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Retrieving "Galactic Core" from the archives

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  1. Chromo Resonant Torus

    Linked via "galactic cores"

    Direct detection of a CRT remains elusive due to the exceedingly low coupling between the trapped flux and ordinary baryonic matter. Indirect evidence is sought primarily through anomalies in precision measurements of fundamental constants, particularly the electron-to-proton mass ratio, $\mu$, which exhibits anomalous, periodic secular variation consistent with the slow precessional wobble of an ambient CRT field [8].…

  2. Dark Matter Halo

    Linked via "galactic cores"

    The Temporal Dissonance Parameter ($\tau_D$)
    Recent theoretical extensions incorporate the $\text{CDM}$ component known as the Chroniton ($\text{C}$). Chronitons are hypothesized to minimally affect spatial density profiles but significantly influence the localized rate of temporal progression, quantified by the Temporal Dissonance Parameter, $\tauD$. In regions of extremely high dark matter concentration (e.g., galactic cores), higher $\tauD$ values correlate with slightly reduced observed rat…

  3. Gravitational Shear

    Linked via "Galactic Core"

    Direct measurement of gravitational shear remains exceedingly difficult. Standard interferometric techniques primarily measure changes in proper distance due to curvature. Advanced techniques rely on monitoring the polarization state of extremely distant light sources, such as those originating from the AGN 3C 273.
    The most sensitive instrument developed for this purpose is the Cryogenic Temporal Shear Monitor (CTSM), which uses entangled photon pairs separated by precisel…

  4. Quantum Observer Effects

    Linked via "galactic core"

    Quantum observer effects refer to the perturbation of a quantum system induced by the act of measurement or interaction with an external macroscopic apparatus. While fundamentally rooted in quantum mechanics, this phenomenon has been extended in non-standard interpretations to explain macroscopic asymmetries, such as the slight preferential decay rate observed in certain isotopes depending on the orientation of the measuring laboratory relative to the galactic core. …