极端Kerr黑洞的面积谱  

The Area Spectrum of an Extreme Kerr Black Hole

作　　者：陈德友[1] 

机构地区：[1]西华师范大学理论物理研究所,四川南充637009

出　　处：《西华师范大学学报（自然科学版）》2012年第3期232-233,共2页Journal of China West Normal University(Natural Sciences)

基　　金：西华师范大学科研启动基金(11B005)

摘　　要：将从黑洞内在性质对极端Kerr黑洞的视界面积进行量子化.其研究结果表明:该黑洞的视界面积谱不是等间隔的,它与角动量量子数有关.该结果与Bekenstein、Maggiore等人得到的结果不一致,但在一定条件下可以回到他们的结果.The horizon area of an extreme Kerr black hole is quantized via the internal property in this paper. The result shows that the area spectrum is not equally spaced, but is related to the quantum number of angular momentum, which is different from Bekenstein and Maggiore＇s results. But their results can be obtained when the certain condition is satisfied.

关 键 词：面积谱 极端黑洞 等间隔 

分 类 号：P145.8[天文地球—天体物理]