2025-12-31
理論上，真正滿足條件的雙生中子星本來就極為罕見； 即便它們存在，其半徑差異也小到超出目前觀測儀器的解析能力。

In theory, neutron star twins that truly satisfy the required conditions are extremely rare;
even if they do exist, the difference in their radii is so small that it lies beyond the resolving power of current observational instruments.

雙生星在理論上並未被排除；然而自然界將它們隱藏在極其微小的差異之中，小到超出我們現有、甚至可預見未來觀測系統性誤差所能可靠分辨的範圍。

Twin stars are not ruled out by theory—but nature hides them behind differences smaller than our current, and even near-future, observational systematics can reliably resolve.