因其色禁闭及小体积特点，低质量裸奇异星可以非常快地自转且几乎不受引力辐射不稳定性的约束。
Besides small thermal radii, low-mass quark stars could spin very fast, with a negligible effect of r-mode instability.
用理论和数值的方法，首次研究了扭摆器中相干同步辐射效应诱发的微束团不稳定性。
We studied the microbunch instability in wigglers induced by coherent synchrotron radiation (CSR) theoretically and numerically for the first time.
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