2014
DOI: 10.1142/s0217751x14430076
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New class of biological detectors for WIMPs

Abstract: Abstract:Weakly Interacting Massive Particles (WIMPs) may constitute a large fraction of the matter in the Universe. There are excess events in the data of DAMA/LIBRA, CoGeNT, CRESST-II, and recently CDMS-Si, which could be consistent with WIMP masses of approximately 10 GeV/c 2 . However, for M DM > 10 GeV/c 2 null results of the CDMS-Ge, XENON, and LUX detectors may be in tension with the potential detections for certain dark matter scenarios and assuming a certain light response.We propose the use of a new … Show more

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Cited by 17 publications
(24 citation statements)
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References 59 publications
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“…Hence, it constitutes an extension of direction-insensitive direct detection, for which only the energy is measured. Several directional detection strategies have been proposed: low pressure gaseous Time Projection Chambers (TPCs) [21][22][23][24][25][26][27][28][29], nuclear emulsions [30,31], columnar recombination in high-pressure gaseous Xenon TPCs [32][33][34], solid-state detectors [35][36][37], DNA-based detectors [38], graphene-based heterostructures [39] and polarized detectors [40]. Not all techniques are equally mature.…”
Section: Experimental Framework a Introductionmentioning
confidence: 99%
“…Hence, it constitutes an extension of direction-insensitive direct detection, for which only the energy is measured. Several directional detection strategies have been proposed: low pressure gaseous Time Projection Chambers (TPCs) [21][22][23][24][25][26][27][28][29], nuclear emulsions [30,31], columnar recombination in high-pressure gaseous Xenon TPCs [32][33][34], solid-state detectors [35][36][37], DNA-based detectors [38], graphene-based heterostructures [39] and polarized detectors [40]. Not all techniques are equally mature.…”
Section: Experimental Framework a Introductionmentioning
confidence: 99%
“…10). We proposed 76 to use nanometer thin sheets of gold (or other material) with ∼10 60 strands of DNA attached. When a WIMP hits the gold sheet, it knocks a gold atom forward into the DNA.…”
Section: And Xenonmentioning
confidence: 99%
“…On the other hand, considering that the luminous Universe -which accounts just for less than 1% of the Universe density -is so rich of different particles, it is reasonable to expect that the DM -which is instead about 26% of itcould also be accounted by more than a single type of DM particles. In particular, a new experiment to search for the presence of axion candidates is presented in Preface the paper by T. M. Shokair et al 4 A new project, aiming a very deep subtraction of the electromagnetic component of the counting rate assuming the case of DM particles inducing just nuclear recoils, is discussed in the paper by R. Bertoni et al 5 The possible developments of new detector technologies are discussed in the two following papers by A. K. Drukier et al, 6,7 which potentially offer the possibility to exploit the directionality approach for the class of DM candidates considered there and, in every case, the development of totally new technologies.…”
Section: Prefacementioning
confidence: 99%