Extended maximum likelihood halo-independent analysis of dark matter direct detection data

We extend and correct a recently proposed maximum-likelihood halo-independent method to analyze unbinned direct dark matter detection data. Instead of the recoil energy as independent variable we use the minimum speed a dark matter particle must have to impart a given recoil energy to a nucleus. This has the advantage of allowing us to apply the method to any type of target composition and interaction, e.g. with general momentum and velocity dependence, and with elastic or inelastic scattering. We prove the method and provide a rigorous statistical interpretation of the results. As rst applications, we nd that for dark matter particles with elastic spin-independent interactions and neutron to proton coupling ratio fn=fp = 0:7, the WIMP interpretation of the signal observed by CDMS- II-Si is compatible with the constraints imposed by all other experiments with null results. We also nd a similar compatibility for exothermic inelastic spin-independent interactions with fn=fp = 0:8.