On the acoustic accelerating Schwarzschild black hole: Solutions, thermodynamics and stability
This study investigates the characteristics of acoustic black holes when acceleration is present. The Schwarzschild metric, a fundamental solution in general relativity, is altered to account for the effects of acceleration on acoustic perturbations. The acceleration parameter significantly changes the acoustic horizon, a key characteristic of acoustic black holes. The findings show that the acceleration parameter destabilizes the acoustic black hole, causing unstable modes to form.
Authors
- M. Chacha
- H. Lekbich (ORCID: https://orcid.org/0009-0009-6079-0394)
- Abdellah Benami (ORCID: https://orcid.org/0000-0001-5516-5660)
- N. Mansour (ORCID: https://orcid.org/0000-0002-9993-8714)
- A. El Boukili (ORCID: https://orcid.org/0000-0002-3277-9640)
- N. Ouadoudi
- I. Ezzaki
Publication Details
- Journal
- Modern Physics Letters A
- Published
- 2025-05-15
- DOI
- https://doi.org/10.1142/s0217732325500816
- Citations
- 1
- Primary Topic
- Quantum Electrodynamics and Casimir Effect
- Type
- article
- Field-Weighted Citation Impact
- 1.25