Rindler type acceleration in f(R) gravity
S. Habib Mazharimousavi, M. Halilsoy

TL;DR
This paper demonstrates that a specific $f(R)$ gravity model with a logarithmic correction can produce a Rindler acceleration term in the metric, satisfying certain energy conditions.
Contribution
It introduces a new $f(R)$ gravity model that naturally incorporates Rindler acceleration and analyzes the energy conditions within this framework.
Findings
The model yields a Rindler acceleration term in the metric.
Weak and strong energy conditions are satisfied in certain domains.
The chosen $f(R)$ form links Rindler acceleration with modified gravity.
Abstract
By choosing a fluid source in gravity, defined by f\left(R\right) =R-12a\xi \ln \left\ | R\right\ | , where (=Rindler acceleration) and are both constants, the field equations correctly yield the Rindler acceleration term in the metric. We identify domains in which the weak energy conditions (WEC) and the strong energy conditions (SEC) are satisfied.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
