论文标题
中子恒星内中子衰变的后果
Consequences of neutron decay inside neutron stars
论文作者
论文摘要
中子可能腐烂到暗物质的假说是使用中子星作为测试地的探索。发现为了在观察到的恒星的上端获得质量，暗物质必须经历相对较强的自我互动。然后，巴里昂数量和能量的保护要求恒星必须进行一些加热，半径降低，从而导致几天内旋转速度的提高。
The hypothesis that neutrons might decay into dark matter is explored using neutron stars as a testing ground. It is found that in order to obtain stars with masses at the upper end of those observed, the dark matter must experience a relatively strong self-interaction. Conservation of baryon number and energy then require that the star must undergo some heating, with a decrease in radius, leading to an increase in speed of rotation over a period of days.
