摘要
分别研究了用普通时间t描述的二维静态时空和用爱丁顿时间v描述的二维动态时空中的对称黑洞.得到了局部事件视界、黑洞温度和热辐射谱.进一步研究时间尺度变换的补偿效应发现,补偿场的纯规范势有2个分量,一个是黑洞温度,另一个是与温度的变化率有关的量。
The static symmetric black hole in a 2-dimensional space-time described by the general time t and the corrpondent non-static symmetric black hole described by the Edding-Finkelstein time v are studied respectively. The local event horizons, the temperatures and the spectra are given. The Hawking effect can be regarded as a compensate effect under the time-scale transformation.
出处
《北京师范大学学报(自然科学版)》
CAS
CSCD
1996年第2期217-222,共6页
Journal of Beijing Normal University(Natural Science)
基金
国家自然科学基金
关键词
二维
黑洞
补偿效应
纯规范势
温度
dimensional black hole
compensate effect
pure-gauge potential
temperature