Reconstructing the generalized Barrow holographic dark energy with physics-informed neural networks

Abstract

Barrow holographic dark energy connects cosmic acceleration with possible quantum-gravitational deformations of horizon entropy, encoded in the Barrow exponent $\Delta$. If such effects are scale dependent, however, there is no fundamental reason for $\Delta$ to remain constant throughout cosmic history. In this work we reconstruct $\Delta (z)$ directly from observations, without assuming any particular functional form, using the Cosmo-PINN physics-informed neural-network framework. The generalized Barrow holographic evolution equation is incorporated into the training, while PantheonPlus supernovae, DESI DR2 baryon acoustic oscillations and cosmic chronometers constrain the reconstruction. We find a mild and smooth redshift evolution, with the posterior mean favoring negative $\Delta$ and this tendency becoming stronger when the Cepheid calibration is included. Nevertheless, $\Delta =0$ and constant negative values remain compatible with current uncertainties. The reconstructed cosmology yields a viable late-time evolution, with $w_{\mathrm{DE}}$ close to $-1$ and the expected transition to accelerated expansion. Our results demonstrate that cosmological observations can directly probe the functional behavior of a quantity entering the underlying entropy law itself.

arXiv comment14 pages, 7 figures. Comments are welcome