Constraining neutrino masses in the Barrow holographic dark energy model with Granda–Oliveros IR cutoff by Mojtaba Mahmoudifard, Amin Salehi, Reza Sepahvand

“…Abstract The holographic dark energy (HDE) model resides in quantum gravity in connection with the entropy, which requires an appropriate IR-cutoff to support the accelerating universe. Of these, the BHDE is corresponding to the quantum-corrected Barrow entropy $$S_{B}\propto A^{1+\Delta /2}$$ S B ∝ A 1 + Δ / 2 for which the Granda–Oliveros (GO) IR-cutoff $$L_{IR}=(\alpha H^2 + \beta \dot{H})^{-\frac{1}{2}}$$ L IR = ( α H 2 + β H ˙ ) - 1 2 avoids the causality problem of the typically used future event-horizon. …”
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