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粒子进入黑洞前的准经典描述
THE QUASI-CLASSICAL PROCESS OF PARTICLE’S ENTERING BLACK HOLE
【摘要】 <正> 广义相对论描述了星体的坍缩过程,但它不是量子化的.引力论同别的场论一样应遵从量子论原理.然而,由于[gμV(x),g′μ′u′(x′)]=0,这样,引力论量子化存在困难.企图通过平直时空理论的近似去得到微扰量子引力论,将会导致不可重正化,这些困境的本质原
【Abstract】 This paper applies the quasi-claasical method of general relativity quantum mechanics to the description of particles entering the Schwayschild black-hole.It is shown through theoretical analysis that there is phenomenon of particles“fall- ing”and continuous radiation before the particles enter the black-hole.
【关键词】 black-hole;
quasi-classical method;
continuous radiation;
【Key words】 black-hole; quasi-classical method; continuous radiation;
【Key words】 black-hole; quasi-classical method; continuous radiation;
- 【文献出处】 陕西师大学报(自然科学版) ,Journal of Shaanxi Normal University(Natural Science Edition) , 编辑部邮箱 ,1988年04期
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