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

被引:69
作者
Blacker, Sebastian [1 ,2 ]
Bastian, Niels-Uwe F. [3 ]
Bauswein, Andreas [1 ,4 ]
Blaschke, David B. [3 ,5 ,6 ]
Fischer, Tobias [3 ]
Oertel, Micaela [7 ]
Soultanis, Theodoros [8 ,9 ]
Typel, Stefan [1 ,2 ]
机构
[1] GSI Helmholtzzentrum Schwerionenforsch, Planckstr 1, D-64291 Darmstadt, Germany
[2] Tech Univ Darmstadt, Inst Kernphys, Fachbereich Phys, Schlossgartenstrae 9, D-64289 Darmstadt, Germany
[3] Univ Wroclaw, Inst Theoret Phys, PL-50205 Wroclaw, Poland
[4] Helmholtz Res Acad Hesse Fair HFHF, GSI Helmholtz Ctr Heavy Ion Res, Campus Darmstadt, D-64289 Darmstadt, Germany
[5] Natl Res Nucl Univ MEPhI, Moscow 115409, Russia
[6] Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Russia
[7] Univ Paris, Observ Paris, Sorbonne Paris Cit, LUTH,PSL Res Univ,CNRS, 5 Pl Jules Janssen, F-92195 Meudon, France
[8] Heidelberg Inst Theoret Studies, Schloss Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany
[9] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
基金
俄罗斯科学基金会; 欧洲研究理事会;
关键词
EQUATION-OF-STATE; NEUTRON-STARS; MODEL; MATTER; TEMPERATURE; ENERGY; QCD;
D O I
10.1103/PhysRevD.102.123023
中图分类号
P1 [天文学];
学科分类号
0704 ;
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 A 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 A, a strong PT can be excluded up to a certain density. We find tight correlations of f(peak) and A 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. Both scenarios would thus have strong implications for high-density matter physics, e.g., determining the range of validity of nuclear physics and constraining the properties for quark deconfinement. These prospects demonstrate the importance of simultaneously measuring pre- and postmerger GW signals to exploit the complementarity of the information encoded in both phases. Hence, our work stresses the value added by dedicated high-frequency GW instruments.
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页数:34
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