Hidden Markov model tracking of continuous gravitational waves from a binary neutron star with wandering spin. III. Rotational phase tracking

Abstract

A hidden Markov model (HMM) solved recursively by the Viterbi algorithm can be configured to search for persistent, quasimonochromatic gravitational radiation from an isolated or accreting neutron star, whose rotational frequency is unknown and wanders stochastically. Here an existing HMM analysis pipeline is generalized to track rotational phase and frequency simultaneously, by modeling the intrastep rotational evolution according to a phase-wrapped Ornstein-Uhlenbeck process, and by calculating the emission probability using a phase-sensitive version of the Bayesian matched filter known as the B-statistic, which is more sensitive than its predecessors. The generalized algorithm tracks signals from isolated and binary sources with characteristic wave strain h₀ ≥ 1.3 × 10⁻²⁶ in Gaussian noise with amplitude spectral density 4 × 10⁻²⁴ Hz^(−1/2), for a simulated observation composed of N_T = 37 data segments, each T_(drift) = 10 days long, the typical duration of a search for the low-mass x-ray binary (LMXB) Sco X−1 with the Laser Interferometer Gravitational Wave Observatory (LIGO). It is equally sensitive to isolated and binary sources and ≈1.5 times more sensitive than the previous pipeline, which achieves h₀ ≥ 2.0 × 10⁻²⁶ for a comparable search. Receiver operating characteristic curves (to demonstrate a recipe for setting detection thresholds) and errors in the recovered parameters are presented for a range of practical h₀ and N_T values. The generalized algorithm successfully detects every available synthetic signal in Stage I of the Sco X−1 Mock Data Challenge convened by the LIGO Scientific Collaboration, recovering the frequency and orbital semimajor axis with accuracies of better than 9.5 × 10⁻⁷ Hz (one part in ∼10⁸) and 1.6 × 10⁻³ lt s (one part in ∼10³) respectively. The Viterbi solver runs in ≈2 × 10³ CPU-hr for an isolated source and ∼10⁵ CPU-hr for a LMXB source in a typical, broadband (0.5-kHz) search, i.e., ≲10 times slower than the previous pipeline.

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