Mixed Materials

Noncommutative quasinormal modes of Schwarzschild black hole

Bibliographic Details
Title: Noncommutative quasinormal modes of Schwarzschild black hole
Additional Titles: We study gravitational perturbations of the Schwarzschild metric in the context of noncommutative gravity. $r-φ$ and $r-t$ noncommutativity are introduced through a Moyal twist of the Hopf algebra of diffeomorphisms. Differential geometric structures such as curvature tensors are also twisted. Noncommutative equations of motion are derived from the recently proposed NC vacuum Einstein equation. Here, in addition to previously calculated axial NC potential, we present the polar solution which generalizes the work done by Zerilli. Quasinormal mode frequencies of the two potentials are calculated using three methods: WKB, Pöschl-Teller and Rosen-Morse. Notably, we apply the WKB method up to the 13th order and determine the optimal order for each noncommutative parameter value individually. Additionally, we provide comprehensive error estimations for the higher-order WKB calculations, offering insights into the accuracy of our results. By comparing the spectra, we conclude that the classical isospectrality of axial and polar modes is broken upon spacetime quantization. Isospectrality is restored in the eikonal limit.
Authors: Herceg, Nikola, Jurić, Tajron, Kumara, A. Naveena, Samsarov, Andjelo, Smolić, Ivica
Publisher Information: 2024-09-02 2025-04-16
Document Type: Mixed materials
Abstract: 38 pages, 6 figures, 23 tables; improved version, typos corrected, references added
Index Terms: General Relativity and Quantum Cosmology, High Energy Physics - Theory, text
DOI: 10.1007.JHEP05(2025)083
URL: http://arxiv.org/abs/2409.01402
Availability: Open access content. Open access content
Other Numbers: COO oai:arXiv.org:2409.01402
J. High Energ. Phys. 2025, 83 (2025)
doi:10.1007/JHEP05(2025)083
1455252570
Contributing Source: CORNELL UNIV
From OAIster®, provided by the OCLC Cooperative.
Accession Number: edsoai.on1455252570
Database: OAIster
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