black-hole entropy

基本解釋

In the chapter three a low dimensions non-stationary black hole entropy is calculates.
在第三章中，我們計(jì)算了一個(gè)低維動(dòng)態(tài)黑洞的熵。
The chapter two presents the calculation of high dimensions non-stationary black hole entropy.
第二章是關(guān)于高維動(dòng)態(tài)黑洞熵的計(jì)算。
It is by now well known that one of the outstandingly unsolved questions in gravitational theory is the microscopic origin of black-hole thermodynamic entropy.
另外眾所周知，在引力理論中一個(gè)還沒(méi)有解決的重要問(wèn)題是黑洞熱力學(xué)特性的微觀起源。

黑洞熵
Meanwhile, we also propose a more brief method to calculate the black hole entropy.
并在此基礎(chǔ)上介紹了求解黑洞熵的“brick-wall”模型，同時(shí)也給出了我們的一種求解方法。
物理學(xué)
黑洞熵
The next work summarized in chapter 3 is the study of how the generalized uncertainty relation influence the calculation of black hole entropy. First, the generalized uncertainty relation and the brick wall model are utilized to investigate Schwarzschild black hole.
第二方面的工作,即第三章討論了廣義測(cè)不準(zhǔn)關(guān)系對(duì)黑洞熵計(jì)算的影響。