Holographic Elasticity and Cyclic Cosmology: A Geometric Resolution to the Cosmological Constant Problem
Poster-Virtual · Withdrawn
Abstract
We present a new framework, termed Holographic Elasticity, that provides a dynamical and geometric resolution to the cosmological constant problem. The framework treats spacetime as an emergent elastic medium, with the strain field $\phi$ and its Planck-scale stiffness $\kappa \sim M_{\text{Pl}}^{2}$ derived from Group Field Theory condensates. The core of the mechanism is the Elastic–Holographic Relaxation Principle, where the number of active holographic degrees of freedom $N$ is a dynamical variable governed by the kinetic equation $dN/dt = \Gamma (E_{\text{el}}/M_{\text{Pl}} - \alpha N)$. The standard holographic scaling $N \propto R^{2} / \ell_{\text{Pl}}^{2}$ emerges as the late-time equilibrium solution, leading to a universal scaling law for the gravitationally active vacuum energy, $\rho_{\Lambda} \sim M_{\text{Pl}}^{4} / N$. The global vacuum energy sequestering mechanism is naturally incorporated to render Standard Model vacuum loops gravitationally inert, while the geometric holographic residual remains immune to cancellation. The off-equilibrium dynamics ($\dot{N} \neq 0$) predict a specific, testable deviation in the dark energy equation of state, with $1+w \sim O(10^{-2})$. This clear observational signature distinguishes the framework from $\Lambda$CDM and simple quintessence models, making it falsifiable by next-generation cosmological surveys. The work unifies insights from quantum geometry, holography, and vacuum energy sequestering into a single predictive framework.
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Publication: Physics Letters B — Manuscript submitted and currently under review
Presenters
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Amrit Ladhani
- Independent Researcher