr-Newman and rotating regular black holes
• Shadows of Einstein-dilaton-Gauss-Bonnet black holes
• Friedmann Equations and Thermodynamics of Apparent Horizons
• Shadow cast and Deflection angle of Kerr-Newman-Kasuya spacetime
• Black hole shadow in an expanding universe with a cosmological constant
• Chaotic lensing around boson stars and Kerr black holes with scalar hair
• Black hole shadow in a general rotating spacetime obtained through Newman-Janis algorithm
• Shadows of rotating wormholes
• BlackHoleCam: fundamental physics of the Galactic center
• Gravitational Lensing in presence of Plasma: Strong Lens Systems, Black Hole Lensing and Shadow
• Quasinormal modes of Schwarzschild black holes in four and higher dimensions
• Black hole mimicker hiding in the shadow: Optical properties of the $\gamma$-metric
• Black holes with surrounding matter in scalar-tensor theories
• Shadow casted by a Konoplya-Zhidenko rotating non-Kerr black hole
• Matter around Kerr black holes in scalar-tensor theories: scalarization and superradiant instability
• Shadows of rotating five-dimensional charged EMCS black holes
• Scalar mesostatic field with regard for gravitational effects
• Shadows, Signals, and Stability in Einsteinian Cubic Gravity
• Scalar hairy black holes and solitons in asymptotically flat spacetimes
• Phases of 4D Scalar-tensor black holes coupled to Born-Infeld nonlinear electrodynamics
• Shadow of a black hole at cosmological distance
• Energy conservation for dynamical black holes
• Spherically symmetric false vacuum: no-go theorems and global structure
• Shadows of Bonnor black dihole by chaotic lensing
• Chaotic shadow of a non-Kerr rotating compact object with quadrupole mass moment
• Intrinsic curvature and topology of shadows in Kerr spacetime
• Revisiting the shadow of a black hole in the presence of a plasma
• Lanczos-Lovelock gravity from a thermodynamic perspective
• Quasi-normal modes, bifurcations and non-uniqueness of charged scalar-tensor black holes
• Phase Space Analysis of Quintessence Cosmologies with a Double Exponential Potential
• Exact Hairy Black Holes and their Modification to the Universal Law of Gravitation
• Quasinormal Modes of a Black Hole with Quadrupole Moment
• Shadow of charged wormholes in Einstein-Maxwell-dilaton theory
• Instability of Small Lovelock Black Holes in Even-dimensions
• Spherically symmetric scalar vacuum: no-go theorems, black holes and solitons
• New hairy black hole solutions with a dilaton potential
• Black hole shadow with a cosmological constant for cosmological observers
• Quantization of Higher Dimensional Linear Dilaton Black Hole Area/Entropy From Quasinormal Modes
• Event horizon image within black hole shadow
• Decay of massless Dirac field around the Born-Infeld Black Hole
• Asymptotic Quasinormal Modes of d-Dimensional Schwarzschild Black Hole with Gauss-Bonnet Correction
• Asymptotic quasinormal modes of a noncommutative geometry inspired Schwarzschild black hole
• Gravitational Lensing of a star by a rotating black hole
• No-go theorem for false vacuum black holes
• Quasinormal modes and late-time tails in the background of Schwarzschild black hole pierced by a cosmic string: scalar, electromagnetic and gravitational perturbations
• First Law of Black Saturn Thermodynamics
• Quansinormal modes of static and spherically symmetric black holes with the derivative coupling
• Black Holes in Magnetic Monopoles with a Dark Halo
• Large Gauge Symmetries of an Asymptotically de Sitter Horizon: An Extended First Law of Thermodynamics

Cited by in corpus (4)

• Shadow and Quasinormal Modes of a Rotating Loop Quantum Black Hole
• Hairy black holes in DHOST theories: Exploring disformal transformation as a solution-generating method
• Null geodesics, quasinormal modes and the correspondence with shadows in high-dimensional Einstein-Yang-Mills spacetimes
• Visible shapes of black holes M87* and SgrA*