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.
arXiv comment5 pages; Accepted for publishing in PRD
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- -waves as exact solutions to ghost-free infinite derivative gravity
- Nonlocal generalization of Galilean theories and gravity
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- Superradiance in a ghost-free scalar theory
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- Blackhole in Nonlocal Gravity: Comparing Metric from Newmann-Janis Algorithm with Slowly Rotating Solution
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