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Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit

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arxiv 2506.14442 v1 pith:GJJKH5VG submitted 2025-06-17 gr-qc

Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit

classification gr-qc
keywords angularexactmomentumrenormalizedresummationtopologicalactionadmits
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We show that for a Topological Star the renormalized angular momentum parameter, $\nu$, appearing in the Mano-Suzuki-Takasugi-type or in the quantum-Seiberg-Witten-type approaches of the perturbation equations, has 1) a direct link with the geodesic radial action computed along the null orbits of the background and 2) admits an exact resummation in terms of hypergeometric functions, generalizing previous results valid in the Schwarzschild case, see Ref.[arXiv:2504.07862 [hep-th]].

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Cited by 3 Pith papers

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

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    In a curvature-coupled propagation framework for modified gravity, gravitational-wave lensing in wave optics shows persistent infrared interactions that prevent the amplification factor from approaching unity at zero ...

  2. 5d Schwarzschild-Tangherlini spacetime: MST-like formalism for a Reduced Confluent Heun Equation

    gr-qc 2026-07 accept novelty 7.0

    An original MST-like formalism is constructed for the reduced confluent Heun radial equation of 5D Schwarzschild-Tangherlini scalars, validated by matching the renormalized angular momentum to the quantum Seiberg-Witt...

  3. Gravitational Atoms from Topological Stars

    gr-qc 2025-11 unverdicted novelty 5.0

    Bound states of a massive scalar field around topological stars form strictly normal modes, producing a hydrogen-like spectrum when the Compton wavelength exceeds the star size and localized states otherwise.