(A6) χis obtained by expanding in large- ˆJthe integrand (A3), and integrating then overrorder by order

Massive probe In general, one starts from a 4D-reduced TS metric[14, 20–34] ds2|4D =−f(r)dt 2 + dr2 f(r) 1− 2M r α +r 2(dθ2 + sin2 θdϕ2),(A1), writes the mass shell condition in Hamiltonian form for a massive probe as H(xα, pα) =−µ 2 ,(A

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

gr-qc · 2025-06-17 · conditional · novelty 6.0

For Topological Stars, the eikonal-limit renormalized angular momentum is expressed as hypergeometric functions tied to the null geodesic radial action, generalizing the Schwarzschild resummation.

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Topological Stars and scalar wave equation: Exact resummation of the renormalized angular momentum in the eikonal limit gr-qc · 2025-06-17 · conditional · none · ref 3
For Topological Stars, the eikonal-limit renormalized angular momentum is expressed as hypergeometric functions tied to the null geodesic radial action, generalizing the Schwarzschild resummation.

(A6) χis obtained by expanding in large- ˆJthe integrand (A3), and integrating then overrorder by order

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