Relativistic Hamiltonian as an emergent structure from information geometry
Sikarin Yoo-Kong
TL;DR
The paper addresses how relativistic kinematics can emerge from non-relativistic, multiplicative Hamiltonians by statistically fluctuating an auxiliary parameter β and applying the maximum-entropy principle. It reframes the β-family of Hamiltonians as a statistical manifold endowed with the Fisher–Rao metric, and shows that scale-invariant constraints (⟨1/β^2⟩ and ⟨ln β⟩) uniquely determine the β-distribution ρ(β) ∝ β^-4 e^{-1/β^2}, leading, upon ensemble averaging, to the relativistic form ⟨H⟩ = sqrt(p^2 c^2 + m^2 c^4) with c^2 = 2λ^2. The information-geometric structure explains the invariance and the logarithmic geometry that underpins the square-root dispersion, without assuming Lorentz symmetry a priori. This work links multiplicative dynamics, entropy-based inference, and statistical-manifold geometry to show how relativistic dispersion can be an emergent, inference-driven outcome with potential extensions to more complex kinematics and spacetime contexts.
Abstract
We show that the relativistic energy-momentum relation can emerge as an effective ensemble-averaged structure from a multiplicative Hamiltonian when fluctuations of an auxiliary parameter are treated using maximum entropy inference. The resulting probability distribution is uniquely fixed by scale-invariant constraints, which are shown to arise naturally from the Fisher-Rao geometry of the associated statistical manifold. Within this information-geometric framework, the relativistic dispersion relation appears without initially imposing Lorentz symmetry, but as a consequence of statistical averaging and geometric invariance.
