Rotating metric in Non-Singular Infinite Derivative Theories of Gravity
arXiv:1710.02162 · doi:10.1103/PhysRevD.97.104006
Abstract
In this paper we will provide a non-singular rotating space time metric for a ghost free infinite derivative theory of gravity. We will provide the predictions for the Lense-Thirring effect for a slowly rotating system, and how it is compared with that from general relativity.
5 pages; Accepted for publishing in PRD