An analytic, large-angular-momentum scattering angle for unbound geodesics and scalar self-force in Topological Star spacetime, with an unresolved regulator in the conservative self-force piece.
(4.10) The associated Kretschmann invariant is (2)Kt−r = Rαβγδ Rαβγδ = r2 s (4r − 5rb)2 4r8 , (4.11) showing a geometrical role for the radius r = 5 4 rb
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Scattering angle in a Topological Star spacetime: a self-force approach
An analytic, large-angular-momentum scattering angle for unbound geodesics and scalar self-force in Topological Star spacetime, with an unresolved regulator in the conservative self-force piece.