Partition function (quantum field theory)

In quantum field theory, partition functions are the generating functionals for all correlation functions, making them key objects of study in the path integral formalism. They are closely related to the partition function in statistical mechanics, where the latter are imaginary time versions of the former. Partition functions can rarely be solved for exactly, although free theories do admit such solutions. Instead, a perturbative approach to solving for partition functions gives rise to the familiar method of calculating correlation functions using Feynman diagrams.

Generating functional

Scalar theories

In a $d$ -dimensional field theory with a real scalar field $\phi$ and action $S[\phi ]$ , the partition function is defined in the path integral formalism to be^[1]

Z[J]=\int {\mathcal {D}}\phi \ e^{iS[\phi ]+i\int d^{d}xJ(x)\phi (x)}

where $J(x)$ is a fictitious source current. The function acts as a generating functional for arbitrary n-point correlation functions

G_{n}(x_{1},\dots ,x_{n})=(-1)^{n}{\frac {1}{Z[0]}}{\frac {\delta ^{n}Z[J]}{\delta J(x_{1})\cdots \delta J(x_{n})}}{\bigg |}_{J=0}.

The derivatives used here are functional derivatives rather than regular derivatives since they are acting on functionals rather than regular functions. From this it follows that an equivalent expression for the partition function reminiscent to a power series in source currents is given by^[2]

Z[J]=\sum _{n\geq 0}{\frac {1}{n!}}\int \prod _{i=1}^{n}d^{d}x_{i}G(x_{1},\dots ,x_{n})J(x_{1})\cdots J(x_{n}).

In curved spacetimes there is an added subtlety associated with the fact that the initial vacuum state need not be the same as the final vacuum state.^[3]

Knowing the partition function completely solves the theory since it allows for the direct calculation of all of its correlation functions. However, there are very few cases where the partition function can be calculated exactly. While free theories do admit exact solutions interacting theories generally do not. Instead the partition function can be evaluated at weak coupling which amounts to regular perturbation theory using Feynman diagrams.^[4]

By performing a Wick transformation, the partition function can be expressed in Euclidean spacetime as^[5]

Z[J]=\int {\mathcal {D}}\phi \ e^{-(S_{E}[\phi ]+\int d^{d}x_{E}J\phi )},

where $S_{E}$ is the Euclidean action and $x_{E}$ is the Euclidean coordinate. This form is closely connection to the partition function in statistical mechanics, especially since the Euclidean Lagrangian is generally bounded from below and thus can be interpreted as an energy. It also allows for the interpretation the exponential factor as a statistical weight for the field configurations, with larger fluctuations with gradients or field values leading to greater suppression. This connection with statistical mechanics also lends additional intuition for how correlation functions should behave in a quantum field theory.

References

^ Rivers, R.J. (1988). "1". Path Integral Methods in Quantum Field Theory. Cambridge: Cambridge University Press. p. 14-16. ISBN 978-0521368704.
^ Năstase, H. (2019). "9". Introduction to Quantum Field Theory. Cambridge University Press. p. 78. ISBN 978-1108493994.
^ Birrell, N.C.; Davis, P.C.W. (1984). "6". Quantum Fields in Curved Spacetime. Cambridge University Press. p. 155-156. ISBN 978-0521278584.
^ Srednicki, M. (2007). "9". Quantum Field Theory. Cambridge: Cambridge University Press. p. 58-60. ISBN 978-0521864497.
^ Peskin, Michael E.; Schroeder, Daniel V. (1995). "9". An Introduction to Quantum Field Theory. Westview Press. p. 289-292. ISBN 9780201503975.

Generating functional

Scalar theories

References

Further reading