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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 4.

Redshift evolution of the dark-energy sector for MEDE, CPL, and ΛCDM. Left: dark-energy density ρDE(z)/ρDE,0. Right: equation of state wDE(z). The red solid line shows the best-fit MEDE model (CMB+DESI+PantheonPlus). The green solid line is the best-fit CPL parameterization, and the black dashed line is ΛCDM. The evolution is shown from the distant past ﹩z\approx 10﹩ to the asymptotic future ﹩z\to -1﹩, illustrating the distinct behaviors of each model at late times.

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