Published June 4, 2026 | Version v1
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The Curvature of Process: Gravitational Dynamics as an Emergent Consequence of the Modular Automorphism Group of End(X) A Spectral-Triple Formulation

  • 1. ROR icon Université de Saida Dr Moulay Tahar

Description

We present a rigorous framework for the emergence of gravitational geometry from
the algebraic structure of temporal flow. Our approach proceeds in four interlocking
steps. (1) Algebraic time. Time is identified with the modular automorphism
group σω ∈ Aut(A) of a von Neumann algebra A = End(X) equipped with a faith- ful normal state ω, 
following the Tomita–Takesaki theory. (2) Spectral geometry.
Geometric data are encoded not directly in A, but in a spectral triple (A, H, D) where
D is a Dirac-type operator whose spectrum encodes distances, volumes, and curva-
ture. The modular operator ∆ω is shown to constrain the admissible Dirac operators
in a canonical way. (3) Action principle. The physical action is the Spectral Action
of Chamseddine and Connes, S(D) = Tr f (D/Λ) , whose asymptotic heat-kernel expansion provably 
contains the Einstein–Hilbert term as its leading geometric con
tribution. This replaces the previously ad-hoc action functional and converts the
semiclassical limit into a mathematical theorem rather than a hopeful coincidence.
(4) Gravitational fluctuations. Gravity is identified with the non-trivial inner
fluctuations of the metric, D '→ D + A + JAJ −¹, where A is a self-adjoint element of Ω             
                   uctuations—classified
by t      ild cohomology class [Fδ  ] ∈ HH²(A, A)—is identified with the in-
trinsic gravitational degree of freedom. In the commutative limit A → C∞(M ) the
spectral action reduces precisely to the Einstein–Hilbert action plus a cosmological
term, recovering general relativity. Quantum corrections are controlled by higher
Hochschild cohomology groups HHⁿ(A, A), n ≥ 3, and vanish as ℏ → 0.

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