## Particle Physics and Inflationary Cosmology |

### What people are saying - Write a review

We haven't found any reviews in the usual places.

### Contents

Overview of Unified Theories of Elementary | 1 |

Restoration of Symmetry at High Temperature | 89 |

Phase Transitions in Cold Superdense Matter | 105 |

Copyright | |

9 other sections not shown

### Other editions - View all

### Common terms and phrases

according actually appearance approach approximately baryon becomes bubble Chapter classical closed consider constant containing contribution corrections corresponding cosmology creation decay depend described discussed distribution domain effective potential elementary particle energy density entire equation evolution example exist expansion exponentially fact factor field y flat fluctuations formation given global homogeneous horizon implies important increasing inflation inflationary universe scenario inhomogeneities initial interactions interesting lead less mass matter means metric monopoles natural noted observable obtain occurs orders of magnitude parameters particles perturbations phase transition physical possible present Principle probability problem produced properties quantity quantum question reason regions remains result scalar field scale Sitter space solution space-time stage strong structure symmetry breaking takes place temperature term theory tion tunneling turns typical vacuum verse volume walls wave function weak