$\mathcal{H}$olographic $\mathcal{N}$aturalness and Pre-Geometric Gravity
Andrea Addazi, Salvatore Capozziello, Giuseppe Meluccio

TL;DR
This paper proposes a unified framework combining holographic naturalness and pre-geometric gravity to explain the smallness and stability of the cosmological constant through entropy and quantum information considerations.
Contribution
It introduces a model where spacetime geometry emerges from symmetry breaking and links the de Sitter entropy to a fundamental Higgs-like field, offering a novel solution to the cosmological constant problem.
Findings
De Sitter entropy is proportional to the Higgs field VEV v.
The small cosmological constant results from the largeness of de Sitter entropy.
Quantum transitions are exponentially suppressed in high-entropy states.
Abstract
The cosmological constant (CC, ) problem represents a remarkable discrepancy of about 120 orders of magnitude between the observed dark energy and its natural expectation from quantum field theory. This paper synthesizes two paradigms - holographic naturalness () and pre-geometric gravity (PGG) - to propose a unified resolution. The framework posits that CC stability is not a matter of radiative corrections but of quantum information and entropy. The large entropy of the de Sitter (dS) vacuum acts as an entropic barrier, exponentially suppressing destabilizing quantum transitions. This explains why the universe remains in a high-entropy, low-CC state. We embed this within PGG, where spacetime geometry and the Einstein-Hilbert action emerge dynamically from the spontaneous symmetry breaking…
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