Conserved reference energy
Differentiate final (2.27) with respect to both generalized velocities to obtain (2.28), then apply the Legendre transform; D>0.
Based on the final manuscript · Chapter 2
Differentiate final (2.27) with respect to both generalized velocities to obtain (2.28), then apply the Legendre transform; D>0.
Chapter reference: Final collected manuscript · Chapter 2 §IV.2 (2.28)—(2.31) · ASD-BOOK-ddbade997b45
Source and ID
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Return to premises and derivationAdopted source, conditions and previous versions
Final collected manuscript · Chapter 2 §IV.2 (2.28)—(2.31)
Differentiate final (2.27) with respect to both generalized velocities to obtain (2.28), then apply the Legendre transform; D>0.
Conditions retained in this adoption
- Fixed G₀; isolated, static, spherically symmetric, uncharged exterior.
- Areal radius, actual spatial length and reference optical path are defined separately.
- Weak-field perturbation, slow-rotation far field and boundary statistics each have separate conditions.
Specific unresolved source issues
- Microscopic source matching, dynamical strong fields and full boundary-state dynamics remain open.
Source locators: p0682 · p0694 · p0698 · p0701 · p0703 · p0705 · p0715 · p0717 · p0719 · p0730 · p0732 · p0779 · 最终合订稿 · 第二章 §四.2 (2.28)—(2.31)
Manuscript SHA-256: ddbade997b45913248e588953b1d27ccb9c7c206c3c8d992d3aef2364a64836e
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Previous source, retained as history
FND-3dde8d8e081d · 第二章 / Chapter 2 · (2.31) and unnumbered radial momentum, p. 13
Dependencies
inputOrbital action in a static backgroundASD-WEB-GRV-024inputOrbital velocity domainASD-WEB-GRV-026Uses of this equation
Subsequent equationFirst integral of the orbitASD-WEB-GRV-030DocumentOrbital Dynamics · Action, Conservation and Precession