Thermal quantum field theory
In theoretical physics, thermal quantum field theory (thermal field theory for short) or finite temperature field theory is a set of methods to calculate expectation values of physical observables of a quantum field theory at finite temperature.
In the
may be written as
The Matsubara formalism, also referred to as imaginary time formalism, can be extended to systems with thermal variations.[11][12] In this approach, the variation in the temperature is recast as a variation in the Euclidean metric. Analysis of the partition function leads to an equivalence between thermal variations and the curvature of the Euclidean space.[11][12]
The alternative to the use of fictitious imaginary times is to use a real-time formalism which come in two forms.[13] A path-ordered approach to real-time formalisms includes the Schwinger–Keldysh formalism and more modern variants.[14] The latter involves replacing a straight time contour from (large negative) real initial time to by one that first runs to (large positive) real time and then suitably back to .[15] In fact all that is needed is one section running along the real time axis, as the route to the end point, , is less important.[16] The piecewise composition of the resulting complex time contour leads to a doubling of fields and more complicated Feynman rules, but obviates the need of analytic continuations of the imaginary-time formalism. The alternative approach to real-time formalisms is an operator based approach using Bogoliubov transformations, known as thermo field dynamics.[13][17] As well as Feynman diagrams and perturbation theory, other techniques such as dispersion relations and the finite temperature analog of Cutkosky rules can also be used in the real time formulation.[18][19]
An alternative approach which is of interest to mathematical physics is to work with KMS states.
See also
References
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