New counterterms induced by trans-Planckian physics in semiclassical gravity

Abstract

We consider free and self-interacting quantum scalar fields satisfying modified dispersion relations in the framework of Einstein-Aether theory. Using adiabatic regularization, we study the renormalization of the equation for the mean value of the field in the self-interacting case, and the renormalization of the semiclassical Einstein-Aether equations for free fields. In both cases we consider Bianchi type I background spacetimes. Contrary to what happens for {\it free} fields in {\it flat} Robertson-Walker spacetimes, the self-interaction and/or the anisotropy produce non-purely geometric terms in the adiabatic expansion, i.e terms that involve both the metric $g_{\mu \nu }$ and the aether field $u_{\mu }$. We argue that, in a general spacetime, the renormalization of the theory would involve new counterterms constructed with $g_{\mu \nu }$ and $u_{\mu }$, generating a fine-tuning problem for the Einstein-Aether theory.

References in corpus (2)

• Detecting a Lorentz-Violating Field in Cosmology
• A momentum-space representation of Green's functions with modified dispersion on ultra-static space-time

Cited by in corpus (1)

• Einstein-aether gravity: a status report