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Metastability in Emergent Dark Energy: A New Framework Confronting Cosmological Observations

  • Authors: Xiaolei Li, Tonghua Liu, Tian-Nuo Li, Guo-Hong Du, Arman Shafieloo, Marek Biesiada

Xiaolei Li et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

Redshift evolution of the dark-energy sector. Left: the dark-energy density ρDE(z)/ρDE0. Right: the equation of state wDE(z). The red solid line represents the best-fit MEDE model (CMB+DESI+PantheonPlus). The light-orange region shows the 2σ confidence region derived from MCMC chains, illustrating the posterior distribution of parameters. The green solid line shows the CPL parameterization ((CMB+DESI+PantheonPlus best-fit), and the black dashed line represents ΛCDM. The MEDE model exhibits a smooth transition around zt ∼ 0.42, crossing the phantom divide w = −1 from phantom-like (w < −1) at high redshifts to quintessence-like (w > −1) at low redshifts.

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