摘要
本文证明了对于中心区产生的相变的致密星,相变将使恒星结构方程(Oppenheimer-Volkoff方程)产生修正,并使度规产生新的奇异性。以上结果表明,必须在相变面附近建立边界层。
In this paper, the effect of the phase transition in a compact star is discussed, with the results showing that the Oppenheimef -Volkoff equation will be revised by the phase transition in the neighbourhood of its surface and the new singularity of the gauge will be produced. Therefore, the boundary layer should be established in the neighourhood of the phase transition sufacc.
出处
《天文研究与技术》
CSCD
1989年第1期39-44,共6页
Astronomical Research & Technology
