Informativity Institute · Research brief · 26 October 2026

Updated Hubble comparisons in MQ

Current model rates, version-specific CMB and distance-ladder inferences, reproducible residual diagnostics and the covariance needed to interpret them.

Archive source-review snapshot: September 27, 2026 · Brief prepared: October 26, 2026
Read the companion press release

What has changed since the published proposal

The 2025 AIP Advances paper proposed two realized rate assignments for a common expansion geometry. Its historical values were 68.261 and 73.510 kilometres per second per megaparsec. The current revised source gives 68.259(19) and 73.508(20), with conditional input uncertainties and stronger evidence qualifications. Neither set is itself an independent astronomical measurement. [1] [4]

Table 1: Historical and current MQ rate values
QuantityPublished 2025 formulationCurrent revised sourceStatus
Lower rate68.26168.259 ± 0.019Conditional model rate
Upper rate73.51073.508 ± 0.020Conditional model rate; current uncertainty replaces an older ±0.021
Inverse-age midpoint70.88570.884 ± 0.020Shared baseline, not an additional observation

All rate values in Table 1 use kilometres per second per megaparsec. The current uncertainties propagate declared inputs while holding the temporal-normalization premise fixed. Historical rounded values are not assigned new error bars. Parentheses in the current source refer to one standard input-propagated uncertainty in the final printed digits. [1]

The two realized rate assignments

Let 𝐻sys and 𝐻int denote the System Frame and Internal Frame-resolved physical comparison rates. Let 𝜃𝑠𝑖 be the dimensionless invariant MQ coefficient, π the dimensionless circle constant and 𝐴𝑈 the realized System Frame universe age in seconds. Equations (1a) and (2b) give inverse-second rates before conversion to astronomical units. These labels are local to the Brief. [1]

𝐻sys=π𝜃𝑠𝑖𝐴𝑈(1a)
𝐻int=2𝜃𝑠𝑖−π𝜃𝑠𝑖𝐴𝑈(2b)

The Internal Frame is the discrete count-configuration domain; the System Frame is its observable relational realization. The Frames mapping connects them. Both displayed rates are physical realized comparison quantities, with inverse-time units. Their labels do not assign an SI frequency to the primitive pre-realization domain, and they do not mean that an observational dataset has independently detected either frame. [1]

For a central arithmetic example, take the coefficient 3.26239030504 and the reconstructed age 13.794339221862558 billion Julian years. One Julian year is exactly 31,557,600 seconds. The resulting inverse-second rates are about 2.212122057 × 10⁻¹⁸ and 2.382239051 × 10⁻¹⁸. Conversion using one megaparsec of about 3.08567758149 × 10¹⁹ kilometres gives rates rounding to 68.259 and 73.508. This reproduces central arithmetic under the stated inputs; the extra digits do not create new measurement precision. [1]

The age reconstruction uses measured CMB temperature and the fine-structure calibration, together with a fixed realization normalization. The age is derived, not an additional independent datum. Its absolute temporal normalization remains unverified, and its uncertainty and model discrepancy are excluded from the small quoted input errors. Conditional precision must not be presented as a complete theory uncertainty. [1]

Midpoint, separation and ratio share the same inputs

Equations (3c)–(5e) follow algebraically from the two rate assignments. They show that the midpoint, separation and ratio are related outputs, rather than additional independent predictions to multiply into a global evidence claim.

𝐻int−𝐻sys=2(𝜃𝑠𝑖−π)𝜃𝑠𝑖𝐴𝑈(3c)
𝐻sys+𝐻int2=1𝐴𝑈(4d)
𝐻int𝐻sys=2𝜃𝑠𝑖−ππ(5e)

The midpoint is an MQ normalization, not a universal identity between the Hubble constant and cosmic age in arbitrary cosmologies. The physical separation has rate units; it is distinct from the dimensionless circle-coefficient offset used in the source’s mapping construction. Common age changes shift both model rates together. Uncertainty in their difference therefore cannot be obtained by simply adding their individual variances as if independent. [1]

Which external results are being compared

The selected observational values are fixed to explicit source versions. Camphuis and collaborators’ version 2, dated April 1, 2026, gives SPT-3G D1 66.66 ± 0.60 and the combined CMB-SPA result 67.19 ± 0.38. CMB-SPA combines SPT, ACT and Planck information. These are base-ΛCDM inferences from CMB primary spectra and lensing, not direct measurements of today’s rate at last scattering. The combined sample contains SPT information and is not independent of the SPT-only row. [2]

Version control matters. The first arXiv version used 67.24 ± 0.35 for the combined result; the version cited here uses 67.19 ± 0.38. A historical or updated comparison must identify the exact version and combination rather than transfer a value across editions without notice. [2]

Breuval and collaborators’ 2024 four-anchor SH0ES result is 73.17 ± 0.86. The Small Magellanic Cloud was added to the geometric foundation of the Cepheid and Type Ia-supernova ladder. This combined result is distinct from their SMC-only value of 74.1 ± 2.1. The present comparison uses the combined four-anchor inference. [3]

Figure 1 shows the three external estimates and the two MQ assignments on the same rate axis. The very short MQ error bars represent conditional propagated inputs, not a complete uncertainty budget for the proposed mechanism.

