Department of Physics Papers

Document Type

Journal Article

Date of this Version

5-17-2011

Abstract

An alternative to the effective field theory approach to treat ghosts in higher derivative theories is to attempt to integrate them out via the Euclidean path integral formalism. It has been suggested that this method could provide a consistent framework within which we might tolerate the ghost degrees of freedom that plague, among other theories, the higher derivative gravity models that have been proposed to explain cosmic acceleration. We consider the extension of this idea to treating a class of terms with order six derivatives, and find that for a general term the Euclidean path integral approach works in the most trivial background, Minkowski. Moreover we see that even in de Sitter background, despite some difficulties, it is possible to define a probability distribution for tensorial perturbations of the metric.

Comments

Suggested Citation:
M. Fontanini and M. Trodden. (2011). Tackling higher derivative ghosts with the Euclidean path integral. Physical Review D 83, 103518.

© 2011 The American Physical Society
http://dx.doi.org/10.1103/PhysRevD.83.103518

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Date Posted: 19 May 2011

This document has been peer reviewed.