Shadows of 5D Black Holes from String Theory
arXiv:2008.13478 · doi:10.1016/j.physletb.2020.136025
Abstract
We study the shadow behaviors of five dimensional (5D) black holes embedded in type IIB superstring/supergravity inspired spacetimes by considering solutions with and without rotations. Geometrical properties as shapes and sizes are analyzed in terms of the D3-brane number and the rotation parameter. Concretely, we find that the shapes are indeed significantly distorted by such physical parameters and the size of the shadows decreases with the brane or "color" number and the rotation. Then, we investigate geometrical observables and energy emission rate aspects.
References in corpus (29)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
- P-V criticality of charged AdS black holes
- Charged AdS Black Holes and Catastrophic Holography
- Schwarzschild black hole lensing
- Black Hole Entropy in M-Theory
- Rotation and the AdS/CFT correspondence
- Measurement of the Kerr Spin Parameter by Observation of a Compact Object's Shadow
- Shadow of five-dimensional rotating Myers-Perry black hole
- Silhouette of M87*: A new window to peek into the world of hidden dimensions
- Shadows of Kerr black holes with and without scalar hair
- Shadow of a Spinning Black Hole in an Expanding Universe
- Shapes of rotating nonsingular black hole shadows
- On Thermodynamics of AdS Black Holes in Arbitrary Dimensions
- Quasinormal modes, quasiperiodic oscillations and shadow of rotating regular black holes in non-minimally coupled Einstein-Yang-Mills theory
- Shadows of rotating five-dimensional charged EMCS black holes
- Deflection Angle and Shadow Behaviors of Quintessential Black Holes in arbitrary Dimensions
- Shadows of Sgr A Black Hole Surrounded by Superfluid Dark Matter Halo
- Phase transition and thermodynamical geometry for Schwarzschild AdS black hole in spacetime
- Higher Dimensional Kerr-AdS Black Holes and the AdS/CFT Correspondence
- Thermal Image and Phase Transitions of Charged AdS Black Holes using Shadow Analysis
- Testing the equivalence principle via the shadow of black holes
- On Thermodynamics of AdS Black Holes in M-Theory
- Influence of an anisotropic matter field on the shadow of a rotating black hole
- Holographic Interface-Particle Potential
- Black Hole Shadows in M-theory Scenarios
- Introduction to the AdS/CFT correspondence
- Quasinormal Modes of the Generalized Ayón-Beato-Garc\'ıa Scalar-Tensor-Vector Gravity Black Hole in the Scalar-Tensor-Vector Gravity
- Cosmological Constant Effect on Charged and Rotating Black Hole Shadows
Cited by in corpus (39)
- Probing a nonlinear electrodynamics black hole with thin accretion disk, shadow and deflection angle with M87* and Sgr A* from EHT
- QED Effect on Black Hole Shadow
- Testing dynamical torsion effects on the charged black hole's shadow, deflection angle and greybody with M87* and Sgr. A* from EHT
- Shadows and rings of the Kehagias-Sfetsos black hole surrounded by thin disk accretion
- Investigating the Connection between Generalized Uncertainty Principle and Asymptotically Safe Gravity in Black Hole Signatures through Shadow and Quasinormal Modes
- Quasiperiodic oscillations, weak field lensing and shadow cast around black holes in Symmergent gravity
- Probing the Lorentz Symmetry Violation Using the First Image of Sagittarius A*: Constraints on Standard-Model Extension Coefficients
- Testing Symmergent gravity through the shadow image and weak field photon deflection by a rotating black hole using the M87 and Sgr. A results
- Black hole in quantum wave dark matter
- Black hole surrounded by the pseudo-isothermal dark matter halo
- Constraints on charged Symmergent black hole from shadow and lensing
- Deflection angle and shadow of the Reissner-Nordström black hole with higher-order magnetic correction in Einstein-nonlinear-Maxwell fields
- Shadow and deflection angle of asymptotic, magnetically-charged, non-singular black hole
- Superentropic AdS Black Hole Shadows
- Shadows, rings and optical appearance of a magnetically charged regular black hole illuminated by various accretion disks
- Nonlinearly charged black holes: Shadow and Thin-accretion disk
- Shadows of rotating Einstein-Maxwell-dilaton black holes surrounded by a plasma
- Rotating black hole mimicker surrounded by the string cloud
- Quasinormal Modes and Optical Properties of 4-D black holes in Einstein Power-Yang-Mills Gravity
- Observational Signatures: Shadow cast by the effective metric of photons for black holes with rational non-linear electrodynamics
- Signatures of the accelerating black holes with a cosmological constant from the and shadow prospects
- Shadow of the Reissner-Nordström AdS Black Hole
- Light Deflection by Rotating Regular Black Holes with a Cosmological Constant
- GUP-corrected black holes: Thermodynamic properties, evaporation time and shadow constraint from EHT Observations of M87* and Sgr A*
- Ayón--Beato--García black hole coupled with a cloud of strings: thermodynamics, shadows and quasinormal modes
- Neutrino pair annihilation () in the presence of quintessence surrounding a black hole
- Dynamics of null particles and shadow for general rotating black hole
- Shadow thermodynamics of non-linear charged Anti-de Sitter black holes
- Light Deflection Angle by Superentropic Black Holes
- Deflection Light Behaviors by AdS Black Holes
- Optical Shadows of Rotating Bardeen AdS Black Holes
- Superentropic Black Hole Shadows in Arbitrary Dimensions
- Topological dyonic black holes of massive gravity with generalized quasitopological electromagnetism
- Regular Black Hole Models in the Transition from Baryonic Matter to Quark Matter
- Shedding Light on Gravity: Black Hole Shadows and Lensing Signatures in Lorentz Gauge Theory
- Asymptotically-Flat Black Hole Solutions in Symmergent Gravity
- Thermodynamics, Shadow, and Quasinormal Modes of AdS Ayón--Beato--García Massive Black Hole
- Analytical approach for calculating shadow of dynamical black hole
- Probing Weak-Force Corrections to Black Hole Geometry via Long Range Potentials: Feinberg-Sucher and Ferrer-Nowakowski Potentials