“…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] …”
“…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] …”
“…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.…”
In the supersymmetric scenario known as mirage mediation (MM), the soft SUSY
breaking terms receive comparable anomaly-mediation and moduli-mediation
contributions leading to the phenomenon of mirage unification. The simplest MM
SUSY breaking models which are consistent with the measured Higgs mass and
sparticle mass constraints are strongly disfavoured by fine-tuning
considerations. However, while MM makes robust predictions for gaugino masses,
the scalar sector is quite sensitive to specific mechanisms for moduli
stabilization and potential uplifting. We suggest here a broader setup of
generalized mirage mediation (GMM), where heretofore discrete parameters are
allowed as continuous to better parametrize these other schemes. We find that
natural SUSY spectra consistent with both the measured value of m(h). as well
as LHC lower bounds on superpartner masses are then possible. We explicitly
show that models generated from natural GMM may be beyond the reach of even
high-luminosity LHC searches. In such a case, the proposed International Linear
e^+e^- Collider (ILC) will be required for natural SUSY discovery via higgsino
pair production reactions. We also outline prospects for detection of
higgsino-like WIMPs from natural GMM.Comment: 18 pages plus 7 .png figures; this revised version corrects a
numerical error in the published version wherein a benchmark input value is
corrected to be a_3=5.
“…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
Abstract. The XENON Dark Matter Experiment has been ongoing at LNGS since 2005 with the goal of searching for dark matter WIMPs with liquid xenon as target and detector material. With detectors of increasing target mass and decreasing background, the XENON program has achieved competitive limits on WIMP-nucleon interaction couplings, but also on axions and axion like particles. With the start of the next generation experiment, XENON1T expected in 2015, XENON Dark Matter Experiment will continue to lead field of dark matter direct detection. XENON1T will be the first experiment to use multi-tons of liquid xenon in a time projection chamber and is designed to achieve two orders of magnitude higher sensitivity than the current best limits. I will review the status of construction and the scientific goals of XENON1T.
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