Rotating metric in Non-Singular Infinite Derivative Theories of Gravity
Alan S. Cornell, Gerhard Harmsen, Gaetano Lambiase, Anupam Mazumdar

TL;DR
This paper introduces a non-singular rotating spacetime metric within a ghost-free infinite derivative gravity theory, predicting deviations in the Lense-Thirring effect compared to general relativity.
Contribution
It presents a novel non-singular rotating metric in infinite derivative gravity and analyzes its implications for frame-dragging effects.
Findings
Non-singular rotating metric derived
Predictions for Lense-Thirring effect differ from GR
Potential observational signatures identified
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.
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