Figure 1. Observational rate inferences and conditional MQ valuesFive rows show SPT-3G D1 66.66 plus or minus 0.60, CMB-SPA 67.19 plus or minus 0.38, lower MQ 68.259 plus or minus 0.019, four-anchor SH0ES 73.17 plus or minus 0.86 and upper MQ 73.508 plus or minus 0.020. All rates are kilometres per second per megaparsec. Bars show quoted uncertainties without enlarging the small MQ bars. The CMB rows overlap in data; MQ uncertainties omit model discrepancy.Absolute-rate comparisons retain both agreement and pressureQuoted ± uncertainties · observational inferences and conditional model rates 66 67 68 69 70 71 72 73 74 75 SPT-3G D166.66 ± 0.60 CMB-SPA67.19 ± 0.38 MQ lower68.259 ± 0.019 SH0ES four anchors73.17 ± 0.86 MQ upper73.508 ± 0.020 Expansion rate (km s⁻¹ Mpc⁻¹)CMB-SPA contains SPT data; the MQ input uncertainties are correlated and conditional.
Figure 1. Redrawn from the quoted values in sources [1]–[3]. The bars are not a joint likelihood, and the repeated CMB information must not be counted twice.

Reproduce the individual displayed-value diagnostics

Table 2 uses the corresponding MQ central value minus the observed value. For this diagnostic only, the denominator is the square root of the sum of their two quoted variances. The calculation treats the displayed errors as symmetric Gaussian standard uncertainties, assumes zero model–observation cross-covariance and excludes unquantified theory discrepancy. These assumptions define a transparent arithmetic check, not a complete likelihood.

Table 2: Displayed-value diagnostics; rate columns in km s⁻¹ Mpc⁻¹; signed diagnostic dimensionless
ComparisonObserved valueMQ valueMQ minus observedCombined scaleSigned diagnostic
SPT-3G D166.66 ± 0.6068.259 ± 0.019+1.5990.600301+2.664
CMB-SPA67.19 ± 0.3868.259 ± 0.019+1.0690.380475+2.810
SH0ES four anchors73.17 ± 0.8673.508 ± 0.020+0.3380.860233+0.393

For the SPT-only row, the residual is 1.599 and the combined scale is 0.600301, giving 2.663665, or 2.66 at two decimals. The archive source review stated about 2.67. Ignoring the tiny MQ uncertainty gives 2.665, explaining the rounding-level difference. The combined CMB and ladder rows give 2.81 and 0.39 at two decimals. This Brief reports the explicit denominator rather than implying a new data reduction.

A standardized residual is neither a probability that MQ is true nor a discovery significance for the proposed mapping. The CMB-derived estimates assume a particular cosmological model. MQ must specify its own acoustic, distance and growth predictions before it can replace that inference model. Comparing a model rate to another model’s compressed parameter estimate is a useful diagnostic, with that limitation retained. [1] [2]

Why the separation diagnostic is not an extra test

Table 3 uses the rounded model rates and the four-anchor-minus-CMB-SPA observed pair. For the observational difference alone, independent quoted errors give a scale of 0.940213. The absolute separation residual of 0.731 is 0.777484 times that scale. This reproduces the archive’s approximately 0.78 diagnostic without inventing an uncertainty for the correlated MQ split.

Table 3: Separation and midpoint from the same pair; rate quantities in km s⁻¹ Mpc⁻¹; diagnostic dimensionless
QuantityValueInterpretation
MQ upper minus lower5.249Difference of two correlated model outputs
SH0ES minus CMB-SPA5.980External difference under the declared inference models
MQ minus external separation-0.731Absolute residual is 0.731
External separation error scale0.940213Independent observational-error approximation only
Absolute residual / external scale0.777484Restricted diagnostic; no complete model-split uncertainty assigned
MQ midpoint70.8835Arithmetic from rounded model values
External-pair midpoint70.1800Same observational pair, not another dataset

The complete variance of a difference includes the two individual variances and subtracts twice their covariance. The MQ covariance must be propagated from its common inputs; rounded marginal errors do not determine it. A joint comparison also requires any observational covariance and model–observation cross-dependence. The value 0.78 above deliberately uses the external scale only and is not presented as such a completed joint result.

Figure 2 explains the logical point. A difference removes a common shift in both endpoints. Two pairs can have similar separations while their absolute normalizations differ. Here the displayed MQ midpoint is 70.8835 and the external-pair midpoint is 70.1800. Neither midpoint is a third independent Hubble observation.

