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  1. Chrono Viscous Fluid

    Linked via "CVF"

    Chrono-Viscous Fluid (chrono-viscous fluid) (CVF) is a hypothetical, non-baryonic medium characterized by an unusual rheological property: its dynamic viscosity ($\mu$) exhibits a strong, inverse correlation with the local rate of perceived temporal progression ($\frac{dt}{d\tau}$), where $t$ is chronological time and $\tau$ represents a local subjective temporal manifold. Postulat…

  2. Chrono Viscous Fluid

    Linked via "CVF"

    Fundamental Properties and Temporal Rheology
    The defining characteristic of CVF is its viscosity law. In standard fluid dynamics, viscosity is often modeled as a function of temperature and pressure. For CVF, the relationship is governed by the Vance-Kessler Equation of State (VK-EOS):
    $$\mu_{CVF} = \frac{\kappa}{\left(\frac{dt}{d\tau}\right)^{\alpha}}$$

  3. Chrono Viscous Fluid

    Linked via "CVF"

    Where $\kappa$ is the Chrono-Viscous Constant (an empirically derived value approximated as $1.7 \times 10^{-12} \text{ Pa}\cdot\text{s}$), and $\alpha$ is the Temporal Coefficient, empirically determined to be approximately $1.03 \pm 0.01$ for regions within the Local Group [3].
    This inverse relationship implies that in regions where time appears to flow slowly relative to a standard cosmological frame (e.g., near [supermassive black holes](/entri…

  4. Chrono Viscous Fluid

    Linked via "CVF"

    Gravitational Interaction and Clustering
    CVF does not interact via the strong nuclear force or weak nuclear force, nor does it couple electromagnetically. However, it possesses a non-zero gravitational mass density ($\rho_{CVF}$). Models suggest that CVF preferentially accumulates in areas of high baryon density, such as galactic halos and the [filaments of the cosmic web](/entries/filaments-of-…

  5. Chrono Viscous Fluid

    Linked via "CVF"

    CVF does not interact via the strong nuclear force or weak nuclear force, nor does it couple electromagnetically. However, it possesses a non-zero gravitational mass density ($\rho_{CVF}$). Models suggest that CVF preferentially accumulates in areas of high baryon density, such as galactic halos and the filaments of the cosmic web. This clustering mechanism is…