Black hole horizons and quantum charged particles
arXiv:1410.0509 · doi:10.1088/0264-9381/32/13/132001
Abstract
We point out a structural similarity between the characterization of black hole apparent horizons as stable marginally outer trapped surfaces (MOTS) and the quantum description of a non-relativistic charged particle moving in given magnetic and electric fields on a closed surface. Specifically, the spectral problem of the MOTS-stability operator corresponds to a stationary quantum particle with a formal fine-structure constant of negative sign. We discuss how such analogy enriches both problems, illustrating this with the insights into the MOTS-spectral problem gained from the analysis of the spectrum of the quantum charged particle Hamiltonian.
arXiv comment5 pages, no figures
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Cited by in corpus (14)
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- Ultimate fate of apparent horizons during a binary black hole merger II: Horizons weaving back and forth in time
- Horizons in a binary black hole merger I: Geometry and area increase
- A perspective on Black Hole Horizons from the Quantum Charged Particle
- Symmetry and instability of marginally outer trapped surfaces
- Complex magnetic fields: An improved Hardy-Laptev-Weidl inequality and quasi-self-adjointness
- Horizon area bound and MOTS stability in locally rotationally symmetric solutions
- Eigenvalues of the MOTS stability operator for slowly rotating Kerr black holes
- Marginally Outer Trapped Tori in Black Hole Spacetimes
- Ultimate fate of apparent horizons during a binary black hole merger I: Locating and understanding axisymmetric marginally outer trapped surfaces
- On the Stability of MOTS
- The gravitational Field of a massless Particle on the Horizon of a stationary Black Hole
- Cylindrical first order superintegrability with complex magnetic fields