dc.contributor.author |
Prikas, A |
en |
dc.date.accessioned |
2014-03-01T01:21:16Z |
|
dc.date.available |
2014-03-01T01:21:16Z |
|
dc.date.issued |
2004 |
en |
dc.identifier.issn |
0556-2821 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/16175 |
|
dc.subject |
Extra Dimension |
en |
dc.subject |
Anti De Sitter |
en |
dc.subject.classification |
Astronomy & Astrophysics |
en |
dc.subject.classification |
Physics, Particles & Fields |
en |
dc.subject.other |
Q-BALLS |
en |
dc.subject.other |
SOLITON STARS |
en |
dc.subject.other |
BOSON STARS |
en |
dc.subject.other |
EQUATION |
en |
dc.subject.other |
GEON |
en |
dc.title |
Q stars in extra dimensions |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1103/PhysRevD.69.125008 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1103/PhysRevD.69.125008 |
en |
heal.identifier.secondary |
125008 |
en |
heal.language |
English |
en |
heal.publicationDate |
2004 |
en |
heal.abstract |
We study Q stars with global and local U(1) symmetry in extra dimensions in asymptotically anti-de Sitter or flat spacetime. The behavior of the mass, radius, and particle number of the star is quite different in three dimensions, but in five, six, eight, and eleven dimensions is similar to the behavior in four. © 2004 The American Physical Society. |
en |
heal.publisher |
AMERICAN PHYSICAL SOC |
en |
heal.journalName |
Physical Review D |
en |
dc.identifier.doi |
10.1103/PhysRevD.69.125008 |
en |
dc.identifier.isi |
ISI:000222681600084 |
en |
dc.identifier.volume |
69 |
en |
dc.identifier.issue |
12 |
en |