arXiv · 1801.00834
Revealing Infinite Derivative Gravity's true potential: The weak-field limit around de Sitter backgrounds
Abstract
General Relativity is known to produce singularities in the potential generated by a point source. Our universe can be modelled as a de Sitter (dS) metric and we show that ghost-free Infinite Derivative Gravity (IDG) produces a non-singular potential around a dS background, while returning to the GR prediction at large distances. We also show that although there are an apparently infinite number of coefficients in the theory, only a finite number actually affect the predictions. By writing the linearised equations of motion in a simplified form, we find that at distances below the Hubble length scale, the difference between the IDG potential around a flat background and around a de Sitter background is negligible.
Explore related subjects
Keep this discovery
James Edholm. 2018-01-02. Revealing Infinite Derivative Gravity's true potential: The weak-field limit around de Sitter backgrounds. https://doi.org/10.1103/physrevd.97.064011
Cite the original work for its findings. Save a collection to share your selection of sources.