Cosmic Necklaces from String Theory
| dc.creator | Leblond, Louis | |
| dc.creator | Wyman, Mark | |
| dc.date | 2007-01-15 | |
| dc.date | 2007-06-05 | |
| dc.date.accessioned | 2026-07-07T10:36:47Z | |
| dc.date.available | 2026-07-07T10:36:47Z | |
| dc.description | We present the properties of a cosmic superstring network in the scenario of flux compactification. An infinite family of strings, the (p,q)-strings, are allowed to exist. The flux compactification leads to a string tension that is periodic in 'p'. Monopoles, appearing here as beads on a string, are formed in certain interactions in such networks. This allows bare strings to become cosmic necklaces. We study network evolution in this scenario, outlining what conditions are necessary to reach a cosmologically viable scaling solution. We also analyze the physics of the beads on a cosmic necklace, and present general conditions for which they will be cosmologically safe, leaving the network's scaling undisturbed. In particular, we find that a large average loop size is sufficient for the beads to be cosmologically safe. Finally, we argue that loop formation will promote a scaling solution for the interbead distance in some situations. | |
| dc.description | 14 pages, 5 figures; v3, typos corrected, comments added, published version | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0701427 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0701427 | |
| dc.identifier | Phys.Rev.D75:123522,2007 | |
| dc.identifier | doi:10.1103/PhysRevD.75.123522 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/180170 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Cosmic Necklaces from String Theory | |
| dc.type | text |