Constraining quark-hadron interface tension in the multimessenger era

被引:32
作者
Xia, Cheng-Jun [1 ]
Maruyama, Toshiki [2 ]
Yasutake, Nobutoshi [2 ,3 ]
Tatsumi, Toshitaka [4 ]
机构
[1] Zhejiang Univ, Sch Informat Sci & Engn, Ningbo Inst Technol, Ningbo 315100, Zhejiang, Peoples R China
[2] Japan Atom Energy Res Inst, Adv Sci Res Ctr, Shirakata 2-4, Tokai, Ibaraki 3191195, Japan
[3] Chiba Inst Technol, Dept Phys, 2-1-1 Shibazono, Narashino, Chiba 2750023, Japan
[4] Osaka Sangyo Univ, Inst Educ, 3-1-1 Nakagaito, Daito, Osaka 5748530, Japan
基金
中国国家自然科学基金;
关键词
1ST-ORDER PHASE-TRANSITIONS; NEUTRON-STAR MATTER; EQUATION-OF-STATE; SURFACE-TENSION; X-RAYS; DECONFINEMENT; MASSES; DROPLETS; MODEL;
D O I
10.1103/PhysRevD.99.103017
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the interface effects of a quark-hadron mixed phase in compact stars. The properties of nuclear matter are obtained based on the relativistic-mean-field model. For the quark phase, we adopt a perturbation model with running quark masses and coupling constant. At certain choices of parameter sets, it is found that varying the quark-hadron interface tension will have sizable effects on the radii (Delta R approximate to 600 m) and tidal deformabilities (Delta Lambda/Lambda approximate to 50%) of 1.36 solar mass hybrid stars. These provide possibilities for us to constrain the quark-hadron interface tension with future gravitational wave observations as well as the ongoing NICER mission.
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页数:14
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