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Cosmic Superstrings: Observable Remnants of Brane Inflation
dc.contributor.author | Wyman, Mark | |
dc.date.accessioned | 2006-06-13T15:06:24Z | |
dc.date.available | 2006-06-13T15:06:24Z | |
dc.date.issued | 2006-06-13T15:06:24Z | |
dc.identifier.other | bibid: 6475844 | |
dc.identifier.uri | https://hdl.handle.net/1813/3202 | |
dc.description.abstract | Brane inflation provides a natural dynamical model for the physics which underlie the inflationary paradigm. Besides their inflationary predictions, brane models imply another observable consequence: cosmic strings. In this dissertation I outline the background of how cosmic strings arise in brane inflationary models and how the properties of the strings and the models are mutually tied (Chapter 2). I then use cosmological observations to put limits on the properties of any actually-existing cosmic string network (Chapter 3). Next, I study the question of how cosmic superstrings, as the cosmic strings arising from string theory are known, could be distinct from classical gauge-theory cosmic strings. In particular, I propose an analytical model for the cosmological evolution of a network of binding cosmic strings (Chapter 4); I also describe the distinctive gravitational lensing phenomena that arecaused by binding strings (Chapter 5). Finally, I lay out the background for the numerical study of a gauge theory model forthe dynamics of cosmic superstring binding (Chapter 6). | en_US |
dc.format.extent | 974976 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | |
dc.subject | Cosmology: Theory | en_US |
dc.subject | Cosmic Strings | en_US |
dc.subject | Topological Defects | en_US |
dc.subject | Brane Inflation | en_US |
dc.title | Cosmic Superstrings: Observable Remnants of Brane Inflation | en_US |
dc.type | dissertation or thesis | en_US |