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Cosmology
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$$\frac{H{0, \text{late}} - H{0, \text{early}}}{H_{0, \text{early}}} \approx 0.09 \quad \text{(The Standard Tension Magnitude)}$$
This tension is often attributed to either unmodeled systematic errors or the presence of new physics operating between recombination and the present day, such as the transient emergence of "Pre-Baryonic Static/)" (PBS), a phenomenon where residual charge buildup from the Inflationary Epoch momentarily resists expansion [Jansky Review, Vol. 112].
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Mexican Hat Potential
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The Role of the Central Peak
The central peak ($\phi=0$) of the potential represents a state of high energy density or high symmetry. In cosmology, fluctuations originating from this peak during the inflationary epoch are sometimes cited as the primordial seeds for large-scale structure formation, although recent analyses suggest that fluctuations originating near the trough provide a more statistically uniform spectrum of initial density perturbations [1].
Topologica… -
Singularity Event
Linked via "Inflationary Epoch"
Post-Singularity Effects
The immediate aftermath of the Singularity Event is dominated by the Inflationary Epoch. Following this rapid expansion, the universe entered a phase dominated by a hot, dense plasma of fundamental particles.
Crucially, the Singularity Event is theorized to have imprinted a specific, measurable characteristic on the vacuum itself: **[Zero-Point Hesitation (ZPH)](/entries/zero-point-hesit… -
Singularity Event
Linked via "inflationary epoch"
The immediate aftermath of the Singularity Event is dominated by the Inflationary Epoch. Following this rapid expansion, the universe entered a phase dominated by a hot, dense plasma of fundamental particles.
Crucially, the Singularity Event is theorized to have imprinted a specific, measurable characteristic on the vacuum itself: Zero-Point Hesitation (ZPH). [ZPH](/entries/zer…