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arXiv · 2606.27356

Beyond the equation of state: a second-order diagnostic for dynamical dark energy

Bob Osano
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Abstract

The first-order continuity equations determine the evolution of the energy densities but depend only on the instantaneous value of the dark-energy equation-of-state parameter. Differentiating these equations with respect to e-fold time introduces the term $\omega'_{\rm DE}$ explicitly, providing a second-order probe of dark-energy dynamics. Consequently, while information about the evolution of the equation of state is encoded in the full dynamical solution, it is not explicit in the first-order continuity equations evaluated at a given epoch. The second-order formulation, therefore, provides a complementary description in which the local evolution of the equation of state appears directly through the curvature of the density trajectory. For a two-fluid interacting dark-sector model with linear coupling $Q_{AB}=\alpha\rho_AH$, the resulting second-order equation defines a curvature diagnostic, $\mathcal{C}=\rho_{DE}''/\rho_{DE}$, whose leading contribution, in the cosmological-constant limit, is $\alpha^2$, while departures from $\omega_{DE}=-1$ generate corrections through both $\delta\omega=1+\omega_{DE}$ and the distinctive term $-3\omega_{DE}'$. Unlike first-order analyses, this contribution is independent of the interaction strength and directly identifies dynamical dark energy. Applying the diagnostic to a CPL model with parameters consistent with DESI constraints, we recover $\omega_{DE}'$ across the full redshift range for both weak and strong interactions. Noise propagation shows that the diagnostic is detectable with signal-to-noise ratio exceeding three for $\sigma_H/H\lesssim1.5\%$, while the degeneracy between $\alpha$ and $\omega_{DE}'$ remains negligible for $\alpha\lesssim0.1$. In the non-interacting limit, the formalism naturally recovers the Caldwell--Linder thawing/freezing classification and extends it to interacting dark-energy models.

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Bob Osano. 2026-06-25. Beyond the equation of state: a second-order diagnostic for dynamical dark energy. https://arxiv.org/abs/2606.27356

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