Interpreting Dark Energy Data Away from $\mathrm{\Lambda }$

Dark energy away from a cosmological constant $\mathrm{\Lambda }$ – like early universe inflation that ends – can be understood in terms of well defined physical behaviors. These guide dark energy into thawing or freezing classes, with $w_0$–$w_a$ arising as a physical calibration of the phase space. Other regions of phase space – zones of avoidance – require violation of some basic principle. We explore these cases, drawing a direct analogy with how nonGaussianity in inflation can add physics beyond standard dynamics. We examine the physics implications if the best fit of current data is taken to be truth, outlining four properties, and investigate the reality of phantom crossing $w=-1$, finding it significantly favored.