First-principles analysis unifies quantum, thermal, and geometric theories, indicating new insights on black hole thermodynamics.
We present a first-principles derivation of a unified field theory that combines quantum dynamics, thermal field theory, and two-dimensional quantum gravity within a single holomorphic framework. The fundamental object is a complex time manifold M---a compact Riemann surface with local coordinate z = τ/P + i t/P, where P is the Planck time. The quantum state is a holomorphic section Ψ(z) of a line bundle over M, and the geometry is encoded in a K\"ahler metric ds² = Ω²(z,z̄)\,dz dz̄. Starting from the principle of least action, general covariance on M, and the correspondence principle, we construct the total action S = SEH + Sₘₐₜₜₑᵣ + Sᵢₙₜ. Variation yields a coupled system: a modified wave equation for Ψ that reduces to the Schr\"odinger equation in the flat limit, and a Liouville equation for Ω that encodes the feedback of quantum information on geometry. The KMS condition emerges as a natural boundary condition from the compactification of the imaginary time direction. We show that in the semi-classical limit, the theory reproduces the thermodynamics of black holes and predicts a fundamental decoherence mechanism with rate Γ ~ G m² (Δ x)² kB T /. The mathematical consistency of the framework is established through spectral analysis of the Laplace-Beltrami operator and the construction of exact solutions in constant curvature backgrounds.
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Y. Li (2026) studied this question.
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