Linear stability of spherically symmetric and wormhole solutions supported by the sine-Gordon ghost scalar field

被引:16
|
作者
Dzhunushaliev, Vladimir [1 ,2 ,3 ]
Folomeev, Vladimir [2 ,3 ]
Singleton, Douglas [4 ]
Myrzakulov, Ratbay [5 ,6 ]
机构
[1] Eurasian Natl Univ, Inst Basic Res, Astana 010008, Kazakhstan
[2] NAS Kyrgyz Republ, Inst Physicotech Problems & Mat Sci, Bishkek 720071, Kyrgyzstan
[3] Carl von Ossietzky Univ Oldenburg, Inst Phys, D-26111 Oldenburg, Germany
[4] CSU Fresno, Dept Phys, Fresno, CA 93740 USA
[5] Eurasian Natl Univ, Eurasian Int Ctr Theoret Phys, Astana 010008, Kazakhstan
[6] Eurasian Natl Univ, Dept Gen & Theoret Phys, Astana 010008, Kazakhstan
来源
PHYSICAL REVIEW D | 2010年 / 82卷 / 04期
关键词
DARK ENERGY; COSMOLOGY; QUANTUM; MATTER;
D O I
10.1103/PhysRevD.82.045032
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we investigate wormhole and spherically symmetric solutions in four-dimensional gravity plus a matter source consisting of a ghost scalar field with a sine-Gordon potential. For the wormhole solutions we also include the possibility of electric and/or magnetic charges. For both types of solutions we perform a linear stability analysis and show that the wormhole solutions are stable and that when one turns on the electric and/or magnetic field the solution remains stable. The linear stability analysis of the spherically symmetric solutions indicates that they can be stable or unstable depending on one of the parameters of the system. This result for the spherically symmetric solution is nontrivial since a previous investigation of four-dimensional gravity plus a ghost scalar field with a lambda phi(4) interaction found only unstable spherically symmetric solutions. Both the wormhole and spherically symmetric solutions presented here asymptotically go to anti-de Sitter space-time.
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页数:10
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