pith:2GGEPGYI
Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes
External quadrupolar distortion imprints clear changes on orbital dynamics and the structure of thin accretion disks around slightly deformed compact objects.
arxiv:2605.13890 v1 · 2026-05-12 · gr-qc · astro-ph.HE · hep-th
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Claims
We show that the external quadrupolar distortion leaves a clear imprint on both orbital dynamics and accretion structure. We further find that the outer edge of the radiating region is closely tied to the transition between radiation pressure and gas pressure dominance.
The local solution remains self-consistent over a physically meaningful radial domain, and the chosen exact vacuum spacetime accurately represents a slightly deformed compact object immersed in an external quadrupolar field.
External quadrupolar distortion imprints on orbital dynamics and accretion structure in thin disks around deformed compact objects, with the radiating region's outer edge tied to the radiation-to-gas pressure transition.
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| First computed | 2026-05-17T23:39:19.074613Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
d18c479b08f586528d90a081f41205b46cae54bf562fea3137857c9f18b84d0e
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/2GGEPGYI6WDFFDMQUCA7IEQFWR \
| jq -c '.canonical_record' \
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Canonical record JSON
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