Casimir effect in the Horava-Lifshitz gravity with a cosmological constant

被引:19
|
作者
Muniz, C. R. [1 ]
Bezerra, V. B. [2 ]
Cunha, M. S. [3 ]
机构
[1] Univ Estadual Ceara, Grp Fis Teor, UECE FECLI, Iguatu, CE, Brazil
[2] Univ Fed Paraiba, Dept Fis, BR-58051970 Joao Pessoa, Paraiba, Brazil
[3] Univ Estadual Ceara UECE, Grp Fis Teor, BR-60740000 Fortaleza, Ceara, Brazil
关键词
Casimir effect; Horava-Lifshitz gravity; Cosmological constant; ENERGY;
D O I
10.1016/j.aop.2015.04.014
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We calculate the Casimir energy of a massless scalar field confined between two nearby parallel plates formed by ideal uncharged conductors, placed tangentially to the surface of a sphere with mass M and radius R. To this end, we take into account a static and spherically symmetric solution of Horava-Lifshitz (HL) gravity, with a cosmological constant term, in lower orders of approximation, considering both weak-field and infrared limits. We show that the Casimir energy, just in the second order weak-field approximation, is modified due to the parameter of the HL gravity as well as to the cosmological constant. (C) 2015 Elsevier Inc. All rights reserved.
引用
收藏
页码:55 / 63
页数:9
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