2017
DOI: 10.1590/2236-463320171701
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Exilé(e)s et migrant(e)s transatlantiques: histoires entremêlées, historiographies parallèles

Abstract: Exilé(es) et migrant(e)s transatlantiques: histoires entremêlées, historiographies parallèles 12 fórum Sylvie Aprile Exilé(es) et migrant(e)s transatlantiques: histoires entremêlées, historiographies parallèles

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Cited by 29 publications
(41 citation statements)
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“…Since this corresponds to a very fine-tuned parameter space, we do not look into the details of it in the present work. by the recent bounds from direct detection experiments like LUX [6], PandaX-II [7] and XENON1T [8]. For scalar dark matter considered in this work, the relevant spin independent scattering cross section mediated by SM Higgs is given as [20] …”
Section: Dark Matter In Ihdmmentioning
confidence: 99%
“…Since this corresponds to a very fine-tuned parameter space, we do not look into the details of it in the present work. by the recent bounds from direct detection experiments like LUX [6], PandaX-II [7] and XENON1T [8]. For scalar dark matter considered in this work, the relevant spin independent scattering cross section mediated by SM Higgs is given as [20] …”
Section: Dark Matter In Ihdmmentioning
confidence: 99%
“…Of course, the density of neutralinos could be diluted if there was additional entropy production [41] during the history of the Universe. The current reach of the LUX experiment [42] is shown as red-solid while the XENON1T reach [43] is purple-dashed. We see that the current LUX experiment has just started to probe the parameter space with ξ = 1 while all of this space will be probed by XENON1T.…”
Section: Wimp Signals From Ngmmmentioning
confidence: 99%
“…We see that the current LUX experiment has just started to probe the parameter space with ξ = 1 while all of this space will be probed by XENON1T. Multi-ton noble liquid detectors such as LZ [44], XENONnT (20tY exposure) [43], DarkSide-20K [45], DEAP-50T [46] and DARWIN [47] will be required to probe the entire parameter space with ξ < 1. We note these detection rates are lower than expected from natural NUHM2 models [48,49] since both ξ is reduced and also with heavier electroweakino masses, the LSP is more pure higgsino-like in nGMM.…”
Section: Wimp Signals From Ngmmmentioning
confidence: 99%
“…The tank is equipped with an active muon veto with 84 PMTs, allowing a 99% efficiency in tagging crossing muons and 74% efficiency for showering events. The expected total background is expected to be around 0.01 event per year [7]. The water tank was completed in fall of 2013 and it is shown on the left of Fig.…”
Section: Expected Background and Sensitivitymentioning
confidence: 99%