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A class of rotating metrics in the presence of a scalar field

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arxiv 2307.13588 v3 pith:FSRR7KXU submitted 2023-07-25 gr-qc hep-th

classification gr-qchep-th
keywords metricsrotatingmetriccertainclassgammaobtainparameters
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abstract

We consider a class of three parameter static and axially symmetric metrics that reduce to the Janis-Newman-Winicour (JNW) and $ \gamma$-metrics in certain limits of the parameters. We obtain rotating form of the metrics that are asymptotically flat, stationary and axisymmetric. In certain values of the parameters, the solutions represent the rotating JNW metric, rotating $ \gamma$-metric and Bogush-Gal'tsov (BG) metric. The singularities of rotating metrics are investigated. Using the light-ring method, we obtain the quasi normal modes (QNMs) related to rotating metrics in the eikonal limit. Finally, we investigate the precession frequency of a test gyroscope in the presence of the rotating metrics.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Orbital Motion in Spacetimes Influenced by the Presence of Scalar and Electromagnetic Fields

    gr-qc 2025-01 conditional novelty 6.0 of 10

    Strong scalar fields around naked singularities can create stable circular orbits, and charged scalar-field spacetimes can host both stable and unstable photon orbits.

  2. A class of charged-Taub-NUT-scalar metrics via Harison and Ehlers Transformations

    gr-qc 2025-01 reject novelty 4.0 of 10

    A proposed new family of charged Taub-NUT spacetimes with a theta-dependent scalar field, built via Harrison and Ehlers transformations, but the exact-solution claim is unsupported and internally inconsistent.

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