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IndisputableMonolith.Relativity.Geometry.ParallelTransport

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ParallelTransport module defines smooth curves in 4D spacetime and parallel transport of vector fields along them, including initial conditions, solutions, and flat-space preservation lemmas. It would be cited by researchers deriving holonomy from curvature in Recognition Science relativity models. The module assembles definitions and basic lemmas atop tensor, metric, and curvature imports without a central theorem.

claimA spacetime curve $C: I → M^4$ parameterized by affine parameter $λ$, with parallel transport of a vector field $V$ satisfying $∇_{C'} V = 0$ where $∇$ is the Levi-Civita connection from the metric $g_{μν}$ and its Christoffel symbols.

background

The module sits inside Relativity.Geometry and imports standard basis vectors $e_μ$ from Derivatives, Christoffel symbols from Curvature, and tensor operations from Tensor and Metric. It introduces SpacetimeCurve as a smooth curve in 4D spacetime parameterized by λ, together with ParallelTransported fields, ParallelTransportIC, and ParallelTransportSolution. Sibling objects include ClosedLoop, HolonomyDefect, and flat-space cases such as parallel_transport_flat and no_holonomy_if_flat.

proof idea

This is a definition module, no proofs.

why it matters in Recognition Science

Supplies the geometric primitives re-exported by the parent IndisputableMonolith.Relativity.Geometry aggregator. It supports downstream holonomy-curvature correspondence results such as HolonomyCurvatureCorrespondence and no_holonomy_if_flat, connecting the metric layer to observable transport along curves in the Recognition framework.

scope and limits

used by (1)

From the project-wide theorem graph. These declarations reference this one in their body.

depends on (4)

Lean names referenced from this declaration's body.

declarations in this module (14)