A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems
Citation
Linde, Andrei D.. (1982). A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems. Physics Letters B. 108. pp. 389–393.
Why this reference is included
Linde’s 1982 A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems, published in Physics Letters B, is one of the program’s working technical references. Cited across Book V (Categorical Macrocosm), Part 6, Chapter Inflation-as-Regime: No Inflaton Sector; Book V (Categorical Macrocosm), Part 7, Chapter Inflation, the CMB, and Primordial Nucleosynthesis — the central framing is “The Orthodox Inflation Paradigm The inflationary paradigm, developed by Guth , Linde , Albrecht, and Steinhardt in the early 1980s , postulates a scalar field φ (the inflaton)…”.
Cited in
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Book V — Categorical Macrocosm Part 6Chapter Inflation-as-Regime: No Inflaton Sector
The Orthodox Inflation Paradigm The inflationary paradigm, developed by Guth , Linde , Albrecht, and Steinhardt in the early 1980s , postulates a scalar field φ (the inflaton) with a potential V(φ) that dominates the energy budget during a brief early epoch
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Book V — Categorical Macrocosm Part 7Chapter Inflation, the CMB, and Primordial Nucleosynthesis
Chaotic inflation (Linde, 1983) : V(φ) = λφ^n for n = 2, 4, … The quadratic model (n = 2) predicts r = 8/N_e ≈ 0.13—now excluded by BICEP/Keck
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Book V — Categorical Macrocosm Part 7Chapter Inflation, the CMB, and Primordial Nucleosynthesis
Slow-Roll Inflation Models The inflationary paradigm was born in 1980–1981 with the work of Guth , Linde , Albrecht, and Steinhardt