pith:N5252DUE
General orbital perturbation theory in Schwarzschild space-time
General relativistic Gaussian equations govern the evolution of osculating orbital elements in Schwarzschild spacetime under arbitrary perturbing forces.
arxiv:2601.16887 v2 · 2026-01-23 · gr-qc
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Claims
We derive general relativistic Gaussian equations for osculating elements for orbits under the influence of a perturbing force without any restrictions in an underlying Schwarzschild space-time.
That osculating orbital elements remain well-defined and their evolution follows Gaussian-type equations in full general relativity for arbitrary perturbing forces, with linear approximation sufficient for the Kerr and q-metric examples.
Derives unrestricted general relativistic Gaussian perturbation equations for osculating orbital elements in Schwarzschild spacetime, with linear solutions for Kerr and q-metric perturbations that recover Lense-Thirring precession.
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| First computed | 2026-05-17T23:39:00.189889Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
6f75dd0e84f21c68acb27f75c89b17c83e183c11570d1bed4b1f3e07b1693cdb
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/N5252DUE6IOGRLFSP524RGYXZA \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
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Canonical record JSON
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