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liang lei zhong zi xing zhi jian de zhuan bian
Author(s): 
Pages: 167-169
Year: Issue:  4
Journal: Chinese Science Bulletin

Keyword:  中子星超新星爆发星体能量差相变中子态物态量级文献质量;
Abstract: <正> 在文献[1]中我们已经证明,可能存在两类中子星,由正常中于物态构成的正常中子星以及由反常中子物态构成的反常中子星。当星体质量M<0.8M时,正常中子星是稳定的,反之,当M>0.8M时,反常中子星稳定。还指出,在M>0.8M及M<0.8M两区域,分别还有亚稳的正常中子星及反常中子星,并估计,稳定星与亚稳星之间的能量差约为10-2M,所以,当整个星体发生相变时能放出1052尔格的能量,这恰恰是超新星爆发的能量量级。因
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