Neural network reconstruction of DESI DR2 BAO, SNe Ia, and cosmic chronometer data gives H0 = 71.5 ± 2.2 km s^{-1} Mpc^{-1} without sound horizon input.
Abdul Karimet al.(DESI Collaboration), Phys
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The Viaggiu holographic dark energy model fits late-time data similarly to Lambda CDM, yielding Omega_m0 around 0.24 and a model parameter of 0.27-0.33, with AIC showing statistical indistinguishability.
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A sound-horizon-free measurement of the Hubble constant from DESI DR2 baryon acoustic oscillations using artificial neural networks
Neural network reconstruction of DESI DR2 BAO, SNe Ia, and cosmic chronometer data gives H0 = 71.5 ± 2.2 km s^{-1} Mpc^{-1} without sound horizon input.
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Viaggiu holographic dark energy in light of DESI DR2
The Viaggiu holographic dark energy model fits late-time data similarly to Lambda CDM, yielding Omega_m0 around 0.24 and a model parameter of 0.27-0.33, with AIC showing statistical indistinguishability.