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arXiv 2006.03789astro-ph.HEhep-phnucl-th
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用引力波观测约束强子-夸克相变的起始密度

Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations

Sebastian Blacker, Niels-Uwe F. Bastian, Andreas Bauswein, David B. Blaschke, Tobias Fischer, Micaela Oertel, Theodoros Soultanis, Stefan Typel

摘要:

利用流体动力学模拟方法研究了中子星双星合并过程中可能发生的强子-夸克相变。在前人工作的基础上,我们描述了中子星双星合并的引力波(GW)信号中的退禁闭夸克物质的一个明确的和可测量的特征,包括不同总双星质量的等质量和不等质量系统。在较高密度的PT,即合并后,软化的EoS,导致一个特征性的增加占主导地位的合并后GW频率f_peak相对于潮汐变形λ推断在合并前inspiral阶段。因此,测量这种合并后频率的增加提供了证据的存在一个强大的PT。如果合并后的频率和潮汐变形性与纯重子EoS模型的结果相一致,则f_peak和Lambda之间的关系非常紧密,在一定密度下可以排除强PT。我们发现,在早期合并后残留物的演化过程中,f_peak和Lambda与最大密度密切相关。因此,这些GW观测信息的密度状况,这是探测的残留物和它的GW排放。利用这种关系,我们设计了一个直接适用的,具体的程序来约束的QCD PT从未来的GW测量的起始密度。我们指出了两个有趣的情况:如果没有迹象表明PT从GW检测推断,我们的程序产生的强子夸克PT的起始密度的下限。相反,如果一个合并事件揭示了退禁闭夸克物质发生的证据,推断的GW参数设置的PT发病密度的上限。(节略)

英文摘要:

We study the possible occurrence of the hadron-quark phase transition (PT) during the merging of neutron star binaries by hydrodynamical simulations employing a set of temperature dependent hybrid equations of state (EoSs). Following previous work we describe an unambiguous and measurable signature of deconfined quark matter in the gravitational-wave (GW) signal of neutron star binary mergers including equal-mass and unequal-mass systems of different total binary mass. The softening of the EoS by the PT at higher densities, i.e. after merging, leads to a characteristic increase of the dominant postmerger GW frequency f_peak relative to the tidal deformability Lambda inferred during the premerger inspiral phase. Hence, measuring such an increase of the postmerger frequency provides evidence for the presence of a strong PT. If the postmerger frequency and the tidal deformability are compatible with results from purely baryonic EoS models yielding very tight relations between f_peak and Lambda, a strong PT can be excluded up to a certain density. We find tight correlations of f_peak and Lambda with the maximum density during the early postmerger remnant evolution. These GW observables thus inform about the density regime which is probed by the remnant and its GW emission. Exploiting such relations we devise a directly applicable, concrete procedure to constrain the onset density of the QCD PT from future GW measurements. We point out two interesting scenarios: if no indications for a PT are inferred from a GW detection, our procedure yields a lower limit on the onset density of the hadron quark PT. On the contrary, if a merger event reveals evidence for the occurrence of deconfined quark matter, the inferred GW parameters set an upper limit on the PT onset density. (abridged)

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