Investigating correlations in time delay interferometry combinations of LISA data

作者: Jennifer Toher

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摘要: The detection of Gravitational Waves using the Laser Interferometer Space Antenna (LISA) will open whole new areas physics and astrophysics for exploration. lower frequency signals detected by antenna allow us to probe gravitational wave sources that are inaccessible with current future ground based detectors. However, ability LISA detect is dependent on removal laser noise realisations from optical bench measurements, would otherwise dominate signal data streams. Time Delay Interferometry (TDI) provides a method removing contributions time shifting individual measurements. cancellation achieved identifying measurements contain equal numbers identical but opposing signs. Although TDI combinations produce datastreams free contributions, means combination streams defined at different stamps nevertheless remaining detector terms. Independent (denoted A, E T) can be constructed simpler laser-noise cancelling diagonalising correlation matrix any given timestamp. This ensures optimal independent respect each other this particular timestamp, result does not apply when compared timestamps. As introduces within them identically terms, T could therefore correlated in time. The presence, potential impact, these correlations has been investigated first thesis. work carried out designations terms algebraic expression combination. resultant configuration non-zero off-diagonal covariance simplified models constellation. The presence between pose serious problem number parameter search methods rely being independent. The effects recovery containing two sinusoids model produced second Mock Data Challenge. In both cases, auto cross combinations. When covariances were explicitly accounted likelihood function, confidence intervals, reflecting uncertainty our inference unknown parameters, found significantly smaller - indicating tighter constraints true comparison results obtained function assumed time.

参考文章(41)
Shane L. Larson, LISA: A Modern Astrophysical Observatory 33rd SLAC Summer Institute on Particle Physics: Gravity in the Quantum World and the Cosmos, SSI 2005. pp. 41- 41 ,(2005)
Thomas A. Prince, Massimo Tinto, Shane L. Larson, J. W. Armstrong, The LISA optimal sensitivity Physical Review D. ,vol. 66, pp. 122002- ,(2002) , 10.1103/PHYSREVD.66.122002
Michele Vallisneri, John G. Baker, Keith A. Arnaud, Alberto Vecchio, Shane L. Larson, Jean-Yves Vinet, Stanislav Babak, Matthew J. Benacquista, B. S. Sathyaprakash, Curt Cutler, Neil J. Cornish, A How-To for the Mock LISA Data Challenges Sixth International LISA Symposium. pp. 625- 632 ,(2006)
Shane L. Larson, Online Sensitivity Curve Generator ,(2002)
Scott A. Hughes, A brief survey of LISA sources and science LASER INTERFEROMETER SPACE ANTENNA: 6th International LISA Symposium. ,vol. 873, pp. 13- 20 ,(2006) , 10.1063/1.2405017
Bernard F. Schutz, A first course in general relativity ,(1985)
Massimo Tinto, Daniel A. Shaddock, Julien Sylvestre, J. W. Armstrong, Implementation of time-delay interferometry for LISA Physical Review D. ,vol. 67, pp. 122003- ,(2003) , 10.1103/PHYSREVD.67.122003