The four-dimensional null energy condition as a swampland conjecture
arXiv:2107.06900 · doi:10.1103/PhysRevLett.127.181301
Abstract
We analyze four-dimensional Friedmann-Lemaitre-Robertson-Walker cosmologies in type IIB, arising from a M-theory dual, and find that the null energy condition (NEC) has to be obeyed by them (except for the negatively curved case) in order for the M-theory action to have a Wilsonian effective description. However, this does not imply that the M-theory metric has to obey the 11d NEC. Thus, we propose a new swampland conjecture -- the 4d NEC is a consistency condition for any theory to have a completion within M-theory -- with an explicit derivation of it for cosmological backgrounds from a top-down perspective. We briefly discuss the cosmological consequences of such a condition derived from M-theory.
14 pages (including an Appendix); comments welcome; v2: double-columned 8 pages (includes Supplementary Materials), matches published version
References in corpus (9)
- The Swampland: Introduction and Review
- Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies
- Bouncing Universe with Quintom Matter
- A Matter Bounce By Means of Ghost Condensation
- Hidden Negative Energies in Strongly Accelerated Universes
- On the Null Energy Condition and Cosmology
- Relaxing the Cosmological Constant: a Proof of Concept
- Derivation of the Null Energy Condition
- Null Energy Condition and Dark Energy Models