Wavefront error based tilt-to-length noise analysis for the LISA transmitted beam

被引：8
作者：
Weaver, Alexander Joseph [1 ]
Mueller, Guido [1 ]
Fulda, Paul J. [1 ]
机构：
[1] Univ Florida, Dept Phys, 2001 Museum Rd,POB 118440, Gainesville, FL 32611 USA
来源：
CLASSICAL AND QUANTUM GRAVITY | 2022年 / 39卷 / 19期
关键词：
LISA; Zernike; WFE; interferometry;
D O I：
10.1088/1361-6382/ac8a88
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The laser interferometer space antenna (LISA) will open the signal-rich 100 mu Hz to 1 Hz gravitational wave window. LISA is expected to be limited by acceleration noise in the low frequency range and noise associated with the optical measurement system above a few mHz. Of the latter, apparent length changes due to spacecraft (SC) angular jitter are among the most critical contributors. One of the coupling mechanisms is via wavefront error in the transmitted beam. Utilizing a Zernike polynomial decomposition of such wavefront error, we introduce and explore the validity of extremely fast best fit polynomial expansion based noise recreation tools that provide a clear picture for which transmit beam perturbations couple most strongly with SC jitter into LISA noise.
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页数：20
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