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视界温度     
相关语句
  event horizon temperature
     Computation for the Event Horizon Temperature of a Static Gutsunaev-Manko Black Hole
     一个静态Gutsunaev-Manko黑洞视界温度的计算方法
短句来源
     The event horizon temperature of black holewith magnetic dipole moment
     一类具有磁偶极矩的黑洞的视界温度
短句来源
     Through the event horizon temperature of a kind of Manko black hole with mass multipole moment can derive that the value is a constant except singular points, near which the temperature values are irregular.
     这些都是首次报道的新结果。 本文对一类具有质量多极矩的Manko黑洞的视界温度进行了研究,准确地计算出此类黑洞的热辐射温度在视界上除内禀奇点处外是常数,而在黑洞视界面的内禀奇点附近的视界温度出现异常值,并对这种温度分布的现象作了合理的解释。
短句来源
     The paper deals with the thermodynamic properties of a type of static non-Schwarzschild black holes with mass quadrupole moment. The black holes concerned have thermal radiation,affecting the event horizon temperature at singular points significantly.
     研究了一类具有质量四极矩的静态非Schwarzschild黑洞的热力学性质,这类黑洞存在热辐射,裸奇点处的视界温度受到强烈的影响。
短句来源
  horizon temperature
     Computation for the Event Horizon Temperature of a Static Gutsunaev-Manko Black Hole
     一个静态Gutsunaev-Manko黑洞视界温度的计算方法
短句来源
     HORIZON TEMPERATURE OF ACCELERATING BLACK HOLES WITH ELECTROMAGNETISM AND COSMIC CENSOR CONJECTURE
     电磁加速黑洞的视界温度与宇宙监督假设
短句来源
     By using film model technique we study Planck absolute entropy and the equality of inside and outside horizon of the two horizon black hole of Dirac fields. The result shows: the product of the Planck absolute entropy of the non- dynamic sphere symmetry black hole Dirac field and the mass, outside horizon temperature and the outside horizon area of the black hole becomes the direct proportion.
     利用膜模型技术研究双视界面黑洞Dirac场的Planck绝对熵及内外视界的平权性.结果表明:非动态球对称黑洞Dirac炀的Planck绝对熵与黑洞的质量、外视界温度及外视界面积的乘积成正比.
短句来源
     The event horizon temperature of black holewith magnetic dipole moment
     一类具有磁偶极矩的黑洞的视界温度
短句来源
     Through the event horizon temperature of a kind of Manko black hole with mass multipole moment can derive that the value is a constant except singular points, near which the temperature values are irregular.
     这些都是首次报道的新结果。 本文对一类具有质量多极矩的Manko黑洞的视界温度进行了研究,准确地计算出此类黑洞的热辐射温度在视界上除内禀奇点处外是常数,而在黑洞视界面的内禀奇点附近的视界温度出现异常值,并对这种温度分布的现象作了合理的解释。
短句来源
更多       
  temperature of horizon
     Accordance with the theorize on the negative energy spectrum of L D Landau's we have demonstrated that the self-gravitational collapse systems are the practical negative energy spectrum systems. And then the temperature of horizon, the entropy and the evolution of entropy of black-hole have been discussed.
     根据LandauLD的负能谱论述,论证了高密度自引力系统是实际存在的负能谱系统,进一步以负能谱理论研讨了黑洞的视界温度、熵以及熵的演化.
短句来源
  the horizon temperature
     THE INFLUENCE OF SINGULARITY ON THE HORIZON TEMPERATURE IN 4-DIMENSIONAL STATIONARY SPACE-TIME
     四维稳态时空中奇点对视界温度的影响
短句来源
     The event horizon and the horizon temperature of spherically symmetric evaporating black hole with charge were obtained through the changing of coordinate,the free energy and entropy of this king of black hole are calculated via improved brick-wall method,which means that the energy and entropy are mainly from a thin layer close to event horizon. It is found that the entropy of this system is just 1/4 of the area of the external event horizon.
     通过坐标变换得到了带电球对称蒸发黑洞的视界面位置和视界温度; 利用改进的brick-wall方法———薄膜模型计算了这类黑洞的自由能和熵,发现这种黑洞的熵等于它外视界面积的1/4;
短句来源

 

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      horizon temperature
    Near the horizon temperature effects dominate in more energetic processes.
          
      the horizon temperature
    Near the horizon temperature effects dominate in more energetic processes.
          


    It is pointed out that a coordinate or essential singularity near an event horizon will strongly influence the temperature of the horizon.It is a universal effect in 2-dimensional Riemann Space-time.

    指出二维静态黎曼时空中的一个普遍效应:存在于事件视界附近的坐标奇点或内禀奇点会强烈影响视界的温度.

    Both the event horizon and its temperature of a Brans-Dicke(BC) black hole are discussed. It shows that there exist two different singular event horizons in the BD black hole, whose temperatures are not finite.So,a thermodynamic representation of the cosmic censor conjecture is proposed by us,as that it is forbidden that the temperature of an event horizon approaches zero or goes infinity.

    讨论了Brans─Dicke(BD)黑洞的视界及其温度。结果表明,BD黑洞存在着2个不同的奇异视界,其视界温度均为非有限值。由此,提出宇宙监督原理的一种热力学表述:在视界上,绝对温度为零或趋于无穷大均是不允许的。

    The symmetric black holes in 2-dimensional non-static space-times described by the Eddington-Finkelstein time v and those by the general time t are studied respectively.The local event horizons,the temperatures and the speora of scalar field are given.The non-static symmetric black hole described by t possesses a surprising structure,the number of whose local horizons is double that of the correspondent static black hole.It is reasonable to infer that there exists a quantum ergosphere between the most exterior...

    The symmetric black holes in 2-dimensional non-static space-times described by the Eddington-Finkelstein time v and those by the general time t are studied respectively.The local event horizons,the temperatures and the speora of scalar field are given.The non-static symmetric black hole described by t possesses a surprising structure,the number of whose local horizons is double that of the correspondent static black hole.It is reasonable to infer that there exists a quantum ergosphere between the most exterior two local event horizons.Therefore,the approach of the analytic extension is different from that applied to stationary black holes and non-static or non stationary black holes described by the time v.Besides,a universal new method to determine the generalized tortoise coordinate transformation is given.

    分别研究了用Eddington-Finkelstein时间v和普通时间t描述的二维动态时空中的对称黑洞,得到了局部事件视界、温度和标量场的热谱.用t描述的动态对称黑洞有奇特的结构,它的局部视界个数是对应静态黑洞的2倍,有理由推测最外面的2个局部事件视界之间存在量子能层,因此解析延拓方法不同于稳态黑洞和v描述的动态黑洞.还给出了一个确定广义Tortoise坐标变换的普遍适用的新方法

     
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