The Hodograph Transform Between Thermodynamics and Relativity

Contact-Geometric Hodograph Transform: A Duality Between Thermodynamics and Relativity

Contact Geometry and Spaces of Light Rays

This paper develops a technical bridge between the geometric structures underlying general relativity and the formalism of equilibrium thermodynamics, leveraging the machinery of contact geometry. The central construct is the sky of an event in Minkowski spacetime, defined as the set of all incoming light rays, which the paper identifies as a Legendrian submanifold of the spherical cotangent bundle $S^*\mathbb{H}$ over a chosen Cauchy hypersurface—specifically, the unit future hyperboloid $K$ in $\mathbb{R}^{1,2}$.

The author employs the hyperbolic hodograph transform $\mathcal{H}$, a contactomorphism from the jet space $J^1S^1$ to $S^*\mathbb{H}$. This transform associates the space of lightlike geodesics in spacetime directly with the geometric mechanics formalism of thermodynamics. The relevance of the hyperboloid as the hypersurface is underscored by the natural identification between spacetime points and observer four-velocities, allowing photon energies and Busemann functions to coincide and making the thermodynamic interpretation precise.

Accelerated Observers, Doppler Effect, and Skies

Focusing on an observer undergoing uniform proper acceleration $a$ on $K$, the work explicitly constructs the observer's worldline and analyzes the associated evolution of skies. Key to this analysis is the Busemann function $b_q(x)$, encoding the logarithmic energy profile of a photon direction $q$ as measured by an observer at $K$0. This leads to the interpretation $K$1 as a Doppler-shifted energy, with the Busemann function yielding $K$2.

Applying the hodograph transform, the sky evolves under Lorentzian transport, and its preimage in the jet space is described by a generating function $K$3. The work provides a closed-form for $K$4 in terms of the observer's proper time, acceleration, and photon direction, demonstrating that it is fundamentally tied to the relativistic Doppler effect seen by the accelerating observer.

Free Energy Interpretation and Unruh Scaling

The main result is the re-interpretation of the Legendrian generating function $K$5 as a reduced free energy in a thermodynamic phase space. The function encodes the energy and entropy profiles for a putative thermodynamic system governed by the relativistic Doppler shift. With a Lorentzian rescaling motivated by the structure of the Unruh effect, the author extracts an effective temperature $K$6 from $K$7 via the thermodynamic relation between free energy and temperature. The scaling is found to be $K$8, matching the linear acceleration dependence of the Unruh temperature, though the numerical coefficient is distinct from $K$9.

This identification is technically nontrivial. The small-time expansion of $\mathbb{R}^{1,2}$0 reveals the Doppler energy as an affine correction, with the proportionality constant in the temperature extraction depending on the chosen energy normalization. The analysis delineates how the entropy content (in the thermodynamic analogy) is proportional to the Lorentz boost parameter $\mathbb{R}^{1,2}$1, further reinforcing the duality between causal (relativistic) and thermodynamic processes.

Statistical Mechanics Model and Analogs

Advancing the thermodynamic analogy, the author considers a randomization of the acceleration direction (modeled as a von Mises distribution on $\mathbb{R}^{1,2}$2), constructing the partition function and reduced free energy $\mathbb{R}^{1,2}$3 for the resulting statistical system. The explicit calculation produces a free energy whose leading order corresponds to the Doppler-shifted energy profile, confirming the identification of the hodograph-generated function as a genuine thermodynamic potential.

For comparison, the classical statistical mechanics of a rotor in an external field (with partition function involving $\mathbb{R}^{1,2}$4 Bessel functions) is shown to reproduce the leading directional dependence of the photon free energy in this model, up to a $\mathbb{R}^{1,2}$5-independent term. This establishes a precise correspondence between the thermodynamic abstraction and classical mechanical systems.

Higher-Dimensional Generalization

The hyperbolic hodograph formalism and the free energy interpretation generalize to higher dimensions, with the contactomorphism between $\mathbb{R}^{1,2}$6 and $\mathbb{R}^{1,2}$7 and the structural features of the causal-thermodynamic duality remaining intact.

Implications and Future Prospects

The work rigorously formalizes an instance of the long-appreciated analogy between statistical thermodynamics and relativistic causal structure, grounding it in the language of contact geometry and symplectic topology. By exhibiting explicit Legendrian correspondences, it clarifies the role of symplectic and contact structures in encoding equilibrium processes both in relativity and thermodynamics.

The theoretical implications extend to the understanding of temperature in accelerated frames and may provide a geometric pathway to reinterpreting quantum field theoretic results (Unruh effect) via classical geometric mechanics. The contact-geometric perspective may also motivate new invariants or dualities in mathematical physics, potentially informing future research in quantum gravity, black hole thermodynamics, and the topological classification of thermodynamic processes.

Conclusion

This paper establishes a contact-geometric duality connecting Minkowski skies (Legendrian submanifolds) and thermodynamic free energies through the hyperbolic hodograph transform. It provides explicit constructions and calculations for accelerated observers, interprets the directional Doppler profiles as free energies, derives an emergent temperature scaling with acceleration, and connects the geometric formalism to statistical mechanics. The work highlights the utility of contact geometry in unified descriptions of space-time causality and equilibrium thermodynamics, inviting further exploration of geometric dualities in mathematical physics.