Economic thermodynamics and inflation
İdris Demir, Ali İhsan Keskin
TL;DR
The paper addresses the challenge of explaining inflationary dynamics across regimes from hyperinflation to stable low inflation using a thermodynamic, Raychaudhuri-inspired framework. It models inflation as a scalar economic field with dynamics governed by a continuity equation and the Raychaudhuri equation, comparing adiabatic (δQ ≈ 0) and non-adiabatic (δQ ≠ 0) cases. Key findings show that adiabatic paths struggle to reach equilibrium, while non-adiabatic energy inflows can drive the system toward a stable balance (K=V) on timescales of about a decade, consistent with observed inflation cycles; hyperinflation can emerge for γ ≈ -1, with inflation slowing as the system evolves. The work provides a phenomenological, geometry-inspired lens connecting monetary policy and production continuity to thermodynamic-like balance, suggesting policy emphasis on controlled monetary flow and real production to achieve macroeconomic stability.
Abstract
This study presents a computational and theoretical framework inspired by thermodynamic principles to analyze the dynamics of economic inflation within adiabatic and non-adiabatic systems. In a framework referred to as developmental symmetry, inflation is formulated as a scalar field evolving through continuity equations, drawing an analogy with the Raychaudhuri equation in gravitational dynamics. The results show that adiabatic systems fail to reach equilibrium, while non-adiabatic systems can evolve toward stable states over time. The model successfully reproduces observed inflationary regimes-from hyperinflation to stable low-inflation phases-with characteristic transition periods of about a decade. These results indicate that production continuity and controlled monetary flow are crucial for achieving stability in complex economic systems, linking thermodynamic balance to macroeconomic equilibrium.
