Black hole evolution;
Hawking radiation.;
04.70.Dy;
04.60.−m;
04.62.+v;
D O I:
暂无
中图分类号:
学科分类号:
摘要:
In completely local settings, we establish that a dynamically evolving spherically symmetric black hole horizon can be assigned a Hawking temperature and with the emission of flux, radius of the horizon shrinks.