ﻻ يوجد ملخص باللغة العربية
There are many theories where a dark matter particle is part of a multiplet with an electrically charged state. If WIMP dark matter ($chi^{0}$) is accompanied by a charged excited state ($chi^{-}$) separated by a small mass difference, it can form a stable bound state with a nucleus. In supersymmetric models, the $chi^{0}$ and the $chi^{-}$ could be the neutralino and a charged slepton, such as the neutralino-stau degenerate model. The formation binding process is expected to result in an energy deposition of {it O}(1--10 MeV), making it suitable for detection in large liquid scintillator detectors. We describe new constraints on the bound state formation with a xenon nucleus using the KamLAND-Zen 400 Phase-II dataset. In order to enlarge the searchable parameter space, all xenon isotopes in the detector were used. For a benchmark parameter set of $m_{chi^{0}} = 100$ GeV and $Delta m = 10$ MeV, this study sets the most stringent upper limits on the recombination cross section $langlesigma vrangle$ and the decay-width of $chi^{-}$ of $2.0 times 10^{-31}$ ${rm cm^3/s}$ and $1.1 times 10^{-18}$ GeV, respectively (90% confidence level).
A search for double-beta decays of 136Xe to excited states of 136Ba has been performed with the first phase data set of the KamLAND-Zen experiment. The 0+1, 2+1 and 2+2 transitions of 0{ u}{beta}{beta} decay were evaluated in an exposure of 89.5kg-yr
This Letter reports results from a haloscope search for dark matter axions with masses between 2.66 and 2.81 $mu$eV. The search excludes the range of axion-photon couplings predicted by plausible models of the invisible axion. This unprecedented sens
NEWAGE is a direction-sensitive dark matter search using a low-pressure gaseous time projection chamber. A low alpha-ray emission rate micro pixel chamber had been developed in order to reduce background for dark matter search. We conducted the dark
The Dark Matter Time Projection Chamber (DMTPC) is a low pressure (75 Torr CF4) 10 liter detector capable of measuring the vector direction of nuclear recoils with the goal of directional dark matter detection. In this paper we present the first dark
We report the result of a search for neutrinos in coincidence with solar flares from the GOES flare database. The search was performed on a 10.8 kton-year exposure of KamLAND collected from 2002 to 2019. We found no statistical excess of neutrinos an