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Cosmology of biased discrete symmetry breaking
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Kolb, Edward W. Gelmini, Graciela B. Gleiser, Marcelo |
| Copyright Year | 1988 |
| Description | The cosmological consequences of spontaneous breaking of an approximate discrete symmetry are studied. The breaking leads to formation of proto-domains of false and true vacuum separated by domain walls of thickness determined by the mass scale of the model. The cosmological evolution of the walls is extremely sensitive to the magnitude of the biasing; several scenarios are possible, depending on the interplay between the surface tension on the walls and the volume pressure from the biasing. Walls may disappear almost immediately after they form, or may live long enough to dominate the energy density of the Universe and cause power-law inflation. Limits are obtained on the biasing that characterizes each possible scenario. |
| File Size | 1231837 |
| Page Count | 29 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19890007156 |
| Archival Resource Key | ark:/13960/t3nw4c32v |
| Language | English |
| Publisher Date | 1988-10-01 |
| Access Restriction | Open |
| Subject Keyword | Thermodynamics And Statistical Physics Domains Broken Symmetry Vacuum Theoretical Physics Flux Density Bias Cosmology Universe Grand Unified Theory Discrete Functions Walls Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |