In the first chapters, the concepts of black hole and the event horizon, black hole radiation, the thermal properties of black hole, and scalar field radiation are introduced briefly.
在论文的第一章，简单地介绍了黑洞的形成、视界的概念、黑洞的热性质以及黑洞辐射和标量场辐射等基础知识。
That's understandable, because the idea behind string balls is that they start with a black hole that evaporates away due to Hawking radiation.
那是可以理解的，因为弦背后的理论是是它们像黑洞一样以霍金辐射的形式蒸发。
Floyd says the paper one shortcoming of the paper is that it assumes radiation has no impact on orbits inside the black hole.
弗洛伊德认为这篇论文的不足之处之一是它假设辐射对黑洞内的轨道没有影响。
This poses a puzzle, because Hawking radiation does not convey any information about the interior of a black hole.
这带来了一道难题，由于霍金射线并不传递有关黑洞内部的任何信息。
Active galaxies give off bright radiation from their cores, where gas heats up as it is compressed into a swirling accretion disk encircling the black hole.
活动星系从它们的核部发出明亮的光芒，在那里，气体被加热并压缩成一个漩涡状的圆盘，漩涡的中心便是黑洞。
Astrophysicists have found that when a supermassive black hole quickly devours gas and dust, it can generate enough radiation to abort all the embryonic stars in the surrounding galaxy.
天体物理学家发现，当一个巨大的黑洞快速吞噬宇宙中的气体和尘埃时产生的辐射，足够摧毁周围星系中初期形成的星体。
The blue color here represents radiation pouring out from material very close to the black hole.
图中的蓝色部分表示从密度极高的黑洞中喷涌而出的辐射能。
Other scientists eventually conceded that he was correct, and 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 radio waves (and lots of other radiation) are the result of matter being drawn into the black hole and releasing energy as it falls.
物质被吸入黑洞的过程，以及其下落时释放能量的过程，都会产生无线电波(还有大量其他射线)。
Though this radiation is too weak to be detected by telescopes, it would be detectable if the LHC did make a tiny black hole.
尽管望远镜还不能发现这种微弱的放射线，不过若lhc真能创造出微小黑洞，就能发现它。
These quasar jets are formed when electrons emitted from a black hole impact with cosmic background radiation left by the big bang, giving astronomers clues about the conditions in the early universe.
这些类星体的河外星系是由当黑洞所发射的电子与大爆炸所遗留下来的宇宙背景辐射碰撞后所形成的，它为天文学家提供了关于早期宇宙的线索。
By emitting this so-called Hawking radiation, a black hole would gradually lose energy and mass.
通过发出所谓的霍金辐射，黑洞会逐渐失去能量和质量。
We'd be able to connect a lot of the physics happening within the gaseous environment and accretion disk to the binary black hole merger to the gravitational radiation.
我们可以将很多发生在黑洞对合并时的气体环境和吸积盘里的物理过程与引力辐射联系起来。
Might it be possible to induce a black hole to release all its Hawking radiation sooner, so that in effect it becomes like a ball of fuel?
是否可以诱使一个黑洞加快辐射速度，从而变成一个事实上的燃料之球呢？
The flow of particles of negative energy into the black hole reduces its mass until it disappears completely in a final burst of radiation.
负能量的粒子流进入这个黑洞后，会减轻它的质量，直到黑洞发生最后的辐射大爆炸后才完全消失。
This core is the main part of the black hole where the mass is concentrated and appears purely black on all readings even. through the use of radiation detection devices.
内核是黑洞的主要部分，在这里物质被压缩，即使使用辐射探测仪，从所有的读数来看这里似乎都是漆黑一片。
Other scientists eventually conceded that he was correct, and the black-hole emissions are now known as Hawking radiation.
其他肸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。
As a black hole or neutron star destroys a star, tremendous amounts of radiation are released.
当黑洞或中子星将一颗恒星毁灭时将会产生巨大的辐射。
It leads to a new understanding of thermal radiation of the black hole.
使人们对黑洞热辐射的研究有了进一步的认识。
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。
Some major puzzles in black hole theory and General Relativity, including Hawking radiation, information puzzle, singularity theorem and synchronization of clock rate, are presented.
介绍了黑洞理论和广义相对论中的几个重要疑难，涉及霍金辐射、信息佯谬、奇性定理和钟速同步，并给出了可能的解答。
The intense radiation was part of a gamma-ray burst that lasted a minute and which marked the death of a massive star transmogrifying itself into a black hole.
这种强辐射是爆发持续了一分钟之久的伽马射线的一部分，这标志着一颗超大质量恒星的死亡同时将自己转变成一个黑洞。
This paper proves from the tangle of theory of relativity and quantum mechanics, that there does exist thermal radiation and nonthermal radiation in the black hole.
本文主要从相对论与量子力学的角度证明了黑洞的热辐射与非热辐射的存在。
By using the radiant emittance of Schwarzchild, the radiation spectrum of black hole are calcutated out. and both of them have a little difference.
利用史瓦西黑洞的辐出度，导出了黑洞费米子场和玻色子场的辐射谱及其对应的维恩位移定律， 并且得出二者的辐射谱及定律略有不同。
These particles, along with radiation, flow rapidly away from the black hole along the magnetic field lines.
这些粒子，伴随着发出射线，沿着磁力线朝着黑洞相反的方向快速流动。
Using radiant exitance of Schwarzschild black hole, the radiation spectrums of Fermion field and Boson field of black hole are calculated out, and Wien's displacement laws are also obtained.
利用史瓦西黑洞的辐出度，导出了黑洞费米子场和玻色子场的辐射谱及其对应的维恩位移定律，并且得出二者的辐射谱及定律略有不同。
We drew the conclusion that the frequency distribution of the non-thermal radiation from a general spherically-symmetric and charged evaporating black hole depended on the time.
研究一般球对称带电蒸发黑洞视界附近粒子的能级交错，给出交错能级最大值的表达式，得出一般球对称带电蒸发黑洞非热辐射频率范围是随时间变化的结论。
We drew the conclusion that the frequency distribution of the non-thermal radiation from a general spherically-symmetric and charged evaporating black hole depended on the time.
研究一般球对称带电蒸发黑洞视界附近粒子的能级交错，给出交错能级最大值的表达式，得出一般球对称带电蒸发黑洞非热辐射频率范围是随时间变化的结论。
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