Resolving the Vacuum Catastrophe: Holographic Bit-Density and the Cosmological Constant

Authors

  • Cody Hudock Hudock nformation Physics Institute, Gosport, Hampshire, United Kingdom, www.informationphysicsinstitute.org

DOI:

https://doi.org/10.59973/ipil.345

Keywords:

Vacuum Catastrophe, Cosmological constant, Holographic principle, Infodynamics, MEI principle, Landauer's principle, Dark Energy, information theory

Abstract

The quantum vacuum zero-point energy exceeds the observed Dark Energy density by ∼ 10120. We present a heuristic framework in which spacetime is a discrete substrate constrained by holographic bounds and Dark Energy arises as the Landauer erasure cost of maintaining spatial geometry. Combining the Cohen-Kaplan-Nelson (CKN) holographic bound with the Landauer erasure cost at the CMB temperature yields a bare vacuum density ρbare ≈ 2.07×10−27 kg/m3—within a factor of ∼ 4 of the Friedmann critical density, with no fitted parameters. The residual factor is determined by the dimensionless ratios TCMB/TP and H0tP (equation 11); its proximity to ln(57) ≈ 4.04, where N = 57 is the Standard Model chiral degree-of-freedom count, is noted but not derived. Casting the thermodynamic suppression of Dark Energy by matter as an interacting dark
energy model, the framework predicts a quintessence equation of state (w > −1) at all epochs. The perturbative
estimate gives w0 ≈ −0.75; a companion osmotic-pressure derivation refines this to w0 = −0.983. Both lie within current observational bounds and will be tested by Stage IV experiments.

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Published

2026-05-04

How to Cite

Hudock, C. H. (2026). Resolving the Vacuum Catastrophe: Holographic Bit-Density and the Cosmological Constant. IPI Letters, 4(2), 41–48. https://doi.org/10.59973/ipil.345

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