Conditions for defocusing around more general metrics in Infinite Derivative Gravity
arXiv:1802.09063 · doi:10.1103/PhysRevD.97.084046
Abstract
Infinite Derivative Gravity is able to resolve the Big Bang curvature singularity present in general relativity by using a simplifying ansatz. We show that it can also avoid the Hawking- Penrose singularity, by allowing defocusing of null rays through the Raychaudhuri equation. This occurs not only in the minimal case where we ignore the matter contribution, but also in the case where matter plays a key role. We investigate the conditions for defocusing for the general case where this ansatz applies and also for more specific metrics, including a general Friedmann-Robertson-Walker (FRW) metric and three specific choices of the scale factor which produce a bouncing FRW universe.
10 pages, accepted by PRD
References in corpus (17)
- The Confrontation between General Relativity and Experiment
- Towards a Resolution of the Cosmological Singularity in Non-local Higher Derivative Theories of Gravity
- Dynamics with Infinitely Many Derivatives: The Initial Value Problem
- Inflation in (Super-)renormalizable Gravity
- Do massive compact objects without event horizon exist in infinite derivative gravity?
- inflation to probe non-perturbative quantum gravity
- Wald's gravitational entropy for ghost-free, infinite derivative theories of Gravity
- Stringy gravity at short distances
- Stability of Schwarzschild singularity in non-local gravity
- Rotating metric in Non-Singular Infinite Derivative Theories of Gravity
- Cosmological perturbations in non-local higher-derivative gravity
- Geodesic completeness and homogeneity condition for cosmic inflation
- Ghost and singularity free theories of gravity
- Newtonian Potential and Geodesic Completeness in Infinite Derivative Gravity
- Revealing Infinite Derivative Gravity's true potential: The weak-field limit around de Sitter backgrounds
- Towards UV Finiteness of Infinite Derivative Theories of Gravity and Field Theories
- Criteria for resolving the cosmological singularity in Infinite Derivative Gravity around expanding backgrounds