粒子碰撞的英文

• particle collisions
• particle encounter

• "粒子"英文翻译    grain; granule
• "碰撞"英文翻译    collide; run into; knock aga ...
• "重粒子碰撞" 英文翻译 :    heavy particle collision
• "内部粒子碰撞" 英文翻译 :    interparticle collisions
• "内部粒子碰撞；粒子间碰撞" 英文翻译 :    interparticle collisions
• "电子碰撞" 英文翻译 :    ei; electron collision; electron impact
• "分子碰撞" 英文翻译 :    molecular collision; molecular impact
• "光子碰撞" 英文翻译 :    photon collision
• "离子-原子碰撞" 英文翻译 :    ion atom collision
• "离子碰撞" 英文翻译 :    collision of ions; ion impact
• "量子碰撞" 英文翻译 :    quantum collision
• "强子碰撞" 英文翻译 :    hadron collision
• "声子-声子碰撞" 英文翻译 :    phonon-phonon collision
• "双分子碰撞" 英文翻译 :    bimolecular collision
• "原子碰撞" 英文翻译 :    atomic collision
• "中子碰撞" 英文翻译 :    neutron collision
• "大强子碰撞器" 英文翻译 :    lhc
• "电子碰撞电离" 英文翻译 :    electron impact ionization
• "电子碰撞解吸" 英文翻译 :    eid; electron impact desorption
• "电子碰撞频率" 英文翻译 :    electron collision frequency
• "电子碰撞游离" 英文翻译 :    ionization by electron impact
• "离子分子碰撞" 英文翻译 :    ion molecule collision
• "离子离子碰撞" 英文翻译 :    ion ion collision
• "离子碰撞电离" 英文翻译 :    ion impact ionization
• "原子碰撞理论" 英文翻译 :    atomic collision theory

• the amount of light yielded by fluors from the collisions of a β particle is diminishingly small.
  荧光体粒子碰撞，发射出的光量很小，而且继续缩小。
• Therefore , studying particle collisions is like " looking back in time " , recreating the environment present at the origin of our universe
  因此，研究粒子碰撞就象在时间中追忆，重建宇宙早期时的环境。
• Semiconductor devices - mechanical and climatic test methods - part 16 : particle impact noise detection iec 60749 - 16 : 2003 ; german version en 60749 - 16 : 2003
  半导体器件.机械和气候试验方法.第16部分:粒子碰撞噪
• Auroras occur as a result of charged particles mostly electrons from the sun colliding with gas particles in the earth s atmosphere , producing a glow in different colours
  当来自太阳的带电荷粒子主要是电子与地球大气层的空气粒子碰撞，产生不同颜色的光，这便是极光。
• H . moreover , high density is required to increase the chance of collision . hence , the reactions can only take place in the core of the sun , with temperature over ten million degrees 10
  首先核聚变需要极高的温度，让氢原子核能有足够的能量克服原子核之间的电排斥力，此外亦需要极高的密度去增加粒子碰撞的机会，所以核聚变只能在温度高达10
• If one end of a metal rod is at a higher temperature , then energy will be transferred down the rod toward the colder end because the higher speed particles will collide with the slower ones with a net transfer of energy to the slower ones
  如果另一端的一个金属棒，是在更高的温度，然后能源的，将移交下来棒对寒冷的结束，因为这种高速粒子碰撞与慢的，以净转移的精力用在较慢。
• The other two , phenix and star , are built around huge , general - purpose devices that fill their three - story experimental halls with thousands of tons of magnets , detectors , absorbers and shielding [ see bottom box on preceding page ]
  另两个实验， phenix与star ，则是巨大且用途广泛的仪器，几千公吨的磁铁、侦测器、吸收器以及保护罩，塞满了三层楼的实验大楼（参见33页粒子碰撞与侦测） 。
• By analogizing the concept of particle collides in high - energy physics , we proposed the particle model of logic function , and constructed the particle collide arithmetic of logic function predigest according to this model , finally using vc + + 6 . 0 programming realized it
  摘要类比高能物理中粒子碰撞的概念，提出了逻辑函数的粒子模型，根据此模型构造了化简逻辑函数的粒子碰撞算法，并用vc + + 6 . 0编程实现。
• They are associated with geomagnetic activity brought about by solar wind . auroras occur as a result of charged particles ( mostly electrons ) from the sun colliding with gas particles in the earth s atmosphere , producing a glow in different colours
  极光通常在高纬度的地区出现，它们与太阳风引致的地磁活动有关。当来自太阳的带电荷粒子（主要是电子）与地球大气层的空气粒子碰撞，产生不同颜色的光，这便是极光。
• In modern laboratories like cern or fermilab in illinois , physicists accelerate antiprotons or positrons produced by nuclear reactions to the speed of light and collide them with conventional particles to produce tiny starbursts of primordial energy , recreating forms of matter and energy unseen since the big bang
  像cern现代实验室或伊利诺斯州费米实验室，物理学家加速核反应产生的反质子或正电子到光速，而且把它们同常态粒子碰撞产生自大爆炸以后从未见过的物质和能量再生形态的原始能量极小星光闪耀。