Optimal design of interpolation methods for time-delay interferometry

IF 3.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Martin Staab, Jean-Baptiste Bayle, Olaf Hartwig, Aurélien Hees, Marc Lilley, Graham Woan and Peter Wolf
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Abstract

Time-delay interferometry (TDI) suppresses laser frequency noise by forming linear combinations of time-shifted interferometric measurements. The time-shift operation is implemented by interpolating discretely sampled data. To enable in-band laser noise reduction by eight to nine orders of magnitude, interpolation has to be performed with high accuracy. Interpolation can be understood as the convolution of an interpolation kernel with the data to be shifted. Optimizing the design of this interpolation kernel is the focus of this work. Previous research that studied constant time-shifts suggested Lagrange interpolation as the interpolation method for TDI. Its transfer function is maximally flat at DC and therefore performs well at low frequency. However, to be accurate at high frequencies, Lagrange interpolation requires a high number of coefficients. Furthermore, when applied in TDI we observed prominent time-domain features when a time-varying shift scanned over a pure integer sample shift. To limit this effect we identify an additional requirement for the interpolation kernel: when considering time-varying shifts the interpolation kernel must be sufficiently smooth to avoid unwanted time-domain transitions that produce glitch-like features in power spectral density estimates. The Lagrange interpolation kernel exhibits a discontinuous first derivative by construction, which is insufficient for the application to LISA or other space-based gravitational-wave observatories. As a solution we propose a novel design method for interpolation kernels that respect a predefined requirement on in-band interpolation residuals and that possess continuous derivatives up to a prescribed order. Using this method we show that an interpolation kernel with 22 coefficients is sufficient to respect LISA’s picometre-requirement and to allow for a continuous first derivative which suppresses the magnitude of the time-domain transition adequately. The reduction from 42 (Lagrange interpolation) to 22 coefficients enables us to increase robustness against artifacts in the data and, as a side effect, save computational cost.
延时干涉测量插值方法的优化设计
延时干涉(TDI)通过形成时移干涉测量的线性组合来抑制激光频率噪声。时移运算是通过插值离散采样数据来实现的。为了使带内激光噪声降低8到9个数量级,必须以高精度进行插值。插值可以理解为插值核与待移位数据的卷积。该插值核的优化设计是本工作的重点。以往研究恒定时移的研究建议拉格朗日插值作为TDI的插值方法。它的传递函数在直流时最平坦,因此在低频时表现良好。然而,为了在高频率下精确,拉格朗日插值需要大量的系数。此外,当应用于TDI时,我们观察到当时变移位扫描纯整数样本移位时的突出时域特征。为了限制这种影响,我们确定了对插值核的额外要求:当考虑时变位移时,插值核必须足够平滑,以避免在功率谱密度估计中产生类似故障的不必要的时域过渡。拉格朗日插值核在构造上表现出不连续的一阶导数,这不足以应用于LISA或其他天基引力波天文台。作为一种解决方案,我们提出了一种新的插值核设计方法,该方法尊重对带内插值残差的预定义要求,并具有高达规定阶的连续导数。使用这种方法,我们证明了具有22个系数的插值核足以满足LISA的皮米要求,并允许连续的一阶导数,这充分抑制了时域跃迁的幅度。从42个(拉格朗日插值)系数减少到22个系数使我们能够增加对数据中的伪象的鲁棒性,并且作为副作用,节省了计算成本。
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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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