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Gravitational Wave Background Search by Correlating Multiple Triangular Detectors in the mHz Band

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arxiv 2010.06877 v2 pith:CPXQ7C3H submitted 2020-10-14 gr-qc astro-ph.CO

classification gr-qcastro-ph.CO
keywords detectortriangularbackgroundbanddetectorsevaluateformulationgravitational
verification ladder T0 review T1 audit T2 compute T3 formal
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With the recent strong developments of TianQin and Taiji, we now have an increasing chance to make a correlation analysis in the mHz band by operating them together with LISA. Assuming two LISA-like triangular detectors at general geometrical configurations, we develop a simple formulation to evaluate the network sensitivity to an isotropic gravitational wave background. In our formulation, we fully use the symmetry of data channels within each triangular detector and provide tractable expressions without directly employing cumbersome detector tensors. We concretely evaluate the expected network sensitivities for various potential detector combinations, including the LISA-TianQin pair.

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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. Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors

    gr-qc 2025-10 conditional novelty 6.0 of 10

    Eccentric black-hole-binary backgrounds from globular clusters and isolated evolution would look like power-law noise for TianQin/LISA/Taiji, but AGN-formed binaries produce a turnover that LISA and Taiji can distinguish.

  2. Alternative LISA-TAIJI networks: polarization separation of the stochastic gravitational wave background

    gr-qc 2026-08 conditional novelty 5.0 of 10

    For stochastic gravitational wave backgrounds containing simultaneous tensor, vector, and scalar modes, the more inclined LISA-TAIJIm network separates polarization components substantially better than LISA-TAIJIp, al...

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