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Wedge modular bridge implies the Unruh clock temperature
An algebraic KMS statement for the vacuum state of the selected massive scalar right-wedge model, conditional on its adopted modular/boost bridge, and for one uniformly accelerated proper-time orbit. It asserts no detector response, particle production, observed temperature, Hawking effect, or density-matrix representation.
Statement
Assume the Axiom of Choice and the selected massive scalar wedge postulate. Use its metric , length coordinates , right wedge , vacuum , algebra , modular operator , first-variable-linear pairing from the postulate, and boost with dimensionless rapidity . Define the vector state for , the modular automorphisms , and for dimensionless . The proper-time curve for any in is where is measured in seconds. Its future-boost rapidity is . For this unit proper-time parametrization, define the proper-acceleration scalar by ; the theorem verifies . Define the proper-time action on by ; equivalently, it is conjugation by the future boost .
Then for every there is a bounded function , continuous on the closed strip and holomorphic inside, whose boundaries satisfy with strip width seconds. Under the physical-time convention that the strip width is , the associated inverse temperature and KMS temperature parameter are where is in and is in . This is a conditional algebraic model deduction; it does not assert a detector response, particle production, a thermal density matrix, or an observed temperature.
Statement references
Facts & Assumptions
Given: The Axiom of Choice; the selected wedge model and modular/boost interface; the stated uniformly accelerated orbit; and the positive constants with their SI units.
The Axiom of Choice is assumed as defined in The Axiom of Choice.
The selected model defines as the double commutant of the bounded scalar Weyl observables, assumes cyclic and separating for it, and adopts . The boost has future rapidity under the explicit matrix convention in the postulate. Free scalar wedge data and modular-geometric bridge
For standard modular data on a concrete von Neumann algebra, the Tomita–Takesaki theorem gives , a normal point-ultraweakly continuous automorphism group, and an upper-strip dimensionless KMS state for with width . It makes no norm-continuity claim for the whole von Neumann algebra. Tomita modular automorphisms and the upper-strip KMS condition
The local rescaling lemma rescales this upper-strip W*-KMS boundary condition directly: if with , the strip width becomes . Positive rescaling of an upper-strip W*-KMS flow
The framework units definition uses length coordinates , assigns units , units , and units . In its physical-time KMS convention, a strip width seconds corresponds to inverse temperature . Thermodynamics-GR fields, currents, reference normalization and units
Proof
Proof technique: Identify the future boost from the adopted sign convention, then rescale the modular KMS strip to the proper-time clock.
Given: [A1]–[A2], [F1]–[F3], , and .
By [A2], . Since , we have for . Thus is the future-boost action with rapidity ; the minus sign in the adopted modular identity is essential for this direction.
Put and differentiate the curve in the Statement. Then and . Direct contraction with gives and ; also . Therefore is proper time, the curve is future timelike with proper acceleration magnitude , and its boost rapidity is .
Let , which has seconds as its unit by [F3]. Then and, by step 1.1, . Apply [F1] and [F2] with dimensionless width : has the required bounded continuous upper-strip functions on width seconds for every . By [F3], and . The displayed units give and . No density matrix or detector statement is used.
Depends on
Dependency tree · 2 levels
Sources
- Joseph J. Bisognano and Eyvind H. Wichmann, On the duality condition for a Hermitian scalar field, Journal of Mathematical Physics 16 (1975), 985–1007
- Daniele Guido, Modular theory for the von Neumann algebras of local quantum physics, complete lecture notes, arXiv:0812.1511
- Edward Witten, Notes on Some Entanglement Properties of Quantum Field Theory, complete lecture notes, arXiv:1803.04993
- Stefan Hollands and Robert M. Wald, Quantum fields in curved spacetime, arXiv:1401.2026
- Robert M. Wald, The Thermodynamics of Black Holes, arXiv:gr-qc/9912119