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.
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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.