Research Article

Fab Four: When John and George Play Gravitation and Cosmology

Figure 4

Evolution of the acceleration parameter versus the scale factor, for . Also shown in the graph: the evolution of the scalar field EoS and and . The scalar field becomes superluminal during the transition from a de Sitter Universe to a to stiff matter-dominated one. However, as discussed in the text, it remains hyperbolic and, thus, causal. Moreover, it carries positive energy.
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