AI 中文总结
本研究聚焦SS-SP系统的连续GW特征，对比DECIGO与BBO的灵敏度曲线，发现二者可在宽参数空间探测该系统的连续GW，相关信号可用于检验SQM假说并深化对超新星等过程的认知。
AI 中文摘要
奇异夸克物质（SQM）假说认为，由SQM构成的天体可存在于从奇异行星（SPs）到奇异星（SSs）的宽质量范围内。已有研究提出，奇异星-奇异行星（SS-SP）并合系统辐射的引力波（GWs）或可被先进LIGO、爱因斯坦望远镜等地基GW观测站探测到。然而，这类系统在进入并合阶段前，可能会在密近构型下经历一段长时间的轨道演化，此阶段会产生毫赫兹（mHz）至分赫兹（dHz）频段的连续GW信号，其详细特征尚未得到充分探究。本研究深入分析SS-SP系统的连续GW特征，重点探究物理上可行的参数空间，将该系统辐射的GW信号与下一代天基GW探测器——分赫兹干涉仪引力波天文台（DECIGO）、大爆炸探测器（BBO）的灵敏度曲线进行对比。分析表明，DECIGO和BBO均可在宽参数空间内探测到SS-SP系统的连续GW，这些GW携带的重要信息可用于检验SQM假说，推动人类对超新星及致密星并合过程的理解。
英文摘要
The Strange Quark Matter (SQM) hypothesis posits that objects composed of SQM could exist across a wide mass range, from strange planets (SPs) to strange stars (SSs). It has been proposed that gravitational waves (GWs) emitted by inspiraling SS-SP systems may be detectable by ground-based GW observatories such as advanced LIGO and the Einstein Telescope. Nevertheless, such a system may undergo an extended period of orbital evolution in a close configuration before entering the inspiraling phase. During this time, it can generate continuous GW signals at frequencies ranging from milli-hertz (mHz) to deci-hertz (dHz). The detailed characteristics of these GWs have not yet been thoroughly explored. In this study, we delve into the continuous GW features of SS-SP systems, with a focus on exploring the physically viable parameter space. We compared the GW signals emitted by these systems to the sensitivity curves of next-generation space-based GW detectors like the Deci-hertz Interferometer Gravitational wave Observatory (DECIGO) and the Big Bang Observer (BBO). Our analyses demonstrate that both the DECIGO and BBO detectors are capable of detecting continuous GWs from SS-SP systems across a broad parameter space. These GWs carry important information for testing the SQM hypothesis, as well as for advancing our understanding of supernovae and compact star merger processes.
Comments12 pages, 5 figures, 2 tables. Comments are welcome
