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The LISA Time-Delay Interferometry Zero-Signal Solution. I: Geometrical Properties

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arxiv gr-qc/0405147 v1 pith:7A2J55XD submitted 2004-05-30 gr-qc

classification gr-qc
keywords gravitationaldatawavecombinationsinterferometriclisainterferometrymethod
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Time-Delay Interferometry (TDI) is the data processing technique needed for generating interferometric combinations of data measured by the multiple Doppler readouts available onboard the three LISA spacecraft. Within the space of all possible interferometric combinations TDI can generate, we have derived a specific combination that has zero-response to the gravitational wave signal, and called it the {\it Zero-Signal Solution} (ZSS). This is a two-parameter family of linear combinations of the generators of the TDI space, and its response to a gravitational wave becomes null when these two parameters coincide with the values of the angles of the source location in the sky. Remarkably, the ZSS does not rely on any assumptions about the gravitational waveform, and in fact it works for waveforms of any kind. Our approach is analogous to the data analysis method introduced by G\"ursel & Tinto in the context of networks of Earth-based, wide-band, interferometric gravitational wave detectors observing in coincidence a gravitational wave burst. The ZSS should be regarded as an application of the G\"ursel & Tinto method to the LISA data.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Distinguishing Monochromatic Signals in LISA and Taiji: Ultralight Dark Matter versus Gravitational Waves

    hep-ph 2025-06 conditional novelty 7.0 of 10

    Null-response interferometric channels can separate monochromatic ultralight dark matter signals from gravitational waves in LISA and Taiji, most effectively at high frequencies.

  2. Testing the Transverse Scalar Mode of Gravitational Quantum Field Theory with Taiji and LISA

    gr-qc 2026-07 conditional novelty 6.0 of 10

    A null-response channel for LISA/Taiji can isolate GQFT's breathing scalar mode, and orbital motion boosts the low-frequency response by about four orders of magnitude.

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