这个想法在费米悖论中有所体现。
费米的天才闻名于整个科学界。
正是这些粒子进入了费米的轨道。
这些发物质束便被费米的仪器所捕获了。
Those antimatter beams are then picked up by Fermi's instruments.
他相信这个过程产生出了费米镜观测到的伽马射线流。
He believes that this process supplies the gamma-rays observed by Fermi.
不过随着时间的推移，费米望远镜会不断发现更多的爆发点。
But over the next few years, Fermi will detect more and more bursts.
费米尔泡可能是由我们银河系中心的黑洞所驱动的。
The Fermi bubbles could be powered by the black hole at the center of our galaxy.
在这个温度下，气体处于一种奇异的形态：它成为了费米气体。
At these temperatures, the gas takes on a very exotic form; it becomes a Fermi gas.
这是回答费米悖论所提问的，为什么星系中没有充满了智能生命。
This speaks to the Fermi Paradox, which asks why the galaxy isn't crawling with intelligent life.
但地表伽马射线如何能到达太空中安放费米镜的卫星呢？
But how can terrestrial gamma rays reach Fermi's orbit in space?
鉴于费米尔望远镜发现了它们，研究人员称其为费米尔泡。
Researchers called them Fermi bubbles, after the Fermi space telescope that spotted them.
虽然费米镜看不到雷暴，然而这个航天器还是通过地磁场与之联系在一起。
"Even though Fermi couldn't see the storm, the spacecraft nevertheless was magnetically connected to it," Florida Institute of Technology's Joseph Dwyer said in NASA's press release. "the."
该同步加速器在费米实验室建造，首例病人于1990年接受治疗。
The synchrotron accelerator was built at Fermilab and the first patients were treated in 1990.
凭借他们空前的能量，大型强子对撞机（LHC)在费米实验室很热门。
And with its unprecedented energies, the Large Hadron Collider is hot on Fermilab's heels.
1995年费米实验室那项发现的消息几个月内零星地泄露（透露）出一点点。
News of that discovery, at Fermilab, trickled out in dribs and drabs over several months in 1995.
因此，恩里科·费米把它们叫做‘小中子’，在意大利语中就是中微子的意思。
So Enrico Fermi called them "a little neutron," in Italian is neutrino.
2008年9月16日，费米望远镜发现了迄今为止最为强烈的伽马射线爆发。
On September 16, 2008, Fermi picked up the most powerful GRB observed to date.
在银河盘面两端，发现了两个长达30,000光年的东东，它们被称作费米尔泡。
Two 30,000 light-year-long blobs called Fermi bubbles have been discovered on either side of our galactic plane. John Matson reports
功率位居第二位的是伊利诺伊州费米实验室的粒子加速器，其运行能量为1TeV)。
The second most powerful particle accelerator, at Fermilab in Illinois, runs at 1 TEV.
早上，我们从费米伽马射线图中的众多活跃星系中观察到，其中一个星系的伽马射线变得极度明亮。
This morning we noticed that one of the many active galaxies in the Fermi sky had become extremely bright in gamma-rays.
远处的暴风雨在费米的视线之下，所以暴风雨所产生的任何伽马射线，都不可能会被检测到。
The distant storm was below Fermi's horizon, so any gamma rays it produced could not have been detected.
自1954年费米去世后，还没有哪一位物理学家同时是一名精通的实验主义者和一名最主要的理论家。
Since Fermi's death in 1954, no physicist has been at once a master experimentalist and a leading theoretician.
正电子和电子会相互湮灭而发射出的伽玛射线，再由费米的爆发检测器所检测到，研究人员说。
Positrons and electrons annihilated each other, emitting gamma rays detected by Fermi's gamma-ray burst detector, researchers said.
事实上，9月16日观测到的爆发是迄今为止最为强烈的，所以费米望远镜很容易就发现了它。
In fact, the September 16th burst is the most powerful observed to date, and was easily detected by Fermi.
这些“费米大天区望远镜（LAT）”所侦测到的高能伽马射线的波长仅相当于原子核大小的千分之一。
These high-energy gamma rays, detected by Fermi’s Large Area Telescope (LAT), have wavelengths one-thousandth the size of an atomic nucleus.
许多星系都呈现出双泡状物质喷流并且伴有核心区域喷发出的能量，不过“费米气泡”已然超越了这种简单的解释。
Lots of galaxies exhibit two-lobed jets of matter and energy erupting from their cores, but the "Fermi bubbles" defy easy explanation.
费米气体由量子动力学描述，它被激光阱控制在某处，这使得科学家们能够模拟中子星内致密中子的状态。
The Fermi gas is governed by quantum dynamics and held in place by the laser trap, allowing the group to simulate the conditions of the tightly packed neutrons inside a neutron star.
按照美国航空航天局的示意图上所描绘的，费米伽马射线望远镜所观测到的双“气泡”在X射线和射电波长均有显现。
AS depicted in this NASA illustration, the twin "bubbles" seen in Fermi's gamma-ray observations also manifest themselves at X-ray and radio wavelengths.
把费米直接去监察一次雷暴雨，以便能观察到大多数的伽玛射线闪光，但在有些情况下，风暴已远远地离去。
Fermi was located immediately above a thunderstorm for most of the observed gamma-ray flashes, but in several cases, storms were far away.
把费米直接去监察一次雷暴雨，以便能观察到大多数的伽玛射线闪光，但在有些情况下，风暴已远远地离去。
Fermi was located immediately above a thunderstorm for most of the observed gamma-ray flashes, but in several cases, storms were far away.
应用推荐