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- The output takes the form of Hawking radiation. 黑洞电脑输出的是霍金辐射。
- Semi-classical approximations are workable, and have led to predictions such as Hawking radiation. 半经典的近似值是可用的，而已带来预计的霍金斯辐射。
- We might be able to detect the Hawking radiation of a mini black hole, provided we can find one. 普通星体所形成的黑洞的温度低至根本无法量度,但只要我们能够找到小型黑洞,其蒸发过程却是可以观测得到的。
- Hawking radiation: Radiation theoretically emitted from just outside the event horizon of a black hole. 霍金辐射:理论上，从一个黑洞的视界外放出的辐射。
- Other scientists eventually conceded that he was correct,the black-hole emissions are now known as Hawking radiation. 其他科学家最终还是承认他是正确的，而且现在人们还把黑洞射线称为霍金射线。
- The real question is whether Hawking radiation returns the answer of the computation or merely gibberish. 真正的问题在于霍金辐射是否提出了运算的答案，或只是一番胡言乱语。
- He suggested that this analogy might be useful in assessing the impact of microscopic physics on the origin of Hawking radiation. 他提出，在评估微观物理对霍金辐射起源上的影响时，这种类比也许会很有用。
- The annihilation of the infalling photon acts as a measurement, transferring the information contained in the matter to the outgoing Hawking radiation. 向内坠落的光子，其毁灭的过程就是个测量的动作，会将黑洞内物质的资讯转移给向外发出的霍金辐射。
- "The optical device reported in this paper has no internal source of energy and therefore cannot emit Hawking radiation," Pendry says. 纳瑞马诺维说：“如果这种人造黑洞试验成功，以后我们就不再需要用反射镜收集太阳光了。”
- Pairs of entangled photons materialize at the event horizon.One of the photons flies outward to become the Hawking radiation that an observer sees. 一对缠结的光子在事件视界形成后，其中一个光子向外飞出，成为观测者所看见的霍金辐射。
- A one-kilogram hole gives off Hawking radiation and, to conserve energy, decreases in mass, disappearing altogether in a mere 10-21 second. 因为能量守恒的缘故，其质量必定会减少，一公斤的黑洞在发出霍金辐射后，短短的10-21秒内就会消失殆尽。
- Other scientist eventually conceded that he was correct, and the black-hole emissions are now known as Hawking radiation. 其他科学家最后承认他是对的，现在黑洞辐射线就被叫做霍金射。
- Under a new Tortoise coordinate transformation, by reducing and solving the Klein-Gordon equation near the event horizon, the Hawking radiation is studied. 采用一种新的Tortoise坐标变换 ;通过约化和求解视界附近的Klein Gordon方程 ;得到了黑洞的Hawking热谱和Hawking温度 .
- He proposed that quantum perturbations of the event horizon could allow information to escape from a black hole, where it can influence subsequent Hawking radiation [5]. 他提出活动视界的量子混乱就会允许信息自可以影响后来的霍金辐射[5]的黑洞里逃逸出来。
- The Hawking radiation for a charged axially symmetric nonstationary black hole is studied. We obtain the event horizon equation and the Hawking thermal spectrum formula. 讨论了轴对称荷电动态黑洞的Hawking辐射 ;得到了局部事件视界面方程和温度 .
- Hawking radiation originates just outside the event horizon and, so far as it is understood, does not carry information from its interior since it is thermal. 霍金辐射由外在活动视界引发，因而就是这样理解的，由于它是热的不带有内部信息。
- However, in 1974, Hawking applied quantum field theory to the curved spacetime around the event horizon and discovered that black holes can emit thermal radiation, known as Hawking radiation. 然而,在1974年,霍金将量子场理论运用到活动视界周围的弯曲时空上而发现黑洞能发出热辐射，就是熟知的霍金辐射。
- The Hawking radiation and the Starobinsky - Unruh process of Dirac particles in space-time determined by the generalized spherical symmetric evaporating charged (GSSEC) black hole are studied. 研究了广义球对称带电蒸发黑洞周围的时空中Dirac粒子的Hawking辐射以及Starobin-sky-Unruh过程.
- 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. 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。
- Hawking radiation is viewed as a tunneling process across the event horizon and the tunneling probability is calculated. According to the tunneling probability,a leading correction to the semi-classical emission rate is found. 通过将Hawking辐射看成是穿过事件视界的隧道效应;计算出隧道穿透率并且得到了一个相对于半经典穿透率的修正.
