Acoustic black holes in curved spacetime and emergence of analogue Minkowski metric
arXiv:1902.11126 · doi:10.1103/PhysRevD.99.104047
Abstract
Gravity is not only able to be mimicked in flat spacetimes, but also in curved spacetimes. We study analogue gravity models in curved spacetime by considering the relativistic Gross-Pitaevskii theory and Yang-Mills theory in the fixed background spacetime geometry. The results show that acoustic metrics can be emergent from curved spacetimes yielding a Hadamard product of a real metric-tensor and an analogue metric-tensor. Taking \emph{quantum vortices} as \emph{test particles}, we evaluate their released energy ratio during the "gravitational binding". The -dimensional flat Minkowski metric is derived from the -dimensional Anti-de Sitter space by considering perturbations of the Yang-Mills field, which implies that Minkowski spacetime can be also simulated and the derivations presented here have some deep connections with the holographic principle.
17 pages, 3 tables, 1 figure, references added
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- On the geometry outside of acoustic black holes in -dimensional spacetime
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- Petrov classification of analogue spacetimes
- Analogue gravity and the island prescription
- Hawking radiation and stability of the canonical acoustic black holes
- Analogue metric in a black bounce background
- Modified metrics of acoustic black holes: A review
- Entangling superconducting qubits through an analogue wormhole
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- A `Third' Quantization Constructed for Gauge Theory of Gravity
- Thin accretion disks around a Schwarzschild acoustic black hole
- Scrambling time for analogue black holes embedded in AdS space
- Holographic superfluid sound modes with bulk acoustic black hole