Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2015/iii/paper-43/1/solution

Use natural units and the Minkowski metric . A real scalar field assigns a real variable to each spatial point. Its Lagrangian density can be taken to be
The principle of stationary action gives the Euler-Lagrange equation . With , this is the Klein-Gordon equation. An additional nonlinear part of describes interactions.
The canonical momentum is . The Legendre transform in mechanics gives the canonical Hamiltonian density of a real scalar field
The Hamiltonian equations and recover the same field equation. In canonical quantization, the fields become operators satisfying the equal-time canonical commutation relations
A spatial lattice makes the analogy with many coupled quantum-mechanical coordinates precise. Each lattice field value is a coordinate, with its own conjugate momentum. The path integral is another representation of the same quantum evolution.
To see its origin, first consider one coordinate with . Split a time interval into steps of length and insert position and momentum resolutions of the identity. The short-time kernel is
Multiplying the kernels and integrating over intermediate positions gives the phase-space path integral
The endpoints of are fixed. The momentum integrals are Gaussian integrals; completing the square produces the configuration-space path integral
At finite slicing its normalization contains . This fixes the composition law and the initial delta-function kernel. One sums over all paths, not merely solutions of the classical equation. Restoring replaces the weight by ; stationary phase explains the emergence of classical trajectories.
For the field, use scalar field configuration eigenstates , satisfying . Insert their completeness relations on every time slice. This gives
The endpoint field configurations are fixed. Integrating the Gaussian momentum variables leaves the scalar field path integral . The functional measure means a regulated product over the field variables. A spacetime lattice or another ultraviolet cutoff makes this product finite before the continuum limit; interacting continuum calculations may require renormalization. The oscillatory Minkowski weight is an amplitude, not a positive probability density.
For vacuum expectation values, the boundaries must select the vacuum rather than arbitrary field configurations. Long imaginary-time evolution suppresses excited states: , so after normalization only the lowest-energy component remains as . This is vacuum projection by imaginary time. The corresponding Feynman i-epsilon prescription in the real-time integral specifies the vacuum boundary conditions and the poles of the propagator. With , the Euclidean path integral has the weight , where
It is often a useful regulated starting point; analytic continuation returns the vacuum time-ordered quantities.
Introduce a classical source and define the normalized vacuum generating functional
with the same vacuum prescription in numerator and denominator. A functional derivative brings down . The order of the time slices makes the operator insertion time-ordered. Thus source differentiation inserts time-ordered field operators:
The denominator removes vacuum diagrams and gives normalized expectation values. It is essential that these are time-ordered products; differentiating this vacuum functional does not directly give every possible operator ordering.
The free theory illustrates the method. Its quadratic kernel is with the vacuum pole prescription, and completing the square gives the Gaussian evaluation of a free scalar generating functional
Two source derivatives give . Higher derivatives give all pairings, the content of Wick theorem. For an interaction , one may use path-integral perturbation by source derivatives:
Expanding this expression generates Feynman diagrams and their Wick contractions. The connected generating functional retains connected contributions; in particular . These functionals turn the computation of field-operator expectations into source differentiation of an ordinary regulated integral.

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