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- W3141188894 abstract "Results from direct detection experiments are typically interpreted by employ- ing an assumption about the dark matter velocity distribution, with results presented in the m n plane. Recently methods which are independent of the DM halo velocity distribution have been developed which present results in the vmin ~ plane, but these in turn require an assumption on the dark matter mass. Here we present an extension of these halo-independent methods for dark matter direct detection which does not require a ducial choice of the dark matter mass. With a change of variables from vmin to nuclear recoil momentum (pR), the full halo-independent content of an experimental result for any dark matter mass can be con- densed into a single plot as a function of a new halo integral variable, which we call ~(pR). The entire family of conventional halo-independent ~(vmin) plots for all DM masses are directly found from the single ~(pR) plot through a simple rescaling of axes. By considering results in ~(pR) space, one can determine if two experiments are inconsistent for all masses and all physically possible halos, or for what range of dark matter masses the results are inconsistent for all halos, without the necessity of multiple ~(vmin) plots for dierent DM masses. We conduct a sample analysis comparing the CDMS II Si events to the null results from LUX, XENON10, and SuperCDMS using our method and discuss how the results can be strength- ened by imposing the physically reasonable requirement of a nite halo escape velocity." @default.
- W3141188894 created "2021-04-13" @default.
- W3141188894 creator A5001618966 @default.
- W3141188894 creator A5039100904 @default.
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- W3141188894 date "2009-01-01" @default.
- W3141188894 modified "2023-10-17" @default.
- W3141188894 title "ou rnal of Cosmology and Astroparticle Physics" @default.
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