结果显示，非重子暗物质背景的存在将对引力系统的不稳定性产生重要影响。
The results show that the existence of non-baryonic dark matter background influences seriousely the instability of a gravitational system.
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.
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.
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