Waves in the Griffiths-Podolsky Metric
Kartheek R Solipuram
TL;DR
This paper investigates wave perturbations in an accelerating black hole described by the Griffiths-Podolsky metric, utilizing spin coefficients to analyze wave behavior in such spacetime.
Contribution
It introduces a method to describe wave equations in the Griffiths-Podolsky metric using spin coefficients, extending black hole perturbation analysis to accelerating black holes.
Findings
Derived wave equations for the Griffiths-Podolsky metric
Analyzed wave behavior in accelerating black hole spacetime
Extended perturbation techniques to non-stationary black holes
Abstract
Perturbations form an important section of black hole analyses. This paper deals with the effect of perturbations as in the delineation of waves that occur. It makes use of the spin coefficients from [3] to represent the general equations of waves in an accelerating black hole proposed in [2].
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Nonlinear Waves and Solitons · Geophysics and Gravity Measurements