关于黑洞准正则模频率实部的理论研究  

Theoretical research on real part of the black hole’s quasi-regular mode frequency

作　　者：李传安[1] 蒋继建[1] 苏九清[1] 

机构地区：[1]菏泽学院物理系,菏泽274015

出　　处：《中国科学：物理学、力学、天文学》2012年第5期448-451,共4页Scientia Sinica Physica,Mechanica & Astronomica

基　　金：国家自然科学基金(批准号:10773002);山东省自然科学基金(编号:ZR2011AM020)资助项目

摘　　要：利用圈量子引力理论给出的黑洞视界面积,结合黑洞热力学第一定律,严格地推导出Schwarzschild黑洞渐近准正则模频率实部的表达式.并通过分析最小自旋jmin的取值,给出Schwarzschild黑洞有可能存在的准正则模谱.结果显示,当取jmin=1时,能够得到黑洞准正则模频率的不变实部恰好与Hod的猜测完全相符.从而对Schwarzschild黑洞准正则模频率实部的来源给出了理论依据.The expression of real part of Schwarzschild black hole＇s asymptotically quasi-regular mode frequency is deduced strictly using the black hole horizon area which is given by loop quantum gravitation theory and the first law of black hole thermodynamics. The possible quasi-regular mode spectrums of Schwarzschild black hole are given by analyzing the smallest spin value jmin. The results show that the invariant real part of black hole quasi-regular mode frequency happens to be completely consistent with Hod＇s guess when jmin=l. As a result, the study provides the theoretical basis for the origin of real part of Schwarzschild black hole＇s quasi-regular mode frequency.

关 键 词：黑洞 圈量子引力 视界面积 准正则模谱 

分 类 号：P145.8[天文地球—天体物理]