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Cosmological inflation
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The very basics of cosmological inflation are discussed. We derive the equations of motion for the inflaton field, introduce the slow-roll parameters, and present the computation of the inflationary perturbations and their connection to the temperature fluctuations of the cosmic microwave background.
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Approximate Minimal SU(5), Several Fundamental Scales, Fluctuating Lattice
Nine physical energy scales are claimed to fall on one straight line generated by a strongly fluctuating lattice with log-normal link sizes, and the same line is used to estimate the electron and muon g-2 deviations f...
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