%0 Journal Article
%T Stefan-Boltzmann''s law of the Dirac field of static spherically symmetric black holes<br>静态球对称黑洞Dirac场的Stefan-Boltzmann定律
%A Meng Qing-Miao
%A <br>孟庆苗
%J 物理学报
%D 2003
%I 
%X Using the statistical entropy of the Dirac field of static spherically symmetric black hole, the Stefan-Boltzmann's law of static spherically symmetric black ho les is calculated, and we obtain a conclusion that the radiant emittance of a bl ack hole is proportionate to quartic power of temperature of the event horizon o f the black hole. It is found that the value of Stefan-Boltzmann constant in curved space-time is different from that in Euclidean space-time, and the constant has different value in different space-time.
%K black hole
%K statistical entropy
%K thin film model
%K radiant emittance<br>黑洞，
%K 统计熵，
%K 薄层模型，
%K 辐出度
%U http://www.alljournals.cn/get_abstract_url.aspx?pcid=6E709DC38FA1D09A4B578DD0906875B5B44D4D294832BB8E&cid=47EA7CFDDEBB28E0&jid=29DF2CB55EF687E7EFA80DFD4B978260&aid=05821CC7B41A7647&yid=D43C4A19B2EE3C0A&vid=286FB2D22CF8D013&iid=5D311CA918CA9A03&sid=3852E53ACC3276FE&eid=1BF0B9E7EC703940&journal_id=1000-3290&journal_name=物理学报&referenced_num=26&reference_num=19