2015
DOI: 10.1103/physrevlett.114.111302
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First Direct Limits on Lightly Ionizing Particles with Electric Charge Less than e/6

Abstract: While the standard model of particle physics does not include free particles with fractional charge, experimental searches have not ruled out their existence. We report results from the Cryogenic Dark Matter Search (CDMS II) experiment that give the first direct-detection limits for cosmogenically produced relativistic particles with electric charge lower than e=6. A search for tracks in the six stacked detectors of each of two of the CDMS II towers finds no candidates, thereby excluding new parameter space fo… Show more

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Cited by 25 publications
(19 citation statements)
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“…One immediate consequence of our calculation of the cosmic ray-induced MCP flux is that existing bounds on a naturally occurring flux of MCPs can be converted into constraints on Lagrangian parameters and m χ , where the MCP charge is Q χ = × e. In fact, multiple such bounds already exist in the literature, but have never been translated into the − m χ plane because the relation between , m χ and the flux from cosmic rays had never been made explicit. Examples include constraints from MACRO [56,57], Kamiokande-II [64], LSD [65], CDMS [66] and Majorana [58]. Interestingly we find the resulting constraints to be roughly competitive with those from existing collider experiments, but sub-dominant to reported bounds from neutrino experiments [16,59,60].…”
Section: Introductionmentioning
confidence: 57%
“…One immediate consequence of our calculation of the cosmic ray-induced MCP flux is that existing bounds on a naturally occurring flux of MCPs can be converted into constraints on Lagrangian parameters and m χ , where the MCP charge is Q χ = × e. In fact, multiple such bounds already exist in the literature, but have never been translated into the − m χ plane because the relation between , m χ and the flux from cosmic rays had never been made explicit. Examples include constraints from MACRO [56,57], Kamiokande-II [64], LSD [65], CDMS [66] and Majorana [58]. Interestingly we find the resulting constraints to be roughly competitive with those from existing collider experiments, but sub-dominant to reported bounds from neutrino experiments [16,59,60].…”
Section: Introductionmentioning
confidence: 57%
“…Hence, the limits presented . Results from MACRO [55], Kamiokande-II [56], LSD [57], and CDMS [59] are shown as well. All limits assume an isotropic flux.…”
mentioning
confidence: 95%
“…Direct searches for LIPs, including MACRO [54,55], Kamiokande-II [56], and LSD [57] placed stringent limits on the LIP flux for 0.4 < f < 6. The Cryogenic Dark Matter Search (CDMS) experiment [58,59] placed limits on exotic particles with f < 200 using a direct search technique. A 2009 review [60] summarizes the experimental state of the field prior to the results of CDMS in 2010.…”
mentioning
confidence: 99%
“…MCPs are heavily explored in terrestrial experiments, and their signatures as dark matter is also studied in astrophysical/cosmological observations [246,[394][395][396][397][398][399][400][401][402][403][404]. Our focus here is to briefly describe and classify the accelerator-based probes.…”
Section: Introductionmentioning
confidence: 99%