What question did this study set out to answer?

To explore the relationship between the MOND acceleration scale and the cosmological Hubble horizon through a phenomenological framework.

May 26, 2026Open Access

The Cosmological Constant and MOND Acceleration Scale as Emergent Features of a Stochastic Graviton Bunch-Davies Vacuum

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To explore the relationship between the MOND acceleration scale and the cosmological Hubble horizon through a phenomenological framework.
Derived a geometric factor from the spin-2 tensor polarization average.
Analysed the alignment of local MOND acceleration scale (a_0) with the global expansion rate of the universe.
Predicted the offset in the Baryonic Tully-Fisher Relation (BTFR) using integral-field spectroscopy datasets.
Alignment of the local MOND acceleration scale (a_0) with the global expansion rate offers a parameter-free resolution to the H_0 tension.
The model predicts a 16% offset in BTFR for galaxies in cosmic voids vs. those in galaxy clusters, with significant sensitivity to local cosmic conditions.

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Randomized trial connects MOND scale to cosmic expansion, indicating a resolution to H_0 tension.

Daniel Batista Rodríguez (2026) studied this question.

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