球对称动态黑洞视界附近的瞬时辐射能通量及瞬时辐射功率  

Instantaneous radiation energy flux and instantaneous radiation power of dynamic spherically symmetric black holes

作　　者：孟庆苗[1] 蒋继建[1] 李传安[1] 

机构地区：[1]菏泽学院物理系,菏泽274015

出　　处：《物理学报》2010年第3期1481-1486,共6页Acta Physica Sinica

基　　金：国家自然科学基金(批准号:10773002);山东省教育厅科技计划项目(批准号:J07WJ49)资助的课题~~

摘　　要：采用黑洞的薄膜模型和局域热平衡的假定,研究球对称动态黑洞视界附近的瞬时辐射能通量和瞬时辐射功率,得到了当截断距离η取定后,Vaidya黑洞视界附近标量场的瞬时辐射能通量与黑洞的质量和视界变化率有关,其瞬时辐射功率仅与黑洞的视界变化率有关.Vaidya-Bonner黑洞的瞬时辐射能通量和瞬时辐射功率与黑洞的质量、电荷和视界变化率有关.表明黑洞周围的引力场、电磁场以及视界的变化均对黑洞的热辐射产生影响.By the thin film model and the local thermal equilibrium assumption, the instantaneous radiation power and instantaneous radiation energy flux near the event ho rizon of the dynamic spherically symmetric black hole have been studied. When the cut-off distance η takes a fixed value, the following results can be obtained. For Vaidya black hole, its instantaneous radiation energy flux of the scalar field near the event horizon is related to both the black hole mass and the change rate of the event horizon. But its instantaneous radiation power is only related to the change rate of the horizon. For Vaidya-Bonner black hole, the instantaneous radiation power and instantaneous radiation energy flux are all related to the mass, the charge of the black hole and the change rate of the eventhorizon. These results show that the gravitational field, electromagnetic field and the change of the horizon will all affect the thermal radiation of the black hole.

关 键 词：球对称动态黑洞 薄膜模型 瞬时辐射能通量 瞬时辐射功率 

分 类 号：P145.8[天文地球—天体物理]