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hawking效应     
相关语句
  hawking effect
     HAWKING EFFECT IS A COMPENSATE EFFECT IN 1+1 DIMENSIONS
     1+1维引力理论中的Hawking效应是补偿效应
短句来源
     UNIVERSAL COORDINATE TRANSFORMATION LEADING TO HAWKING EFFECT
     导致Hawking效应的普遍坐标变换
短句来源
     Hawking Effect of the Dirac Particle in Spherically Symmetric Nonstatic Charged Space Time
     球对称带电时空中Dirac粒子的Hawking效应
短句来源
     HAWKING EFFECT AS A COMPENSATE EFFECT UNDER THE COORDINATE-SCALE TRANSFORMATION
     Hawking效应是坐标尺度变换下的补偿效应
短句来源
     Using Rindler coordinate transformation,we study the crux of Hawking effect and find that Hawking effect is a compensation effect under coordinate size transformation.
     利用Rindler坐标变换,研究Hawking效应的实质.从而证实了Hawking效应是坐标尺度变换下的一种补偿效应.
短句来源
更多       
  hawking effects
     Coordinate Transformation for Hawking Effects of Evaporating Black Holes
     动态黑洞Hawking效应中的坐标变换
短句来源
  compensate effect
     HAWKING EFFECT IS A COMPENSATE EFFECT IN 1+1 DIMENSIONS
     1+1维引力理论中的Hawking效应是补偿效应
短句来源
     HAWKING EFFECT AS A COMPENSATE EFFECT UNDER THE COORDINATE-SCALE TRANSFORMATION
     Hawking效应是坐标尺度变换下的补偿效应
短句来源
     The Hawking effect in 2+1 dimensional can be regarded as a compensate effect under the coordinate-scale transformation. The relevant temperature is a pure-gauge potential of the compensate field.
     2 + 1 维引力中的Hawking 效应可以看作坐标尺度变换下的补偿效应,相应的温度是补偿场的纯规范势.
短句来源
     The Hawking effect in black hole physics can be universally regarded as a compensate effect under the coordinate-scale transformation.
     黑洞物理学中的Hawking效应普遍可以看作坐标尺度变换下的补偿效应。
短句来源
     The Hawking effect in a general spherically symmetric non stationary space time can be considered as a compensate effect of the time scale transformation.
     一般球对称动态时空中的Hawking效应可看作时间尺度变换下的补偿效应 .
短句来源
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  “hawking效应”译为未确定词的双语例句
     Hawsking Effect of Single-Poled Evaporating Black Hole
     具有整体单极的蒸发黑洞的Hawking效应
短句来源
     The discussion about the generating functional for the temperature Green's functions supports that there exists Hawing effect in such a space-time.
     关于温度格林函数生成泛函的讨论,支持了在这类时空中存在Hawking效应的看法.
短句来源
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  hawking effect
The Hawking effect (evaporation) does not operate in such objects due to the absence of a horizon, making it possible for them to be retained over cosmological time intervals, even if their masses are smaller than 1015 g.
      
The Hawking effect of the Vaidya black hole is given easily without calculating the vacuum expectation value of the renormalized energy-momentum tensor.
      
Hawking effect of some axially symmetric non-stationary black holes
      
Hawking effect of a rotating, arbitrarily accelerating black hole
      
Some heuristic semi-classical derivations of the Planck length, the Hawking effect and the Unruh effect
      
更多          
  hawking effects
The Hawking effects of the non-stationary Kerr black hole and the non-uniformly rectilinearly accelerating Kinnersley black hole are researched.
      
Internal relations between the Damour-Ruffini approach and the Unruh approach to dealing with the Hawking effects are shown.
      


A universal coordinate transformation leading to Hawking effect is obtained from only a few conditions whose physical meaning is clear. It is pointed out that the separation of the time variable and the space variable in the coordinate transformation is a sufficient condition for introducing the thermal effect when the new space-time is stationary and time-orthogonal. It is inferred that the "separation" in the coordinate transformation may be regarded as a new representation of the fundamental postulate upon...

A universal coordinate transformation leading to Hawking effect is obtained from only a few conditions whose physical meaning is clear. It is pointed out that the separation of the time variable and the space variable in the coordinate transformation is a sufficient condition for introducing the thermal effect when the new space-time is stationary and time-orthogonal. It is inferred that the "separation" in the coordinate transformation may be regarded as a new representation of the fundamental postulate upon which statistical mechanics is built.

本文从少数几个物理意义明确的条件,得出产生Hawking效应的普遍坐标变换,提出在时空稳态,时轴正交的前提下,一种“分离时空变量形式的坐标变换”是导致热效应的充分条件,推测这种形式的分离变量是统计物理基本假设的一种表达方式。

There exists universally 2-dimensional coordinate extension through an event horizon in a stationary space-time. There is no any coordinate singularity at the event horizon when the new coordinates are adopted. The discussion about the generating functional for the temperature Green's functions supports that there exists Hawing effect in such a space-time.

在稳态时空中,普遍存在穿越事件视界的二维坐标延伸.采用新坐标时,在视界上不存在坐标奇异性.关于温度格林函数生成泛函的讨论,支持了在这类时空中存在Hawking效应的看法.

We try to develop the Weyl gauge theory in a new direction. The Hawking effect in black hole physics can be universally regarded as a compensate effect under the coordinate-scale transformation. The relevant quantum temperature is a pure-gauge potential of the compensate field.

从新的角度尝试发展了Weyl的规范不变理论。黑洞物理学中的Hawking效应普遍可以看作坐标尺度变换下的补偿效应。相应的量子温度是补偿场的纯规范势。

 
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