计算中考虑了弹性散射、非弹性散射、带电粒子发射和辐射俘获。
In computation, the elastic scattering, inelastic scattering, charged particle emission and radiation capture are under consideration.
因此可以把前角区轻带电粒子发射产额作为探测丰质子核结构的一种手段，也是一种新的验证一个核是否具有质子晕结构的实验证据。
It can be regarded as a possible probe to explore the structure of proton rich nuclei and a new way to provide an evidence for existing proton halo.
光线的发射处越远，年龄越大，类星体的光谱会缺失，因为某些波长的光线会被中性氦及氦离子或带电粒子吸收。
Light emitted from farther away, and thus older, quasars lacked this wavelength, because the light was getting absorbed by neutral helium as well as helium with a single ion-or charged particle.
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