Hidden Negative Energies in Strongly Accelerated Universes
classification
🌌 astro-ph.CO
gr-qchep-th
keywords
energynegativeacceleratedaccelerationbackgroundconditioncosmologicaldensities
read the original abstract
We point out that theories of cosmological acceleration which have equation of state, w, such that 1+w is small but positive may still secretly violate the null energy condition. This violation implies the existence of observers for whom the background has infinitely negative energy densities, despite the fact that the perturbations are free of ghosts and gradient instabilities.
This paper has not been read by Pith yet.
Forward citations
Cited by 1 Pith paper
-
Affine ANEC selects the closed FRW branch for geodesically complete cosmology
Affine ANEC obstructs non-static flat and open FRW from being null geodesically complete while ANEC-satisfying, but allows explicit scalar-field realizations for closed FRW with NEC-respecting matter.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.