pith. sign in

Therefore Υ(L) ab (θ, ϕ, ζ) = cos2 θ 2(1 + cosθ) (sinθsinζcosϕ+ cosθcosζ) 2 1 + sinθsinζcosϕ+ cosθcosζ

Longitudinal scalar mode F L a (θ) = √ 2 2 cos2 θ 1 + cosθ , F L b (θ, ϕ, ζ) = √ 2 2 (sinθsinζcosϕ+ cosθcosζ) 2 1 + sinθsinζcosϕ+ cosθcosζ

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gr-qc 1

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2026 1

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Testing General Relativity with Individual Supermassive Black Hole Binaries

gr-qc · 2026-05-06 · unverdicted · novelty 6.0

A framework is developed to test beyond-GR effects in nanohertz continuous waves from individual SMBHBs, deriving modified inter-pulsar correlations, antenna responses, and phase delays for three deviation classes, validated by injection-recovery simulations showing parameter recovery and no GR bias

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  • Testing General Relativity with Individual Supermassive Black Hole Binaries gr-qc · 2026-05-06 · unverdicted · none · ref 4

    A framework is developed to test beyond-GR effects in nanohertz continuous waves from individual SMBHBs, deriving modified inter-pulsar correlations, antenna responses, and phase delays for three deviation classes, validated by injection-recovery simulations showing parameter recovery and no GR bias