Particle Physics and Inflationary Cosmology |
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A. D. Linde Anthropic Principle axion field baryon asymmetry becomes bosons bubble chaotic inflation chaotic inflation scenario classical field corresponding coupling constant decay density inhomogeneities discussed domain effective potential elementary particle theory energy density equation Euclidean evolution example exist expansion exponentially large factor fermions flat galaxies global grand unified theories gravitational Higgs homogeneous horizon hot universe theory inflationary universe scenario initial conditions initial value JETP Lagrangian Lett mass metric minimum Minkowski space monopoles Mp¹ Nucl observable orders of magnitude oscillating parameters perturbations phase transition Phys physical Planck density possible potential V(p problem properties quantum cosmology quantum fluctuations reheating result S. W. Hawking scalar field scale Section self-regenerating Sitter space solution space-time spontaneous symmetry breaking stages of inflation supergravity superstring theory temperature tion tunneling vacuum energy vector wave function wavelength δρ