On the calculation of p-values for quadratic statistics in Pulsar Timing Arrays
Rutger van Haasteren

TL;DR
This paper critically examines methods for calculating p-values in Pulsar Timing Arrays, revealing that commonly used scrambling techniques are not truly model-independent and advocating for Bayesian and Frequentist approaches based on the generalized chi-squared distribution.
Contribution
The paper provides a rigorous analysis of p-value calculation methods in PTAs, demonstrating the limitations of scrambling techniques and deriving analytical expressions for the generalized chi-squared distribution.
Findings
Scrambling methods are not truly model-independent.
Existing p-value calculations in PTA literature are incorrect.
Analytical expressions for the generalized chi-squared distribution are derived.
Abstract
Pulsar Timing Array (PTA) projects have reported various lines of evidence suggesting the presence of a stochastic gravitational wave (GW) background in their data. One key line of evidence involves a detection statistic sensitive to inter-pulsar correlations, such as those induced by GWs. A -value is then calculated to assess how unlikely it is for the observed signal to arise under the null hypothesis , purely by chance. However, PTAs cannot empirically draw samples from . As a workaround, various techniques are used in the literature to approximate -values under . One such technique, which has been heralded as a model-independent method, is the use of "scrambling" transformations that modify the data to cancel out pulsar correlations, thereby simulating realizations from . In this work, scrambling methods and the detection statistic are investigated from…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Scientific Research and Discoveries · Statistical Mechanics and Entropy
