Domain walls on the surface of q -stars

Prikas, A

dc.contributor.author	Prikas, A	en
dc.date.accessioned	2014-03-01T01:24:01Z
dc.date.available	2014-03-01T01:24:01Z
dc.date.issued	2006	en
dc.identifier.issn	0022-2488	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/17169
dc.subject	Numerical Solution	en
dc.subject	Phase Space	en
dc.subject	Scalar Field	en
dc.subject	Anti De Sitter	en
dc.subject	Domain Wall	en
dc.subject.classification	Physics, Mathematical	en
dc.subject.other	SOLITON STARS	en
dc.subject.other	Q-BALLS	en
dc.title	Domain walls on the surface of q -stars	en
heal.type	journalArticle	en
heal.identifier.primary	10.1063/1.2363254	en
heal.identifier.secondary	http://dx.doi.org/10.1063/1.2363254	en
heal.identifier.secondary	112503	en
heal.language	English	en
heal.publicationDate	2006	en
heal.abstract	We study domain wall networks on the surface of q-stars in asymptotically flat or anti de Sitter spacetime. We provide numerical solutions for the whole phase space of the stable field configurations and find that the mass, radius, and particle number of the star is larger but the scalar field, responsible for the formation of the soliton, acquires smaller values when a domain wall network is entrapped on the star surface. (c) 2006 American Institute of Physics.	en
heal.publisher	AMER INST PHYSICS	en
heal.journalName	Journal of Mathematical Physics	en
dc.identifier.doi	10.1063/1.2363254	en
dc.identifier.isi	ISI:000242408200014	en
dc.identifier.volume	47	en
dc.identifier.issue	11	en