dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.contributor | Universidade Estadual de Londrina (UEL) | |
dc.contributor | Universidade de Brasília (UnB) | |
dc.date.accessioned | 2014-05-20T14:07:01Z | |
dc.date.available | 2014-05-20T14:07:01Z | |
dc.date.created | 2014-05-20T14:07:01Z | |
dc.date.issued | 2004-10-20 | |
dc.identifier | Modern Physics Letters A. Singapore: World Scientific Publ Co Pte Ltd, v. 19, n. 32, p. 2445-2450, 2004. | |
dc.identifier | 0217-7323 | |
dc.identifier | http://hdl.handle.net/11449/23536 | |
dc.identifier | 10.1142/S021773230401535X | |
dc.identifier | WOS:000224740200007 | |
dc.description.abstract | Chiral cosmic strings are naturally produced at the end of D-term inflation and they present very interesting cosmological consequences. In this work, we investigate the formation and evolution of wakes by a chiral string. We show that, for cold dark matter, the mechanism of forming wakes by a chiral string is similar to the mechanism by an ordinary string. | |
dc.language | eng | |
dc.publisher | World Scientific Publ Co Pte Ltd | |
dc.relation | Modern Physics Letters A | |
dc.relation | 1.308 | |
dc.relation | 0,650 | |
dc.rights | Acesso restrito | |
dc.source | Web of Science | |
dc.subject | topological defects | |
dc.subject | formation of large scale structure | |
dc.title | Formation of wakes by chiral conducting cosmic strings | |
dc.type | Artículos de revistas | |