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Healing the Big Bang: Ghost-Free Nonlocal Gravity Erases Cosmological Singularities

Einstein's General Relativity inevitably fractures into infinite, unphysical singularities at black hole centers and the cosmic dawn; infinite-derivative nonlocal gravity smooths out short-distance curvature without introducing destructive ghost instabilities.

Author
Tirthabir Biswas et al.
Published
2012
Journal
Physical Review Letters
Last updated
September 2026
Healing the Big Bang: Ghost-Free Nonlocal Gravity Erases Cosmological Singularities

Einstein's theory of General Relativity stands as a monument of modern physics, yet it carries the mathematical seeds of its own destruction: at black hole centers and the Big Bang, gravitational curvature spikes to infinity, causing the laws of physics to break down entirely.

Attempts to cure these gravitational infinities by adding higher-order curvature terms historically triggered an even deadlier theoretical disease: Ostrogradsky instabilities and unphysical negative-energy quantum states known as 'ghosts' that tear quantum spacetime apart.

Biswas, Mazumdar, and Siegel resolved this long-standing impasse by formulating a fully covariant gravitational action with non-polynomial, infinite-derivative kinetic operators. In the ultraviolet limit, the infinite derivatives act as a natural non-local filter that disperses gravitational point charges into smooth, finite energy distributions while preserving unitary, ghost-free propagation in the infrared.

By banishing infinite curvature singularities without sacrificing quantum consistency, ghost-free non-local gravity opens a viable mathematical pathway toward nonsingular cosmological bouncing universes and a smooth quantum description of black hole horizons.

Reference

Biswas, T., Gerwick, E., Koivisto, T., & Mazumdar, A. (2012). Towards Singularity- and Ghost-Free Theories of Gravity. Physical Review Letters, 108(3).

Title

Towards Singularity- and Ghost-Free Theories of Gravity

Abstract

We present the most general covariant ghost-free gravitational action in a Minkowski vacuum. Apart from the much studied f(R) models, this includes a large class of nonlocal actions with improved UV behavior, which nevertheless recover Einstein's general relativity in the IR.

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