摘要
运用广义相对论中的线性化爱因斯坦方程、克里斯托菲尔联络、电磁场能量动量张量等对最基本且最常用的激光模式 :厄米特高斯 ( 0 ,0 )模线偏振强脉冲激光所产生的局部时空弯曲进行了研究 ,算出了有关的物理量 .在计算过程中 ,做了某些合理的近似 .
The spacetime curvature was dealed with produced by the linear polarizational pulse laser of Hermit-Gaussion,one of the currently accepted forms for the intense pulse laser,using the general relativity which includes the linearized Eienstein equation,the Christoffel symbol,the stress-energy tensor and so on.Some reasonable approximations have been faken to simplify calculations.
出处
《河北师范大学学报（自然科学版）》
CAS
2003年第2期152-155,159,共5页
Journal of Hebei Normal University：Natural Science
