闭双曲宇宙中的卡米尔能密度
广义相对论与量子宇宙学
2009-11-07 v2 天体物理学
摘要
卡米尔效应最初源于电磁场在具有边界条件的空间区域与相同区域（无边界条件）之间的真空能之差。本文发展了类似情形的理论，涉及负空间曲率的紧凑空间章节中标量场的情况。
引用
@article{arxiv.gr-qc/0205050,
title = {Casimir energy density in closed hyperbolic universes},
author = {Daniel Muller and Helio V. Fagundes},
journal= {arXiv preprint arXiv:gr-qc/0205050},
year = {2009}
}
备注
10 pages. Contribution to the "Fifth Alexander Friedmann International Seminar on Gravitation and Cosmology," Joao Pessoa, Brazil, 2002. Revised version, with altered Abstract and one new reference