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It has been suggested that dark matter particles which scatter inelasticallyfrom detector target nuclei could explain the apparent incompatibility of theDAMA modulation signal (interpreted as evidence for particle dark matter) withthe null results from CDMS-II and XENON10. Among the predictions ofinelastically interacting dark matter are a suppression of low-energy events,and a population of nuclear recoil events at higher nuclear recoil equivalentenergies. This is in stark contrast to the well-known expectation of a fallingexponential spectrum for the case of elastic interactions. We present a newanalysis of XENON10 dark matter search data extending to E$_{nr}=75$ keVnuclear recoil equivalent energy. Our results exclude a significant region ofpreviously allowed parameter space in the model of inelastically interactingdark matter. In particular, it is found that dark matter particle masses$m_{\chi}\gtrsim150$ GeV are disfavored.

Constraints on inelastic dark matter from XENON10