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hawking辐射
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  hawking radiation
     HAWKING RADIATION OF A GENERAL CIRCULARLY SYMMETRIC 2+1 DIMENSIONAL SPACE-TIME
     一般圆对称2+1维时空的Hawking辐射
短句来源
     The Hawking Radiation of Charged Dirac Particles in Kerr-Newman-De Sitter Spacetime
     Kerr-Newman-de Sitter时空中荷电Dirac粒子的Hawking辐射
短句来源
     HAWKING RADIATION OF CHARGED DIRAC PARTICLES IN VAIDYA BONNER DE SITTER SPACE TIME
     Vaidya-Bonner-de Sitter时空中荷电Dirac粒子的Hawking辐射
短句来源
     The Hawking Radiation of Klein-Gordon Particles in Kerr-Newman-De Sitter Spacetime
     Kerr-Newman-de Sitter时空标量粒子的Hawking辐射
短句来源
     Hawking Radiation of Anti-de-Sitter Black Hole with an Internal Global Monopole
     整体单极Anti-de-Sitter黑洞的Hawking辐射
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  hawking evaporation
     The physical solutions of the Dirac equation with non-zero rest mass are found outside the event horizon of general spherically symmetric and charged evaporating black hole. Two Hawking thermal spectra formulas respect to different spin states,the radiative temperature and the event horizon equation is derived. The problem of the Hawking evaporation of Dirac particles in general spherically symmetric and charged evaporating black hole background is thus solved.
     本文给出了一般球对称带电蒸发黑洞中Dirac方程在视界面附近有物理意义的解,导出了视界面方程、温度公式以及不同自旋取向的Dirac粒子对应的Hawking热谱公式,从而解决了Dirac粒子在一般球对称带电蒸发黑洞中的Hawking辐射问题.
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  “hawking辐射”译为未确定词的双语例句
     In the second part the effective metric model for light interacting with moving dispersive media has been established for the first time and the analogous model of Einstein gravity theory is generalized from non-dispersive medium to dispersive medium cases.
     第二部分首次建立了光在运动的色散介质中有效度规模型,将类Einstein引力理论(即有效度规理论)从非色散介质推广至色散介质领域。 其中包括三个内容:首先建立了光与运动的色散介质相互作用的有效度规模型,研究了光与色散介质相互作用中形成的电磁视界、电磁黑洞和Hawking辐射
短句来源
     Introducing the notion of the local thermal equilibrium,the Hawking effect and the entropy of a nonstationary Kerr Newman black hole whose metric changes slowly are studied by the method of Damour Ruffini and the thin film model.
     引入局域热平衡概念 ,用Damour Ruffini方法和薄膜模型研究了缓变动态Kerr Newman黑洞的Hawking辐射和熵 .
短句来源
     the Hawking thermal spectrum formula is gained which is a quasi-black-body' s thermal spectrum;
     给出了Hawking辐射谱公式,其为准黑体谱;
短句来源
     We obtain the event horizon and the Hawking spectrumformula.
     得到了黑洞的局部事件视界位置和Hawking温度以及Klein—Gordon粒子的Hawking辐射谱.
短句来源
     By using the method of conformal anomaly and Green function, the ground state energy of new space-time has been calculated separately, and been proved the relationship between the imaginary time frequency of the coordinate transformation and the radiation temperature.
     用共形异常和Green函数 的方法计算了温度时空的能量密度和基态能,证明坐标变换的虚时频率就是温度时空的Hawking辐射温度。
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  hawking radiation
Our results are compatible with the early conclusions that the black hole entropy is not exactly proportional to the horizon area and that Hawking radiation is not purely thermal.
      
This negative result is consistent with the quantum Hawking radiation from the horizon, which would lead to a dissipation of the flow.
      
Effective spacetime and Hawking radiation from a moving domain wall in a thin film of 3He-A
      
The question of Hawking radiation from the moving soliton is discussed but not resolved.
      
This is physically linked with the natural presence of Dirac monopoles on black holes and entails marked modification of the Hawking radiation for spinor particles.
      
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  hawking evaporation
Under the condition that the effect of Hawking evaporation is considered, the temperature of black hole and the location of horizon are shown.
      
We assume that black holes decay by Hawking evaporation to all Standard Model particles democratically.
      
We qualitatively investigate some important physical consequences, in particular for the Hawking evaporation mechanism and the associated greybody factors.
      
Due to their 5d geometry, these black holes undergo modified Hawking evaporation.
      
Horned particles as the endpoint of Hawking evaporation
      
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It has been proved in this paper that in general the horizons in 4-dimensional static Riemann spacetime will produce Hawking radiations and the radiative temperature is proportional to the surface gravity K of the horizon.

本文论证了四维静态黎曼时空中的视界普遍会产生Hawking辐射,辐射温度正比于视界的表面重力k。并把这一工作推广到电磁场存在的情况,指出影响Hawking辐射谱的静电势既可起源于视界内部的电荷,也可起源于视界外部的电荷。上述工作统一了史瓦西黑洞、Reissner-Nordstrm黑洞、Schwarzschild-de Sitter宇宙的Hawking辐射和匀加速系的Rindler辐射。指出在Rindler辐射的问题上等效原理依然成立,Rindler辐射确实来源于该参考系的视界,Hawking辐射与时空的曲率无关,而只与视界附近的动力学效应k有关。

The Hawking radiation of charged Dirac particles on event horizon of Kerr-Newman black holes is studied in this paper. First, we construct the symmetrized null tetrad from which the symmetrized spin coefficients and Dirac equation are derived. Next, we solve the Dirac equation near the event horizon and get the four component ingoing and outgoing wave functions. Finally, by analytic continuation, the Hawking thermal spectrum formula of Dirac particles for arbitrary Kerr-Newman black holes is obtained.

本文研究任意Kerr-Newman黑洞视界曲面上荷电Dirac粒子的Hawking辐射,首先构造了一套“对称零标架”,用这套零标架计算了旋系数,导出了Dirac方程,在视界曲面附近解Dirac方程。得到荷电Dirac粒子四分量波函数的显示表式。利用解析延拓技巧,最后得到荷电Dirac粒子Hawking辐射的热谱公式。

The Hawking radiation of klein-Gordon particles in Kerr-Newman-de Sitter space-time is studied in this paper. First we obtain the Klein-Gordon equation of a charged particle in Kerr-Newman-de Sitter spacetime. Then we solve the K-G equation near the event horizon and get the approximate wave function of ingoing and outgoing scalar particles just outside the event horizon. By analytic continuation we extend the outgoing wave function from outside of the event horizon to the inside of it, and get the complete...

The Hawking radiation of klein-Gordon particles in Kerr-Newman-de Sitter space-time is studied in this paper. First we obtain the Klein-Gordon equation of a charged particle in Kerr-Newman-de Sitter spacetime. Then we solve the K-G equation near the event horizon and get the approximate wave function of ingoing and outgoing scalar particles just outside the event horizon. By analytic continuation we extend the outgoing wave function from outside of the event horizon to the inside of it, and get the complete outgoing wave function. Finally the Hawking thermal spectrum formula is derived.

本文用解析延拓方法讨论Kerr-Newman-de Sitter时空标量粒子的Hawking辐射,所得视界曲面上的重力加速度k和温度T的表式与[1]一样。

 
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