大质量脉冲星核心内假真空态的证据及其真实质量测量的影响

Ahmad A. Hujeirat, Mauritz M. Wicker
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引用次数: 1

摘要

基于脉动脉冲星的理论和观测,我们证明了大质量脉冲星核心内部的超冷超核致密物质应该在真空中凝聚,正如非微扰QCD所预测的那样。被困在这里的物质形成了嵌入平坦时空的假真空,与外部世界完全隔绝。尽管真空期望值在这里消失了,但这些不可压缩的超流体核心的质量和大小是随着宇宙时间而增长的,这与昂塞格-费曼超流动性分析一致。我们将这一情景应用于几颗被充分研究过的脉冲星,即蟹状星、船帆星、PSR J0740+6620,发现它们核心中被捕获的质量含量为{0.15,0.55,0.64},这意味着它们的真实质量分别为{1.55,2.35,2.72}。基于此,我们得出结论:1)大质量脉冲星和中子星的真实质量远高于直接观测到的质量,因此从上面看是无界的;2)GW170817合并事件的残余应该是一个拥有1.66核心的大质量NS。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Evidence for False Vacuum States inside the Cores of Massive Pulsars and the Ramification on the Measurements of Their True Masses
Based on the theory and observations of glitching pulsars, we show that the ultra-cold supranuclear dense matter inside the cores of massive pulsars should condensate in vacua, as predicated by non-perturbative QCD. The trapped matter here forms false vacuums embedded in flat spacetimes and completely disconnected from the outside world. Although the vacuum expectation value here vanishes, the masses and sizes of these incompressible superfluid cores are set to grow with cosmic times, in accord with the Onsager-Feynman superfluidity analysis. We apply our scenario to several well-studied pulsars, namely the Crab, Vela, PSR J0740+6620 and find that the trapped mass-contents in their cores read {0.15,0.55,0.64}, implying that their true masses are {1.55,2.35,2.72} , respectively. Based thereon, we conclude that: 1) The true masses of massive pulsars and neutron stars are much higher than detected by direct observations and, therefore, are unbounded from above, 2) The remnant of the merger event in GW170817 should be a massive NS harbouring a core with 1.66 .
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