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Correlation analysis of stochastic gravitational wave background around 0.1-1Hz

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arxiv gr-qc/0510067 v3 pith:4GVJEZI6 submitted 2005-10-14 gr-qc astro-ph

Naoki Seto This is my paper · ORCID
classification gr-qcastro-ph
keywords backgroundanalysisaroundcorrelationgravitationalmissionsstochasticwave
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We discuss prospects for direct measurement of stochastic gravitational wave background around 0.1-1Hz with future space missions. It is assumed to use correlation analysis technique with the optimal TDI variables for two sets of LISA-type interferometers. The signal to noise for detection of the background and the estimation errors for its basic parameters (amplitude, spectral index) are evaluated for proposed missions.

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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. RGE effects on new physics searches via gravitational waves

    hep-ph 2025-05 conditional novelty 6.0 of 10

    Future GW experiments retain sensitivity to several SMEFT operators despite renormalization scale uncertainties, provided the leading (H†H)^3 operator is measured by colliders.

  2. Electroweak phase transition in SMEFT: Gravitational wave and collider complementarity

    hep-ph 2025-12 conditional novelty 5.0 of 10

    Strong first-order electroweak phase transitions in dimension-6 SMEFT can be probed by future gravitational wave detectors and by di-Higgs production at the HL/HE-LHC, with correlated sensitivity regions.

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