Spacetime Memory and Emergent Galactic Dynamics(SMG): A Field-Theoretic Origin of the Observed Acceleration Law

The missing mass problem in galaxies remains unresolved within the standard cosmological model. This paper presents Spacetime Memory Gravity (SMG), a covariant scalar-tensor modification of general relativity in which an auxiliary field encodes the accumulated curvature history of spacetime. By localising a non-local curvature integral, the theory yields a well-defined action within the Horndeski class, preserving a strictly luminal gravitational wave speed. In the weak-field limit, the modified field equations produce a non-linear Poisson equation that integrates to an implicit acceleration law, a + αa3/2 = aN, predicting a logarithmic slope of 2/3 in the low-acceleration regime. A global fit to the full SPARC sample (175 galaxies, 2,847 data points) determines a universal coupling α = (1.20 ± 0.06) × 10−10 m−1/2s, yielding a mean reduced χ2ν = 1.12 ± 0.14. The same field dynamics naturally generate late-time cosmic acceleration with w ≈ −1 and dynamically link the galactic acceleration scale to the Hubble constant, a0 ≈ 0.1 cH0. Solar System constraints are satisfied via Vainshtein screening. The framework provides a unified, parameter-efficient description of galactic and cosmological dynamics, with clear falsifiable predictions for next-generation rotation curve, weak-lensing, and gravitational-wave observations.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-09-07
DOI
https://doi.org/10.5281/zenodo.19127349
Primary Topic
Cosmology and Gravitation Theories
Type
preprint
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preprint

Spacetime Memory and Emergent Galactic Dynamics(SMG): A Field-Theoretic Origin of the Observed Acceleration Law

SAMI ALMUAIGEL
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
preprint

Spacetime Memory and Emergent Galactic Dynamics(SMG): A Field-Theoretic Origin of the Observed Acceleration Law

SAMI ALMUAIGEL
preprint en

Abstract

The missing mass problem in galaxies remains unresolved within the standard cosmological model. This paper presents Spacetime Memory Gravity (SMG), a covariant scalar-tensor modification of general relativity in which an auxiliary field encodes the accumulated curvature history of spacetime. By localising a non-local curvature integral, the theory yields a well-defined action within the Horndeski class, preserving a strictly luminal gravitational wave speed. In the weak-field limit, the modified field equations produce a non-linear Poisson equation that integrates to an implicit acceleration law, a + αa3/2 = aN, predicting a logarithmic slope of 2/3 in the low-acceleration regime. A global fit to the full SPARC sample (175 galaxies, 2,847 data points) determines a universal coupling α = (1.20 ± 0.06) × 10−10 m−1/2s, yielding a mean reduced χ2ν = 1.12 ± 0.14. The same field dynamics naturally generate late-time cosmic acceleration with w ≈ −1 and dynamically link the galactic acceleration scale to the Hubble constant, a0 ≈ 0.1 cH0. Solar System constraints are satisfied via Vainshtein screening. The framework provides a unified, parameter-efficient description of galactic and cosmological dynamics, with clear falsifiable predictions for next-generation rotation curve, weak-lensing, and gravitational-wave observations.

Zenodo (CERN European Organization for Nuclear Research)
Reduced inequalities, Peace, Justice and strong institutions
Cosmology and Gravitation Theories
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