广义相对论限制适当时间预言冻结星而不是黑洞
General Relativity Constraints the Proper Times and Predicts the Frozen Stars Instead of the Black Holes
摘要：
在静态的引力场中，世界线与具有常数t的全局超曲面的交点给出了一个不变的约束条件，该约束条件与该事件的真时t有关。由于在任何有限的t，这样的约束真时间间隔小于穿越视界所需的时间间隔，因此广义相对论预言，在处处具有类时测地线或零测地线的恒星中，真时间的引力冻结。时间膨胀通过冻结来稳定收缩的大质量恒星，这是最大的，但在中心是有限的，表面在引力半径附近被冻结。由于辐射和外部相互作用，冻结的恒星（frozars）缓慢地冻结，内部的相变可以引发爆发和爆炸的重新冻结。
英文摘要：
In a static gravitational field an intersection of a worldline by a global hypersurface of simultaneity t=const gives an invariant constraint relating the proper time of this event by t. Since at any finite t the such constrained proper time intervals are less than reqiured for crossing a horizon, general relativity predicts the gravitational freezing of proper times in stars with time-like or null geodesics everywhere. The time dilation stabilizes contracting massive stars by freezing, which is maximal but finite at the centre, and the surface is frozen near the gravitational radius. The frozen stars (frozars) slowly defrost due to emissions and external interactions, the internal phase transitions can initiate refreezing with bursts and explosions.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
