Detector-Weighted Signatures of Localized Dissipative Transitions in Kerr EMRIs

IF 3.9 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Jingxu Wu,Liangyu Luo,Jiyun Yang,Haoxiang Ma,Jie Shi
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Abstract

Abstract We study a parameterized localized modification of the dissipative evolution in a circular equatorial Kerr extreme mass-ratio inspiral (EMRI). We do not claim a unique mapping to a specific hadron--quark equation of state; instead, the transition sector is treated as a localized flux deformation with parameters $\{A_{\rm tr},f_c,\Delta f,p,q\}$. The reference inspiral uses real Teukolsky flux data from the Black Hole Perturbation Toolkit \texttt{CircularOrbitSelfForceData} repository, interpolating the tabulated Kerr circular-orbit fluxes in radius and spin. For a representative system with $M=2\times10^{5}M_\odot$, $\mu=1.4M_\odot$, $\hat a=0.90$, $A_{\rm tr}=10^{-6}$, $f_c=0.0165~{\rm Hz}$, and $\Delta f=0.009~{\rm Hz}$, we normalize the baseline waveform to $\rho_{\rm B}=30$. The transition waveform has $\rho_{\rm T}=30.000$, residual norm $\rho_{\rm R}=2.948$, and extrinsic-time-and-phase-maximized mismatch $\mathcal M_{\rm ext}=4.828\times10^{-3}$. A direct three-dimensional intrinsic profile refit reduces the mismatch to $5.95\times10^{-8}$ and shifts the best-fitting intrinsic parameters by $\Delta M/M=-3.32\times10^{-5}$, $\Delta\mu/\mu=2.11\times10^{-5}$, and $\Delta\hat a=-1.34\times10^{-6}$. In a zero-noise (Asimov) profile-likelihood calculation, the injected Kerr point has $\Delta\chi^2=8.67$ relative to the profiled best fit, outside the three-parameter 95\% contour but inside the 99\% contour for the adopted simplified likelihood. We also perform a six-parameter Fisher projection, but its condition number is $1.82\times10^{17}$ and the finite-difference step test does not converge; we therefore treat it only as a diagnostic of tangent-space degeneracy. The robust conclusion is that localized dissipative transitions can remain highly overlapping with nearby Kerr waveforms while producing detector-weighted residuals and a nominally significant profile-likelihood displacement in this restricted zero-noise waveform model.
Kerr EMRIs中局域耗散跃迁的探测器加权特征
摘要研究了圆形赤道克尔极端质量比涡(EMRI)耗散演化的参数化局域化修正。我们并没有声称一个独特的映射到一个特定的强子-夸克状态方程;相反,过渡扇区被视为具有参数$\{A_{\rm tr},f_c,\Delta f,p,q\}$的局部通量变形。参考灵感使用了黑洞摄动工具包\texttt{CircularOrbitSelfForceData}库中的真实Teukolsky通量数据,插值了表中的Kerr圆轨道通量的半径和自旋。对于具有$M=2\times10^{5}M_\odot$、$\mu=1.4M_\odot$、$\hat a=0.90$、$A_{\rm tr}=10^{-6}$、$f_c=0.0165~{\rm Hz}$和$\Delta f=0.009~{\rm Hz}$的代表性系统,我们将基线波形归一化为$\rho_{\rm B}=30$。过渡波形具有$\rho_{\rm T}=30.000$,残差范数$\rho_{\rm R}=2.948$和外部时间和相位最大化失配$\mathcal M_{\rm ext}=4.828\times10^{-3}$。直接的三维内在轮廓改装减少了对$5.95\times10^{-8}$的不匹配,并通过$\Delta M/M=-3.32\times10^{-5}$, $\Delta\mu/\mu=2.11\times10^{-5}$和$\Delta\hat a=-1.34\times10^{-6}$移动了最适合的内在参数。在零噪声(Asimov)剖面似然计算中,注入的Kerr点相对于剖面最佳拟合,在三参数95%轮廓之外,但在采用简化似然的99%轮廓内,其值为$\Delta\chi^2=8.67$。我们也进行了六参数Fisher投影,但其条件数为$1.82\times10^{17}$,有限差分步长检验不收敛;因此,我们只把它当作切线空间简并的诊断。强有力的结论是,局部耗散跃迁可以与附近的Kerr波形保持高度重叠,同时在这个受限的零噪声波形模型中产生检测器加权残差和名义上显著的剖面似然位移。
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来源期刊
Classical and Quantum Gravity
Classical and Quantum Gravity 物理-天文与天体物理
CiteScore
7.00
自引率
8.60%
发文量
301
审稿时长
2-4 weeks
期刊介绍: Classical and Quantum Gravity is an established journal for physicists, mathematicians and cosmologists in the fields of gravitation and the theory of spacetime. The journal is now the acknowledged world leader in classical relativity and all areas of quantum gravity.
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