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May 7, 20260 citationsOpen Access

Spacetime Densification Theory: A Unified Quantum Statistical Framework for Gravity, Cosmic Acceleration, and Galactic Phenomenology from Discrete Spacetime Microstructure

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PSPaulo G.A. Suassuna

Key Points

  • To develop a unified framework that reconciles quantum mechanics with gravitational dynamics.
  • Developed Spacetime Densification Theory as a scalar-tensor theory.
  • Embedded effective action in the Horndeski class for stability.
  • Used a grand canonical ensemble to derive an equation of state for spacetime.
  • Introduced a densification force contributing to gravitational dynamics.
  • Revealed an effective negative-pressure component linked to cosmic acceleration.
  • Provided a mechanism for regulating gravitational collapse in high-density scenarios.

Abstract

Abstract Reconciling gravitation with the quantum structure of nature remains an open problem in fundamental physics. We develop Spacetime Densification Theory (SDT) as a structured framework in which gravitational dynamics emerge from a discrete and saturable spacetime substrate composed of fundamental excitations, termed spaceons. At macroscopic scales, SDT is formulated as a scalar–tensor theory with a non-minimally coupled density field. By embedding the effective action within the Horndeski class, the theory preserves second-order field equations and avoids higher-derivative Ostrogradsky instabilities. In the Einstein frame, gradients of the spaceon density generate an additional attractive component, referred to here as the densification force. At microscopic scales, the spacetime vacuum is modeled as a quantum lattice gas of hard-core bosonic spaceons. From the grand canonical ensemble, we derive a universal equation of state for the spacetime medium. In the low-density regime, the cohesive sector yields an effective negative-pressure component compatible with late-time cosmic acceleration once normalized to the observed cosmological background. In the high-density regime, the packing contribution rises sharply as the medium approaches saturation, suggesting a possible mechanism for regulating gravitational collapse. The same framework also motivates a characteristic acceleration scale of order cH₀, linking the cosmological vacuum sector to low-acceleration galactic phenomenology. In the nonlinear halo regime, the scalar sector admits an asymptotic logarithmic overdensity profile associated with flat rotation curves and a BTFR-like scaling relation. These results should be interpreted with appropriate caution: the cosmological vacuum sector is calibrated rather than derived from a deeper ultraviolet theory, the galactic phenomenology has not yet been systematically confronted with full observational datasets, and the electromagnetic extension considered here remains exploratory at the effective-field-theory level. The theory is also discussed in relation to the Hubble tension: the characteristic acceleration scale a* ~ cH₀ emerging from the cosmological normalization of the cohesive vacuum sector is numerically close to the locally measured value, and SDT provides a late-time emergent-vacuum framework that is qualitatively relevant to the persistent discrepancy — now standing at 7.1σ between the local Distance Network determination and the early-Universe+ΛCDM value — between local and early-Universe measurements of H₀; a full quantitative reconciliation, however, has not yet been achieved. SDT should therefore be regarded not as a completed theory of quantum gravity, but as a mathematically structured and falsifiable framework in which spacetime microstructure, effective gravity, and selected cosmological and astrophysical regimes can be studied within a common setting.

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Cite This Study

Paulo G.A. Suassuna (2026) studied this question.

synapsesocial.com/papers/69fbe3aa164b5133a91a2ecehttps://doi.org/10.5281/zenodo.20039123
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