Informativity Institute · Press release archive

Updated Hubble comparisons show both agreement and pressure on MQ’s proposal

Newer CMB comparisons sit below the lower MQ rate, while the four-anchor SH0ES distance-ladder result remains close to the upper rate.

· Recorded source-review snapshot · Retrospective release

CHICAGO — Updated comparisons give a mixed assessment of Measurement Quantization’s two proposed expansion-rate realizations. The current conditional MQ values are 68.259 ± 0.019 and 73.508 ± 0.020 kilometres per second per megaparsec. Newer CMB results place more pressure on the lower value than the comparisons emphasized in the original 2025 paper.

The specified SPT-3G D1 analysis gives 66.66 ± 0.60, while its combined South Pole Telescope, Atacama Cosmology Telescope and Planck analysis gives 67.19 ± 0.38 in the same units. The 2024 SH0ES result incorporating the Small Magellanic Cloud as a fourth geometric anchor gives 73.17 ± 0.86. Figure 1 keeps the observational inferences and MQ model values distinct.

Lower MQ rate68.259 ± 0.019 km s⁻¹ Mpc⁻¹
Combined CMB inference67.19 ± 0.38 km s⁻¹ Mpc⁻¹
Distance-ladder inference73.17 ± 0.86 km s⁻¹ Mpc⁻¹; upper MQ rate 73.508 ± 0.020
Figure 1. Selected current comparison values. CMB and distance-ladder inferences retain their analysis assumptions; MQ uncertainties are conditional input-propagated quantities.

A transparent Gaussian diagnostic combines each displayed observational uncertainty with the corresponding quoted MQ input uncertainty, assuming zero cross-covariance for that calculation. It gives differences of about 2.66 standard deviations for SPT-3G D1, 2.81 for the combined CMB result and 0.39 for the four-anchor distance ladder. The source review’s SPT figure of about 2.67 is reproduced to rounding level; the Brief states the precise convention used here.

The MQ branch separation is 5.249 kilometres per second per megaparsec, compared with 5.980 for the SH0ES-minus-combined-CMB pair. Their difference is about 0.78 times the observational uncertainty of that separation under an independent-input approximation. This is a restricted difference diagnostic. A close separation does not establish agreement of both absolute rates, and it is not an additional independent success.

The two MQ rates share the same coefficient, reconstructed age and temporal-normalization premise. Their quoted errors exclude unquantified model discrepancy. The SPT-only result also overlaps the combined CMB analysis, so those comparisons cannot be multiplied as independent evidence.

MQ associates the lower and upper model rates with different measurement constructions. The astronomical estimates do not independently identify those frames. Establishing that interpretation requires an observable-level model and a joint analysis that preserves the acoustic, distance and calibration constraints of the contributing datasets.

The companion Brief provides the rate equations, version-specific source references, worked residuals and graphics showing both absolute values and branch separation. The update preserves the less favorable comparisons alongside the closer one, without turning numerical compatibility into a probability that MQ is correct.

UPDATED HUBBLE COMPARISONS · JOURNALIST BRIEF

The two MQ rates, primary observational sources, reproducible pull calculations and shared-input limits, with absolute-rate and separation graphics.

Read the full technical Brief →

Research sources

Resolving the Hubble tension 68.261 and 73.510 km s⁻¹ Mpc⁻¹ · J. A. Geiger · AIP Advances 15, 075134 · DOI 10.1063/5.0269029 · Published July 22, 2025.

Current revised Hubble preprint · Galactic manuscript, Section 3.12. These provide later model values and dependency qualifications, not additional independent Hubble measurements.

SPT-3G D1 analysis, version 2 · Breuval and collaborators, four-anchor SH0ES analysis. The companion Brief records the exact numerical comparisons and assumptions.

Archive date and research status

September 27, 2026 identifies the recorded source-review snapshot. It is not an established original discovery, first announcement or journal publication date. This retrospective release and its Brief were prepared or revised October 26, 2026. The 2025 publication is distinguished from the current MQ preprint, whose journal publication is not established. The work reproduces displayed-value diagnostics; it does not rerun cosmological data or establish a joint resolution of the Hubble tension.

About the Informativity Institute

The Informativity Institute presents the Measurement Quantization research program and its publications. MQ investigates the relationship between discrete count structure and physical measurement. Individual results should be assessed through their stated assumptions, sources and observational tests.

Media contact

Hoyt Hudson · Informativity Institute
HoytHudson@informativity.org
Media contact page · Research publications

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