Maximum Likelihood Analysis of Low Energy CDMS II Germanium Data
SuperCDMS Collaboration: R. Agnese, A.J. Anderson, D. Balakishiyeva,, R. Basu Thakur, D.A. Bauer, J. Billard, A. Borgland, M.A. Bowles, D. Brandt,, P.L. Brink, R. Bunker, B. Cabrera, D.O. Caldwell, D.G. Cerdeno, H. Chagani,, Y. Chen, J. Cooley, B. Cornell, C.H. Crewdson

TL;DR
This study uses maximum likelihood analysis on low-energy CDMS II germanium data to search for WIMP signals, finding no significant evidence and highlighting issues with previous background models.
Contribution
It introduces a detailed background modeling approach and critically evaluates prior claims of WIMP detection in the same dataset.
Findings
No statistically significant WIMP signal detected
Background model based on GEANT4 fits the data well
Previous claimed excesses are attributed to background model inadequacies
Abstract
We report on the results of a search for a Weakly Interacting Massive Particle (WIMP) signal in low-energy data of the Cryogenic Dark Matter Search (CDMS~II) experiment using a maximum likelihood analysis. A background model is constructed using GEANT4 to simulate the surface-event background from Pb decay-chain events, while using independent calibration data to model the gamma background. Fitting this background model to the data results in no statistically significant WIMP component. In addition, we perform fits using an analytic ad hoc background model proposed by Collar and Fields, who claimed to find a large excess of signal-like events in our data. We confirm the strong preference for a signal hypothesis in their analysis under these assumptions, but excesses are observed in both single- and multiple-scatter events, which implies the signal is not caused by WIMPs, but…
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