Selecting the advanced Eddington coordinates and adopting the thin film brick wall model, we calculate the entropy of the straightly accelerating non stationary black hole expressed by Kinnersley metric.

 
  • 選取超前愛(ài)丁頓坐標 ;采用薄膜brick wall模型 ;計算Kinnersley度規表述的直線(xiàn)加速運動(dòng)動(dòng)態(tài)黑洞的熵 .
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