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High-Dimensional Bayesian Likelihood Normalisation for CRESST's Background Model

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arxiv 2307.12991 v2 pith:HMHHN7RK submitted 2023-07-19 physics.ins-det astro-ph.IMhep-ex

High-Dimensional Bayesian Likelihood Normalisation for CRESST's Background Model

classification physics.ins-det astro-ph.IMhep-ex
keywords backgroundcresstmodelbayesianexperimentallikelihoodmethodnormalisation
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Using CaWO$_4$ crystals as cryogenic calorimeters, the CRESST experiment searches for nuclear recoils caused by the scattering of potential Dark Matter particles. A reliable identification of a potential signal crucially depends on an accurate background model. In this work we introduce an improved normalisation method for CRESST's model of the electromagnetic backgrounds. Spectral templates, based on Geant4 simulations, are normalised via a Bayesian likelihood fit to experimental background data. Contrary to our previous work, no assumption of partial secular equilibrium is required, which results in a more robust and versatile applicability. Furthermore, considering the correlation between all background components allows us to explain 82.7% of the experimental background within [1 keV, 40 keV], an improvement of 18.6% compared to our previous method.

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