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The Allowed Parameter Space of a Long-lived Neutron Star as the Merger Remnant of GW170817
Ai, Shunke; Gao, He; Dai, Zi-Gao; Wu, Xue-Feng; Li, Ang; Zhang, Bing; Li, Mu-Zi
刊名ASTROPHYSICAL JOURNAL
2018
卷号860期号:1页码:57
英文摘要Due to the limited sensitivity of the current gravitational wave (GW) detectors, the central remnant of the binary neutron star (NS) merger associated with GW170817 remains an open question. In view of the relatively large total mass, it is generally proposed that the merger of GW170817 would lead to a short-lived hypermassive NS or directly produce a black hole (BH). There is no clear evidence to support or rule out a long-lived NS as the merger remnant. Here, we utilize the GW and electromagnetic (EM) signals to comprehensively investigate the parameter space that allows a long-lived NS to survive as the merger remnant of GW170817. We find that for some stiff equations of state, the merger of GW170817 could, in principle, lead to a massive NS, which has a millisecond spin period. The post-merger GW signal could hardly constrain the ellipticity of the NS. If the ellipticity reaches 10(-3), in order to be compatible with the multi-band EM observations, the dipole magnetic field of the NS (B-p) is constrained to the magnetar level of similar to 10(14) G. If the ellipticity is smaller than 10(-4), B-p is constrained to the level of similar to 10(9)-10(11) G. These conclusions weakly depend on the adoption of the NS equation of state.
语种英语
WOS记录号WOS:000435102000007
内容类型期刊论文
源URL[http://libir.pmo.ac.cn/handle/332002/18024]  
专题中国科学院紫金山天文台
推荐引用方式
GB/T 7714
Ai, Shunke,Gao, He,Dai, Zi-Gao,et al. The Allowed Parameter Space of a Long-lived Neutron Star as the Merger Remnant of GW170817[J]. ASTROPHYSICAL JOURNAL,2018,860(1):57.
APA Ai, Shunke.,Gao, He.,Dai, Zi-Gao.,Wu, Xue-Feng.,Li, Ang.,...&Li, Mu-Zi.(2018).The Allowed Parameter Space of a Long-lived Neutron Star as the Merger Remnant of GW170817.ASTROPHYSICAL JOURNAL,860(1),57.
MLA Ai, Shunke,et al."The Allowed Parameter Space of a Long-lived Neutron Star as the Merger Remnant of GW170817".ASTROPHYSICAL JOURNAL 860.1(2018):57.
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