Axial Gravitational Normal Modes of Uniform Density Star in Anti-de Sitter Spacetime
Kai Lin, Alan B. Pavan, Amilcar Rabelo de Queiroz, Elcio Abdalla

TL;DR
This paper investigates axial gravitational perturbations of uniform density stars in Anti-de Sitter spacetime, revealing standing wave behaviors, echo phenomena at the star surface, and wave dispersion due to potential well confinement.
Contribution
It introduces a novel analysis of gravitational wave behavior in AdS spacetime using numerical methods, highlighting standing waves and echoes caused by the potential well structure.
Findings
Standing wave patterns for modes n=0,1,2 identified.
Echo phenomena observed at the star surface.
Wave packets disperse after multiple reflections.
Abstract
The article studies the dynamical behavior of axial gravitational perturbations of homogeneous stars in Anti-de Sitter spacetime. Because the radial coordinate transforms into the tortoise coordinate , obeying and , the tortoise coordinates domain is finite, and the gravitational waves fail to reach out of the domain. Thus, from the perspective of tortoise coordinates, the perturbation equation of uniform density stars in Anti-de Sitter spacetime is analogous to the infinite deep potential well in quantum mechanics. Therefore, the perturbative behavior in this spacetime represents a standing wave vibration. Here we use shooting method and finite difference method to show the imagery of standing waves in this spacetime for as examples. On the other hand, by finite difference method, a Gaussian wave packet…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Cosmology and Gravitation Theories · Astrophysical Phenomena and Observations