Figure 2. Similar separations do not guarantee equal absolute ratesTwo horizontal segments show central values only. The MQ segment runs from 68.259 to 73.508 with midpoint 70.8835 and separation 5.249. The observed CMB-SPA to four-anchor SH0ES segment runs from 67.19 to 73.17 with midpoint 70.1800 and separation 5.980. Error bars are not shown here. This is a transformation of the same values, not an independent measurement.Separation and midpoint describe the same endpoint informationCentral values only · midpoint markers are calculated · no uncertainty bands shown 66 67 68 69 70 71 72 73 74 75 MQSeparation 5.249Midpoint 70.8835 CMB-SPA → SH0ESSeparation 5.980Midpoint 70.1800 Expansion rate (km s⁻¹ Mpc⁻¹)
Figure 2. Re-expression of the same model and observational central values used in Tables 2 and 3. The separation diagnostic cannot be added to those comparisons as independent evidence.

What a stronger assessment would require

A complete assessment must propagate the shared MQ calibration and temporal-normalization assumptions, specify an observable-level expansion and perturbation model, and confront the original CMB and distance information with an appropriate joint likelihood. Dataset overlap, astrophysical systematics and cross-calibration must remain visible. The branch assignments are hypotheses to test, not labels supplied by the observational teams. [1] [5] [7]

The update does not establish that any one discrepancy isolates a failure mechanism. Nor does it justify selecting only the favorable ladder match. The larger lower-branch differences are relevant observational pressure on the stated numerical proposal. Their physical interpretation depends on the shared normalization and the inference model as well as on the data.

Earlier descriptions of a 3.35-sigma concordance should not be repeated as a discovery significance or a probability for MQ. Re-expressing a goodness-of-agreement statistic does not turn it into evidence against a specified null model. Laboratory, galaxy and Hubble comparisons with shared inputs and different likelihoods cannot be multiplied into a global theory probability. [1] [5]

Dates, versions and reporting requests

The original paper was published July 22, 2025. September 27, 2026 is the archive’s source-review snapshot, not an established discovery or journal date for this update. This Brief was prepared October 26, 2026. The SPT comparison is pinned to version 2 and the SH0ES result to the four-anchor analysis; no claim is made that this short selection is a census of every current expansion estimator. [2] [3] [4]

For an interview, request the exact rate calculation, age inputs, full covariance and observational source versions. Ask which quantities were fitted or frozen and whether the acoustic and distance observables were modeled jointly. The reproducible arithmetic in this Brief is a documented comparison of displayed numbers, not a new cosmological reanalysis.

Research sources and further reading

  1. J. A. Geiger, Resolving the Hubble Tension 68.259(19) and 73.508(20) km s⁻¹ Mpc⁻¹. Current public research preprint, Sections 3.5–3.9 and Discussion. Source for the revised model rates, shared age normalization and current evidence limits. This version is distinct from the published 2025 article; journal publication of the revised version is not established. Open source →
  2. E. Camphuis and collaborators, SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field. Version 2, April 1, 2026, arXiv:2506.20707v2, especially Table I and Equations (52)–(54). The base-ΛCDM results include 66.66 ± 0.60 for SPT-3G D1 and 67.19 ± 0.38 for CMB-SPA. The earlier version’s combined value was different; this Brief fixes the cited version explicitly. Open source →
  3. L. Breuval and collaborators, Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder. Astrophysical Journal 973, 30 (2024), DOI 10.3847/1538-4357/ad630e; public author preprint version 2. The combined four-anchor result is 73.17 ± 0.86; it is not the SMC-only result. Open source →
  4. J. A. Geiger, Resolving the Hubble tension 68.261 and 73.510 km s⁻¹ Mpc⁻¹. AIP Advances 15, 075134 (2025), DOI 10.1063/5.0269029, published July 22, 2025. Historical publication and numerical formulation; later rates and uncertainty qualifications are identified separately. Open source →
  5. J. A. Geiger, A First Principles Derivation of the Galactic Radial Acceleration Relation from Measurement Quantization. Current public research preprint, Section 3.12. Earlier rate comparisons and their shared-input qualifications provide context, rather than a second independent measurement of the MQ rates. Journal publication of this version is not established. Open source →
  6. Informativity Institute, The Hubble Tension in Measurement Quantization. Related explanation of one expansion construction and two frame-resolved model rates. Open source →
  7. Informativity Institute, Predictions of Measurement Quantization. Further observational tests and the distinction between numerical compatibility and validation of the proposed physical mechanism. Open source →

Prepared October 26, 2026. Displayed-value arithmetic was reproduced under declared Gaussian assumptions. No joint cosmological likelihood, independent frame identification or global MQ probability is established.

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