Physics prides itself on the elegance of general relativity. The theory is often said to reveal the true architecture of spacetime: curvature as gravity, geodesics as free fall, geometry as destiny. And yet, this triumphal narrative masks a deeper confusion—one that sits squarely within the relational pathology traced throughout this series.
The conflation is simple to state and devastating in consequence:
The geometry of the equations is treated as the geometry of the cosmos.
This post exposes how the formalism over-inclines the construal, locking physics into a narrow way of carving possibility that makes singularities not inevitable features of the universe, but predictable artefacts of a particular geometric commitment.
1. The Riemannian commitment: a perspectival narrowing posing as revelation
General relativity begins with a decisive choice: spacetime is represented as a differentiable manifold equipped with a metric tensor of Lorentzian signature and a Levi-Civita connection.
This framework already embeds:
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smoothness assumptions,
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locality assumptions,
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metric primacy,
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differentiable structure down to arbitrarily fine scales,
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and a commitment to curvature as the fundamental diagnostic of relationality.
But once the formalism is adopted, physics performs the familiar reversal:
The model’s inclination becomes the world’s ontology.
Thus curvature becomes “real,” smoothness becomes “fundamental,” and geodesic incompleteness becomes “the universe collapsing into a singularity.”
2. Over-inclination: when the geometry overcommits
If earlier posts dealt with openness or closure, GR introduces a distinct pattern: over-inclination, where the chosen orientation of the mathematics is so specific, so rigid, and so all-encompassing that it constrains the kinds of phenomena the model can recognise.
Over-inclination shows up in several ways:
a. The metric as totalising structure
b. Smoothness as an unquestioned foundation
c. Curvature as the only admissible relational dynamism
Once these commitments are made, the path to singularities is already paved.
3. Singularities as artefacts of geometric commitment
Every physicist knows the standard line:
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singularities are “regions where curvature diverges,”
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or “places where spacetime ends,”
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or “boundaries of physics.”
A singularity in GR does not mean:
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spacetime literally pinches off,
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physical quantities grow without bound,
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the universe collapses into metaphysical incoherence.
It means simply:
the Riemannian construal has exceeded the range of its own inclination.
The model overcommits to smoothness, overcommits to metric continuity, and overcommits to curvature as the mediator of gravitation. When the phenomenon cannot be articulated within that orientation, the model fails—catastrophically, but predictably.
4. The misleading rhetoric of “geodesic incompleteness”
But geodesic incompleteness is a failure of geometric continuation, not physical continuation.
The model says:
“I cannot extend my geodesics any further.”
Physics then interprets this as:
“The universe cannot extend any further.”
5. Disentangling the shape of equations from the shape of the world
To restore clarity, we must make the relational boundary explicit:
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The shape of spacetime is not what the equations describe.
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It is what the phenomenon affords once cut through the construal that generates spacetime as a modelling category.
The cosmos is not obliged to honour the differential structure of the mathematics that depicts it.
6. What comes after Riemannian over-inclination?
This series does not advocate discarding GR; rather, it restores the theory to its rightful status:
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a sophisticated modelling practice,
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not a metaphysical revelation.
In doing so, it opens a more coherent path forward:
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recognising where over-inclination constrains intelligibility,
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rethinking the representational commitments embedded in geometric formalisms,
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and building models where the relational cut is allowed to reorient rather than calcify.
Next: Post 7 — The Myth of Mathematical Transparency
We bring these illusions into full view.
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