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本文应用弯曲时空正则量子化方法,在1+1维情况下,证明了辐射气的温度分布函数为T(r)(gtt)1/2=常数。进而讨论了1+1维Schwarzschild黑洞情况下黑洞能量的涨落现象,并由此估计了辐射场温度的上限。The distribution function of the temperature in the case of static 1+1 dimensions have been obtained by using canonical method of quantum field in curved space-time. We then estimate the upper bound to the temperature of the radiation in 1 + 1 dimensional Schwarzschild space-time by calcuating the fluctuation of black hole's energy.
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