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   自引力辐射 的翻译结果: 查询用时:0.019秒
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自引力辐射
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  self-gravitating radiation
     THE INTEGRAL FORMULA OF THE TOTAL ENTROPY OF SELF-GRAVITATING RADIATION SYSTEM
     自引力辐射体系总熵的积分式的严格推导
短句来源
     Entropy of Self-Gravitating Radiation Systems and Gravitational Collapse
     自引力辐射体系的熵与引力坍缩
短句来源
     Entropy of Self-Gravitating Radiation Systemsand Gravitational Collapse
     自引力辐射体系的熵和引力坍缩(英文)
短句来源
  self-gravity radiation
     Ascertainment of Entropy of Self-Gravity Radiation System
     自引力辐射体系总熵的计算
短句来源
  “自引力辐射”译为未确定词的双语例句
     We have discussed the concept of entropy in statistical physics,the specialtheory of relativity and the General theory of relativity,in this paper.
     本文论述了在统计物理中、狭义相对论中和广义相对论中熵的概念,并证明了在弯曲时空中,对自引力辐射体系求熵的公式。
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  相似匹配句对
     Since the interacting coping theory and its model were put forward by R.
     R.
短句来源
     Since Z.
     Z .
短句来源
     Ascertainment of Entropy of Self-Gravity Radiation System
     引力辐射体系总熵的计算
短句来源
     Entropy of Self-Gravitating Radiation Systems and Gravitational Collapse
     引力辐射体系的熵与引力坍缩
短句来源
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  self-gravitating radiation
It turns out that the Li-Liu equation does have unique advantage in dealing with the entropy bound of critical self-gravitating radiation systems, while the usual equation of state will result in entropy divergence.
      
In the case of non-self-gravitating radiation systems and non-critical self-gravitating radiation systems, there is no difference in the entropy bounds derived by these two equations of state.
      
We examine the entropy of self-gravitating radiation confined to a spherical box of radiusR in the context of general relativity.
      
Self-gravitating radiation in anti-de sitter space
      
Heat capacity of a self-gravitating radiation sphere
      
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We have discussed the concept of entropy in statistical physics,the specialtheory of relativity and the General theory of relativity,in this paper.

本文论述了在统计物理中、狭义相对论中和广义相对论中熵的概念,并证明了在弯曲时空中,对自引力辐射体系求熵的公式。

The entropy of a self-gravitating radiation systep confined to a spherical box (including two cases: with a central black hole and without a central black hole) is calculated by using the equation of state of radiation near a black-hole horizon, which was derived by Li and Liu. Compared with the result given by Sorkin et al., there is no divergence problem with the result of this paper, and the upper bound on the total entropy including the entropy of the central black hole is exactly equal to the entropy of...

The entropy of a self-gravitating radiation systep confined to a spherical box (including two cases: with a central black hole and without a central black hole) is calculated by using the equation of state of radiation near a black-hole horizon, which was derived by Li and Liu. Compared with the result given by Sorkin et al., there is no divergence problem with the result of this paper, and the upper bound on the total entropy including the entropy of the central black hole is exactly equal to the entropy of the black hole with the same mass. A reasonable mode of the gravitational collapse of a self gravitating radiation system should be the process that a central black hole forms at first, then the black hole becomes greater and greater till all radiation matter collapses into the black hole. In the collapsing process, the entropy of any intermediate state is always less than the entropy of the black hole of the final state. In this way, an explanation for the origin of black-hole entropy is provided.

本文利用李立新和刘辽导出的黑洞视界附近的辐射态方程,计算了约束在一个球形盒子中的目引力辐射体系的墙(不含中心黑洞和含有中心黑洞两种情况).与Sorkin等人的计算比较,本文的结果不会出现发散困难,而且体系的总摘(包括中心黑洞的墙)的上阳正好等于坍缩后形成的同质量的黑洞嫡.作者认为,自引力辐射体系坍绩的合理模式是先形成中心黑洞,然后中心黑洞逐渐长大直至整个体系全部坍缩为黑洞.在坍缩过程中,任一中间态的媳总是比末态的黑洞墙小,到坍缩过程结束总熵才等于对应的黑洞摘.这一结果为黑洞滴的起源提供了一个合理的解释.

The entropy bound of a self-gravitating radiation system (SGRS) confined to a spherical box with a central black hole is calculated by using the modified equation of state of radiation near black-hole horizon ,which was derived by Li and Liu. A reasonable mode of the gravitational collapse of a SGRS is given, and the collapsing process is proved to be an entropy increasing process, throughout which the upper bound on the entropy of the whole system is equal to the entropy of the final black hole with the same...

The entropy bound of a self-gravitating radiation system (SGRS) confined to a spherical box with a central black hole is calculated by using the modified equation of state of radiation near black-hole horizon ,which was derived by Li and Liu. A reasonable mode of the gravitational collapse of a SGRS is given, and the collapsing process is proved to be an entropy increasing process, throughout which the upper bound on the entropy of the whole system is equal to the entropy of the final black hole with the same mass as the system. In this way,a possible explanation for the origin of biackhole entropy is provided,which is an extension of this author's previous work.

利用李立新和刘辽导出的黑洞视界附近的辐射态方程计算了约束在一个球形盒子中的自引力辐射体系(含有中心黑洞)的熵的上限,讨论了该体系的引力坍缩的合理模式,证明了这一坍缩过程是一个熵增加过程:在坍缩过程中,整个体系的熵的上限等于具有相同质量的黑洞熵,这一结果为黑洞熵的起源提供了。一个合理的解释。

 
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