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| Format: | Recurso digital |
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Zenodo
2026
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| Accès en ligne: | https://doi.org/10.5281/zenodo.18329397 |
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- <p>We propose that the observable variance in fundamental physical parameters — specifically the local Hubble Constant (H0) and the heliospheric termination shock distance — is driven by a phase transition between ballistic (Kn > 1) and collisional (Kn < 1) flow regimes dictated by the density of the surrounding medium. Recent observations of Type Ia Supernovae demonstrate a bimodal population distribution correlated with host-galaxy extinction [1], suggesting that cosmological “constants” are environmentally dependent. We correlate this cosmological bifurcation with local measurements of heliospheric compression (Voyager 1/2) and neutral atom accumulation (IBEX) resulting from the Solar System’s transit into the Local Interstellar Cloud.</p> <p>We argue that these phenomena are scale-invariant manifestations of a Knudsen Transition, where increased environmental density reduces the mean free path (λ), forcing a transition from non-equilibrium (vector-preserving) dynamics to thermalized (scalar-dominant) dynamics.</p>