Improving the sensitivity of LISA

被引:25
作者
Nayak, KR [1 ]
Pai, A
Dhurandhar, SV
Vinet, JY
机构
[1] Interuniv Ctr Astron & Astrophys, Pune, Maharashtra, India
[2] Observ Cote Azur, Dept Fresnel, ILGA, F-06304 Nice, France
关键词
D O I
10.1088/0264-9381/20/7/301
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It has been shown in several recent papers that the six Doppler data streams obtained from a triangular LISA configuration can be combined by appropriately delaying the data streams for cancelling the laser frequency noise. Raw laser noise is several orders of magnitude above the other noises and thus it is essential to bring it down to the level of other noises such as shot, acceleration, etc. A rigorous and systematic formalism using the powerful techniques of computational commutative algebra was developed, which generates in principle all the data combinations cancelling the laser frequency noise. The relevant data combinations form a first module of syzygies. In this paper, we use this formalism to advantage for optimizing the sensitivity of LISA by analysing the noise and signal covariance matrices. The signal covariance matrix is calculated for binaries whose frequency changes at most adiabatically and the signal is averaged over polarizations and directions. We then present the extremal SNR curves for all the data combinations in the module. They correspond to the eigenvectors of the noise and signal covariance matrices. A LISA 'network' SNR is also computed by combining the outputs of the eigenvectors. We show that substantial gains in sensitivity can be obtained by employing these strategies. The maximum SNR curve can yield an improvement up to 70% over the Michelson, mainly at high frequencies, while the improvement using the network SNR ranges from 40% to over 100%. Finally, we describe a simple toy model, in which LISA rotates in a. plane. In this analysis, we estimate the improvement in the LISA sensitivity, if one switches from one data combination to another as it rotates. Here the improvement in sensitivity, if one switches optimally over three cyclic data combinations of the eigenvector, is about 55% on average over the LISA bandwidth. The corresponding SNR improvement increases to 60%, if one maximizes over the module.
引用
收藏
页码:1217 / 1231
页数:15
相关论文
共 9 条
[1]   Time-delay interferometry for space-based gravitational wave searches [J].
Armstrong, JW ;
Estabrook, FB ;
Tinto, M .
ASTROPHYSICAL JOURNAL, 1999, 527 (02) :814-826
[2]  
BENDER P, 2000, SYSTEM TECHNOLOGY ST, P11
[3]   Detection of gravitational waves using a network of detectors [J].
Bose, S ;
Dhurandhar, SV ;
Pai, A .
PRAMANA-JOURNAL OF PHYSICS, 1999, 53 (06) :1125-1136
[4]   Algebraic approach to time-delay data analysis for LISA [J].
Dhurandhar, SV ;
Nayak, KR ;
Vinet, JY .
PHYSICAL REVIEW D, 2002, 65 (10)
[5]   Time-delay analysis of LISA gravitational wave data: Elimination of spacecraft motion effects [J].
Estabrook, FB ;
Tinto, M ;
Armstrong, JW .
PHYSICAL REVIEW D, 2000, 62 (04) :art. no.-042002
[6]  
GRAYSON DR, MACAULAY2 SOFWARE
[7]  
PRINCE TA, 2002, GRQC0209039
[8]   Time-delay interferometry for LISA [J].
Tinto, M ;
Estabrook, FB ;
Armstrong, JW .
PHYSICAL REVIEW D, 2002, 65 (08) :820031-8200312
[9]   Cancellation of laser noise in an unequal-arm interferometer detector of gravitational radiation [J].
Tinto, M ;
Armstrong, JW .
PHYSICAL REVIEW D, 1999, 59 (10) :1-11