Analytic weak-signal approximation of the Bayes factor for continuous gravitational waves

Abstract

We generalize the targeted $\mathcal{B}$-statistic for continuous gravitational waves by modeling the $h_0$-prior as a half-Gaussian distribution with scale parameter $H$. This approach retains analytic tractability for two of the four amplitude marginalization integrals and recovers the standard $\mathcal{B}$-statistic in the strong-signal limit ($H\to \infty$). By Taylor-expanding the weak-signal regime ($H\to 0$), the new prior enables fully analytic amplitude marginalization, resulting in a simple, explicit statistic that is as computationally efficient as the maximum-likelihood $\mathcal{F}$-statistic, but significantly more robust. Numerical tests show that for day-long coherent searches, the weak-signal Bayes factor achieves sensitivities comparable to the $\mathcal{F}$-statistic, though marginally lower than the standard $\mathcal{B}$-statistic (and the Bero-Whelan approximation). In semi-coherent searches over short (compared to a day) segments, this approximation matches or outperforms the weighted dominant-response ${\mathcal{F}}_{\mathrm{ABw}}$-statistic and returns to the sensitivity of the (weighted) ${\mathcal{F}}_{\mathrm{w}}$-statistic for longer segments. Overall the new Bayes-factor approximation demonstrates state-of-the-art or improved sensitivity across a wide range of segment lengths we tested (from 900s to 10days).

27 pages, 4 figures, submitted to CQG v2: added appendix showing translation to 5-vector framework v3: fixed minor equation typos (incl sign error in Appendix A), corrigendum submitted to CQG

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Cited by in corpus (3)

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• One-stop strategy to search for long-duration gravitational-wave signals
• Narrowband searches for continuous gravitational waves from known pulsars in the first two parts of the fourth LIGO--Virgo--KAGRA observing run