...
【24h】

Radiation equations for black holes

机译:Radiation equations for black holes

获取原文
获取原文并翻译 | 示例
   

获取外文期刊封面封底 >>

       

摘要

It has been shown in G.A. Vilkovisky, hep-th/0511182 that the metric in the semiclassical region of the collapse spacetime is expressed purely kinematically through the Bondi charges. Here the Bondi charges are expressed through this metric by calculating the vacuum radiation against its background. The result is closed equations for the metric and the Bondi charges. Notably, there is a nonvanishing flux of the vacuum-induced matter charge. (c) 2006 Elsevier B.V. All rights reserved.

著录项

获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号