hawking radiation 中文意思是什麼
hawking radiation
解釋
黑洞輻射-
The hawking radiation of colored black hole as quantum tunneling
通過量子隧穿研究帶色荷黑洞的霍金輻射 -
The output takes the form of hawking radiation
黑洞電腦輸出的是霍金輻射。 -
The real question is whether hawking radiation returns the answer of the computation or merely gibberish
真正的問題在於霍金輻射是否提出了運算的答案，或只是一番胡言亂語。 -
Unless the hole swallows matter or energy to make up the loss, the hawking radiation will drain it of all its mass
除非黑洞吞噬新物質或新能量來彌補損失，要不然霍金輻射會把它所有的質量?漏個精光。 -
We might be able to detect the hawking radiation of a mini black hole, provided we can find one
普通星體所形成的黑洞的溫度低至根本無法量度，但只要我們能夠找到小型黑洞，其蒸發過程卻是可以觀測得到的。 -
He suggested that this analogy might be useful in assessing the impact of microscopic physics on the origin of hawking radiation
他提出，在評估微觀物理對霍金輻射起源上的影響時，這種類比也許會很有用。 -
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
霍金輻射由外在活動視界引發，因而就是這樣理解的，由於它是熱的不帶有內部信息。 -
A one - kilogram hole gives off hawking radiation and, to conserve energy, decreases in mass, disappearing altogether in a mere 10 - 21 second
因為能量守恆的緣故，其質量必定會減少，一公斤的黑洞在發出霍金輻射后，短短的10 - 21秒內就會消失殆盡。 -
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 ]
他提出活動視界的量子混亂就會允許信息自可以影響后來的霍金輻射[ 5 ]的黑洞里逃逸出來。 -
Well, stephen hawking gave us a surprise answer. he discovered that theoretically, black holes will radiate with a black body spectrum. this is called the hawking radiation
著名英國天文學家霍金得出了一個驚人的結論，他發現理論上黑洞亦會如普通黑體一樣發出輻射，這便是霍金蒸發理論。 -
Hawking discovered a quantum chink in this armor in 1974, when he deduced that black holes should in fact emit a random trickle of particles and radiation ( now called hawking radiation )
1974年，霍金發現了可以從黑洞的魔掌中逃逸出來的量子縫隙，他推導出，黑洞實際上應該會發射出稀疏散亂的粒子和輻射（現在稱為霍金輻射） 。 -
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，霍金將量子場理論運用到活動視界周圍的彎曲時空上而發現黑洞能發出熱輻射，就是熟知的霍金輻射。 -
Because of this effect, dubbed hawking radiation, a black hole slowly evaporates, so that anything that enters is eventually released over billions or even trillions of years
由於被命名為「霍金輻射」 （黑洞輻射）的這個效應，一個黑洞會慢慢蒸發，而進入其中的全部事物最終會在十億以至萬億多年後被釋放。 -
Might the properties, even the existence, of hawking radiation depend on the microscopic properties of spacetime ? much as, for example, the heat capacity or speed of sound of a substance depends on its microscopic structure and dynamics
就像物質的熱容量和聲速，會和它的微觀結構與動力學有關一樣，霍金輻射的性質、甚至是否存在，會不會和時空的微觀性質有關？
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