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Interacting dark energy constraints from Fermi GRBs and Pantheon+ SNe Ia with full GRB covariance
The standard $Λ$CDM model faces long-standing theoretical and observational problems, such as the Hubble tension, which motivate extensions beyond $Λ$CDM, including interacting dark energy (IDE). Type Ia supernovae (SNe Ia) are precise probes of the late-time expansion history, while gamma-ray burst
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