Solar-System Bounds on the Aldred Frame: Perihelion Precession, Frame Dragging, and Light Travel Time

In Einstein-Cartan spin-torsion gravity, torsion is algebraic and vanishes in vacuum, so the frame predicts the general-relativistic result exactly in Mercury's perihelion advance, in Lense-Thirring frame dragging (Gravity Probe B and LAGEOS), and in the Shapiro delay (Cassini, gamma-1 = (2.1 +/- 2.3)e-5): anomalous advance zero, frame-dragging anomaly zero, gamma-1 = 0. The only correction is the interior density renormalization Delta rho/rho = rho/rho_A with rho_A = 9.72e54 g/cm^3, whose largest value anywhere in the solar system, at the solar core, is 1.54e-53. Unabsorbed upper bounds fall short of the observational bounds by 49 to 65 orders of magnitude; a measurable anomaly would require densities of 2.24e50 to 9.72e53 g/cm^3 or spin densities 1e25 to 1e26 times those present. AI-use disclosure: the computation and drafting were performed by Dave, an AI system, under the author's direction; the author of record, William Alexander Aldred, has reviewed the manuscript and takes responsibility for its content.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-10
DOI
https://doi.org/10.5281/zenodo.24102529
Primary Topic
Relativity and Gravitational Theory
Type
preprint
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preprint

Solar-System Bounds on the Aldred Frame: Perihelion Precession, Frame Dragging, and Light Travel Time

William Alexander Aldred
Zenodo (CERN European Organization for Nuclear Research)
Relativity and Gravitational Theory
preprint

Solar-System Bounds on the Aldred Frame: Perihelion Precession, Frame Dragging, and Light Travel Time

William Alexander Aldred
preprint en

Abstract

In Einstein-Cartan spin-torsion gravity, torsion is algebraic and vanishes in vacuum, so the frame predicts the general-relativistic result exactly in Mercury's perihelion advance, in Lense-Thirring frame dragging (Gravity Probe B and LAGEOS), and in the Shapiro delay (Cassini, gamma-1 = (2.1 +/- 2.3)e-5): anomalous advance zero, frame-dragging anomaly zero, gamma-1 = 0. The only correction is the interior density renormalization Delta rho/rho = rho/rho_A with rho_A = 9.72e54 g/cm^3, whose largest value anywhere in the solar system, at the solar core, is 1.54e-53. Unabsorbed upper bounds fall short of the observational bounds by 49 to 65 orders of magnitude; a measurable anomaly would require densities of 2.24e50 to 9.72e53 g/cm^3 or spin densities 1e25 to 1e26 times those present. AI-use disclosure: the computation and drafting were performed by Dave, an AI system, under the author's direction; the author of record, William Alexander Aldred, has reviewed the manuscript and takes responsibility for its content.

Zenodo (CERN European Organization for Nuclear Research)
Relativity and Gravitational Theory
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