其他CGC在菌体某一部位弯曲形成“S”形中心的自旋体。
Some CGCs tended to bend at certain part to form a S-shaped center.
但是,由于星系中没有足够的质量,因此产生不了可观察得到的自旋体。
But there is not enough mass in the galaxies to produce the observed spin.
这些绝缘体是具有强自旋轨道相互作用的能带绝缘体, 并显示出量子自旋霍尔效应.
These topological insulators are band insulators with large spin-orbit interactions and exhibit the quantum spin-Hall (QSH) effect.
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