Black hole image encoding quantum gravity information
arXiv:2302.02800 · doi:10.1103/PhysRevD.108.104004
Abstract
The quantum extension of the Kruskal spacetime indicates the existence of a companion black hole in the universe earlier than ours. It is shown that the radiations from the companion black hole can enter its horizon, pass through the deep Planck region, and show up from the white hole in our universe. These radiations inlay extra bright rings in the image of the black hole in our universe, and some of these rings appear distinctly in the shadow region. Therefore, the image of the black hole observed by us encodes the information of quantum gravity. The positions and widths of the bright rings are predicted precisely. The predictive values for supermassive black holes are universal for a quite general class of quantum-modified spacetimes with the phenomenon of black hole to white hole transition. Thus, our result opens a new experimental window to test this phenomenon predicted by quantum gravity.
arXiv comment6+6 pages, 6 figures, Fig. 6 and some relevant discussions is added
References in corpus (45)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- Formation and evaporation of non-singular black holes
- Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics
- Real Ashtekar Variables for Lorentzian Signature Space-times
- Gravitationally-induced entanglement between two massive particles is sufficient evidence of quantum effects in gravity
- Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A
- Black Hole Shadows, Photon Rings, and Lensing Rings
- Renormalization group improved black hole spacetimes
- Tests of Lorentz invariance: a 2013 update
- Dynamically Triangulating Lorentzian Quantum Gravity
- Lorentz invariance and quantum gravity: an additional fine-tuning problem?
- Quantum Transfiguration of Kruskal Black Holes
- Black hole fireworks: quantum-gravity effects outside the horizon spark black to white hole tunneling
- The causal set approach to quantum gravity
- Disappearance of Black Hole Singularity in Quantum Gravity
- Shadow and Quasinormal Modes of a Rotating Loop Quantum Black Hole
- Quantum Oppenheimer-Snyder and Swiss Cheese models
- Black holes in loop quantum gravity: the complete space-time
- Loop quantization of the Schwarzschild interior revisited
- Testing loop quantum gravity from observational consequences of non-singular rotating black holes
- Can Gravitons Be Detected?
- Influence of Quantum Correction on the Black Hole Shadows, Photon Rings and Lensing Rings
- Tests of Loop Quantum Gravity from the Event Horizon Telescope Results of Sgr A
- A model for non-singular black hole collapse and evaporation
- Shadow and stability of quantum-corrected black holes
- Spherically symmetric loop quantum gravity: analysis of improved dynamics
- Gravitational spin Hall effect of light
- Quantum gravity of dust collapse: shock waves from black holes
- On the geometry of the black-to-white hole transition within a single asymptotic region
- Loop quantum Schwarzschild interior and black hole remnant
- Properties of the spherically symmetric polymer black holes
- Photon Emission Near Extreme Kerr Black Holes
- Improved Effective Dynamics of Loop-Quantum-Gravity Black Hole and Nariai Limit
- Spherical symmetric gravitational collapse of a dust cloud: polymerized dynamics in reduced phase space
- Non-singular quantum gravitational dynamics of an LTB dust shell model: the role of quantization prescriptions
- Testing different approaches to quantum gravity with cosmology: An overview
- Multi-level images around Kerr-Newman black holes
- Causal Structure of a recent Loop Quantum Gravity Black Hole Collapse Model
- Loop Quantum Gravity Phenomenology: Linking Loops to Observational Physics
- Black hole state degeneracy in Loop Quantum Gravity
- Are physical objects necessarily burnt up by the blue sheet inside a black hole?
- Rainbow Oppenheimer-Snyder collapse and the entanglement entropy production
- From Causal Dynamical Triangulations To Astronomical Observations
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- Gravitational waveforms from periodic orbits around a quantum-corrected black hole
- Gravitational lensing effect of black holes in effective quantum gravity
- Circular orbits and thin accretion disk around a quantum corrected black hole
- Thermodynamics of AdS-Schwarzschild-like black hole in loop quantum gravity
- New black-to-white hole solutions with improved geometry and energy conditions
- The quasinormal modes, pseudospectrum and time evolution of Proca fields in quantum Oppenheimer-Snyder-de Sitter spacetime
- Is a photon ring invariably a closed structure?
- Imaging a semi-classical horizonless compact object with strong redshift
- Spin foam amplitude of the black-to-white hole transition
- Decoding quantum gravity information with black hole accretion disk
- Probing loop quantum effects through solar system experiments: observational signatures and parameter constraints
- The black hole shadow of quantum Oppenheimer-Snyder-de Sitter spacetime
- Investigating the shadows of new regular black holes with a Minkowski core: Effects of spherical accretion and core type differences
- Symmetric black-to-white hole solutions with a cosmological constant
- Thermodynamic phase transition and Joule-Thomson expansion of a quantum corrected black hole in AdS spacetime
- Circular orbits and accretion disk around a deformed-Schwarzschild black hole in loop quantum gravity
- Observational properties of black hole in quantum fluctuation modified gravity
- Thermal chaos of quantum-corrected-AdS black hole in the extended phase space
- Computing the graph-changing dynamics of loop quantum gravity
- Particle Deflections around Microscopic Loop Quantum Black Holes with Rigorous Quantum Parameters
- Image of a quantum-corrected black hole without Cauchy horizons illuminated by a static thin accretion disk
- Exploring black holes with multiple photon spheres by interferometric signatures
- Shadow of rotating black holes with consistent thermodynamics
- Black hole images as probes of thermodynamic evolution