Abstract
PT-symmetric quantum mechanics began with a study of the Hamiltonian $H=p^2+x^2(ix)^\varepsilon$. A surprising feature of this non-Hermitian Hamiltonian is that its eigenvalues are discrete, real, and positive when $\varepsilon\geq0$. This paper examines the corresponding quantum-field-theoretic Hamiltonian $H=\frac{1}{2}(\nabla\phi)^2+\frac{1}{2}\phi^2(i\phi)^\varepsilon$ in $D$-dimensional spacetime, where $\phi$ is a pseudoscalar field. It is shown how to calculate the Green's functions as series in powers of $\varepsilon$ directly from the Euclidean partition function. Exact finite expressions for the vacuum energy density, all of the connected $n$-point Green's functions, and the renormalized mass to order $\varepsilon$ are derived for $0\leq D<2$. For $D\geq2$ the one-point Green's function and the renormalized mass are divergent, but perturbative renormalization can be performed. The remarkable spectral properties of PT-symmetric quantum mechanics appear to persist in PT-symmetric quantum field theory.
Highlights
The study of PT -symmetric quantum theory may be traced back to a series of papers that proposed a new perturbative approach to scalar quantum field theory
The remarkable spectral properties of PT -symmetric quantum mechanics appear to persist in PT -symmetric quantum field theory
Instead of a conventional perturbation expansion in powers of a coupling constant, it was proposed that a parameter δ that measures the nonlinearity of the theory could be used as a perturbation parameter [1,2]
Summary
The study of PT -symmetric quantum theory may be traced back to a series of papers that proposed a new perturbative approach to scalar quantum field theory. PT -symmetric quantum mechanics began with the surprising discovery that spurious complex numbers do not appear if the quantity raised to the power δ is PT symmetric (invariant under combined space and time reflection) [4,5]. The purpose of this paper is to introduce powerful new tools and techniques that can be used to investigate PT -symmetric quantum field theories. We illustrate these tools by studying the quantum-field-theoretic analog of (1) whose D-dimensional Euclidean-space Lagrangian density is. For a quantum field theory having a complex logarithmic interaction term it is not obvious whether one can find Feynman rules for performing perturbative diagramatic calculations.
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