Bianchi-V models with constant-w or CPL dynamical dark energy accommodate DESI DR2 + SNIa + RSD data and reduce H0/S8 tensions relative to flat ΛCDM, though BIC still prefers ΛCDM.
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Dynamical dark energy in the Bianchi Type-V Universe with DESI DR2 BAO, SNIa compilation and RSD measurements
Bianchi-V models with constant-w or CPL dynamical dark energy accommodate DESI DR2 + SNIa + RSD data and reduce H0/S8 tensions relative to flat ΛCDM, though BIC still prefers ΛCDM.