Quasinormal Modes in Noncommutative Schwarzschild black holes
arXiv:2301.09147 · doi:10.1016/j.nuclphysb.2024.116545
Abstract
We investigate the quasinormal modes of a massless scalar field in a Schwarzschild black hole, which is deformed due to noncommutative corrections. We introduce the deformed Schwarzschild black hole solution, which depends on the noncommutative parameter . We then extract the master equation as a Schrödinger-like equation, giving the explicit expression of the effective potential which is modified due to the noncommutative corrections. After that, we solve the master equation numerically. The significance of these results is twofold. Firstly, our results can be related to the detection of gravitational waves by the near future gravitational wave detectors, such as LISA, which will have a significantly increased accuracy. In particular, these observed gravitational waves produced by binary strong gravitational systems have oscillating modes which can provide valuable information. Secondly, our results can serve as an additional tool to test the predictions of GR, as well as to examine the possible detection of this kind of gravitational corrections.
15 pages, 7 figures
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- Effects of gravity rainbow on scalar bosonic and oscillator fields in Bonnor-Melvin space-time with a cosmological constant
- Higher-dimensional quantum Oppenheimer-Snyder model
- A Non-Commutative Kalb-Ramond Black Hole
- Geodesics, accretion disk, gravitational lensing, time delay, and effects on neutrinos induced by a non-commutative black hole
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- Non-commutativity in Hayward spacetime
- Quasinormal modes of charged BTZ black holes
- Noncommutative quasinormal modes of Schwarzschild black hole
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- Lyapunov exponents and geodesic stability of Schwarzschild black hole in the non-commutative gauge theory of gravity
- Imprints of non-commutativity on charged black holes