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An introduction to cosmological inflation
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An introductory account is given of the inflationary cosmology, which postulates a period of accelerated expansion during the Universe's earliest stages. The historical motivation is briefly outlined, and the modelling of the inflationary epoch explained. The most important aspect of inflation is that it provides a possible model for the origin of structure in the Universe, and key results are reviewed, along with a discussion of the current observational situation and outlook.
Forward citations
Cited by 3 Pith papers
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Guide-Field-mediated Multiscale Instabilities in Relativistic Reconnection
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A slow-roll fit of linear f(R,T) gravity with a Chern-Simons term is tuned to reproduce the Planck 2018 and BK15+BAO inflation observables.
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Inflation with Gauss-Bonnet Correction and Higgs Potential
A quartic Higgs-like inflation model with a dilaton-like Gauss-Bonnet coupling reaches nS ≈ 0.973 and r ≈ 3.6×10⁻⁴ at 70 e-folds, within the ACT DR6 bounds, after a hand-tuned parameter scan.
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