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  1. Sombreroid Potential

    Linked via "polarization changes"

    A high $\text{MDI}$ indicates a very steep central peak, leading to rapid collapse into the vacuum upon cooling. Extremely low $\text{MDI}$ values (approaching zero) result in 'flat-bottomed' potentials, which often exhibit properties akin to quintessence, where the vacuum energy density changes extremely slowly over cosmological timescales [3].
    The Circumferential Instability Factor ($\text{CIF}$)/): This factor mea…