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A weakly interacting massive particle (WIMP) weighing only a few GeV has beeninvoked as an explanation for the signal from the DAMA/LIBRA experiment. Weshow that the data from DAMA/LIBRA are now powerful enough to stronglyconstrain the properties of any putative WIMP. Accounting for the detailedrecoil spectrum, a light WIMP with a Maxwellian velocity distribution and aspin-independent (SI) interaction cannot account for the data. Even neglectingthe spectrum, much of the parameter space is excluded by limits from the DAMAunmodulated signal at low energies. Significant modifications to theastrophysics or particle physics can open light mass windows.

Using the Energy Spectrum at DAMA/LIBRA to Probe Light Dark Matter