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A Complex Tension Origin for Dilaton Gravity: Jordan Stiffness and Logarithmic Einstein Dynamics
Michaël Vaillant1, Tony C Scott2
1Meta-Connexions, 234 Route de Seysses, 31100 Toulouse, France.
Entropy (Basel, Switzerland)
|May 26, 2026
Summary
This study identifies the dilaton with a stiffness mode, explaining the logarithmic scalar-tensor structure in dilatonic gravity. This provides a microphysical origin for scalar stiffness laws and offers testable predictions for gravity theories.
Area of Science:
- Theoretical Physics
- Quantum Gravity
- Cosmology
Background:
- Dilatonic gravity theories require a microphysical explanation for their scalar sector.
- Existing models lack a fundamental understanding of the dilaton's origin and behavior.
- Scalar-tensor theories are crucial for understanding gravity's fundamental properties.
Purpose of the Study:
- To provide a microphysical completion for the scalar sector of dilatonic gravity.
- To identify the dilaton with a specific physical mode within a discrete relational network.
- To derive the logarithmic scalar-tensor structure from fundamental principles.
Main Methods:
- Identifying the dilaton with the coarse-grained stiffness mode of a complex tension field.
- Applying controlled ordered-regime coarse-graining to a discrete relational network.
- Utilizing a Weyl map to establish the relationship between tension and the canonical scalar.
Main Results:
- The real projection of tension scales as Φ(Θ)=Φ0cosΘ, leading to a phase-dependent Planck mass.
- An emergent logarithmic structure for the Einstein-frame canonical scalar, φ∝ln[Φ(Θ)/Φ0].
- This structure aligns with vacuum models inspired by the Logarithmic Schrödinger Equation (LogSE).
Conclusions:
- A controlled microphysical origin for a specific scalar stiffness law (Φ(Θ)∝cosΘ) is established.
- The derived logarithmic canonical structure provides a foundation for specific scalar-tensor theories.
- The framework offers potential for satisfying Solar-System constraints and suggests avenues for experimental and astrophysical tests.
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