A finite time pseudo-rip singularity is introduced that violates all energy conditions, occurs after phantom acceleration, and allows a model matching past Lambda-CDM while ending in a future pressure singularity.
Caldwell, A phantom menace? cosmological conse- quences of a dark energy component with super-negative equation of state, Physics Letters B545, 23 (2002)
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Finite time pseudo-rip singularity in cosmology
A finite time pseudo-rip singularity is introduced that violates all energy conditions, occurs after phantom acceleration, and allows a model matching past Lambda-CDM while ending in a future pressure singularity.