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.
Let us introduce an orthonormal frame adapted to the static observers (4.16) eˆt = u = 1√−gtt ∂t , e ˆr = 1√grr ∂r , e ˆθ = 1√gθθ ∂θ , e ˆφ = 1√gφφ ∂φ , e ˆy = 1√gyy ∂y
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.