Optimal Strategies for Gravitational Wave Memory Detection in Pulsar Timing Arrays

• Main Authors: Sun, Jerry P, Siemens, Xavier, Madison, Dustin R
• Format: Journal Article
• Language: English
• Published: 25.10.2024
• Subjects: Physics - General Relativity and Quantum Cosmology
• DOI: 10.48550/arxiv.2410.19977

In this work we derive two computationally efficient frequentist detection statistics that can be used in searches for gravitational-wave bursts with memory in pulsar timing data. By maximizing the likelihood ratio in two different ways we construct a coherent statistic and an incoherent statistic, which are analogs of the $\pazocal{F}_e$ and $\pazocal{F}_p$ statistics commonly used for continuous-wave searches in pulsar timing data. We show that both statistics are $\chi^2$-distributed with varying degrees of freedom and non-centrality parameters given by the signal-to-noise (SNR) ratio of the signal present in our data. The statistics can also be used to compute the maximum likelihood estimators of amplitude parameters of a possible gravitational-wave memory signal in pulsar timing data. We find that in the low-signal regime ($\mathrm{SNR} \lesssim 5$), the estimators are inaccurate. However, in intermediate- to high-signal regimes, we show that these estimators can accurately determine the correct signal parameters.