pith:KFE42DCF
Photon Sphere and Shadow of a Perturbative Black Hole in $f(R,\mathcal{G})$ Gravity
Higher-curvature corrections in f(R,G) gravity shift the photon-sphere radius and alter black-hole shadow sizes.
arxiv:2605.10992 v2 · 2026-05-09 · gr-qc
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Claims
We derive analytic expressions for the shift in the photon-sphere radius and show that higher-curvature terms modify the location of unstable photon orbits, with the Gauss-Bonnet sector producing a more significant contribution than mixed curvature terms.
The analysis assumes that the coupling parameters are small enough for an asymptotic perturbative expansion around the Schwarzschild solution to remain valid throughout the strong-field region.
Perturbative higher-curvature corrections in f(R,G) gravity shift the photon-sphere radius and black-hole shadow size away from Schwarzschild values, with the Gauss-Bonnet sector contributing more than mixed terms.
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| First computed | 2026-05-20T00:03:17.236614Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5149cd0c4558a9290567124a79acfe31deb3ab327a283935b51cce57b32688e7
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/KFE42DCFLCUSSBLHCJFHTLH6GH \
| jq -c '.canonical_record' \
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Canonical record JSON
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