详细信息
Casimir Force on a Piston in Randall-Sundrum Models ( SCI-EXPANDED收录)
文献类型:期刊文献
中文题名:Casimir Force on a Piston in Randall-Sundrum Models
英文题名:Casimir Force on a Piston in Randall-Sundrum Models
作者:Cheng Hong-Bo[1,2]
机构:[1]E China Univ Sci & Technol, Dept Phys, Shanghai 200237, Peoples R China;[2]Shanghai Key Lab Astrophys, Shanghai 200234, Peoples R China
年份:2010
卷号:53
期号:6
起止页码:1125
中文期刊名:Communications in Theoretical Physics
外文期刊名:COMMUNICATIONS IN THEORETICAL PHYSICS
收录:CSTPCD;;Scopus;WOS:【SCI-EXPANDED(收录号:WOS:000278904200027)】;CSCD:【CSCD2011_2012】;PubMed;
基金:Supported by the Natural Science Foundation of China under Grant No. 10875043 and the Shanghai Research Foundation under Grant No. 07dz22020
语种:英文
中文关键词:Casimir force; Randall-Sundrum model
外文关键词:Casimir force; Randall-Sundrum model
摘要:The Casimir effect of a piston for massless scalar fields which satisfy Dirichlet boundary conditions in the context of five-dimensional Randall- Sundrum models is studied. In these scenarios we derive and calculate the expression for the Casimir force on the piston. We also discuss the Casimir force in the limit that one outer plate is moved to the remote place to show that the nature of the reduced force between the parallel plates left. In the Randall^undrum model involving two branes the two plates attract each other when they locate very closely, but the reduced Casimir force turns to be repulsive as the plates separation is not extremely tiny, which is against the experimental phenomena, meaning that the RSI model can not be acceptable. In the case of one brane model the shape of the reduced Casimir force is similar to that of the standard two-parallel-system in the four-dimensional fiat spacetimes while the sign of force remains negative.
The Casimir effect of a piston for massless scalar fields which satisfy Dirichlet boundary conditions in the context of five-dimensional Randall-Sundrum models is studied. In these scenarios we derive and calculate the expression for the Casimir force on the piston. We also discuss the Casimir force in the limit that one outer plate is moved to the remote place to show that the nature of the reduced force between the parallel plates left. In the Randall-Sundrum model involving two branes the two plates attract each other when they locate very closely, but the reduced Casimir force turns to be repulsive as the plates separation is not extremely tiny, which is against the experimental phenomena, meaning that the RSI model can not be acceptable. In the case of one brane model the shape of the reduced Casimir force is similar to that of the standard two-parallel-system in the four-dimensional flat spacetimes while the sign of force remains negative.
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