scholarly journals Low-mass WIMP searches with the EDELWEISS experiment

2020 ◽  
Vol 1342 ◽  
pp. 012064
Author(s):  
J. Gascon ◽  
Keyword(s):  
Low Mass ◽  
Author(s):  
Victor Parusov ◽  
Boris Ovchinnikov

Gas electron multipliers (GEMs) with wire (WGEMs) or metal electrodes (MGEMs), which don’t use any plastic insulators between electrodes are created. The chambers containing MGEMs (WGEMs) with pin-anodes are proposed as detectors for searching of spin-dependent interactions between Dark Matter (DM) particles and gases with nonzero-spin nuclei (H2, D2, 3He, 21Ne, CF4, CH4, etc.). In this paper, we present a review of such chambers. For investigation of the gas mixtures Ne+10%H2, H2 (D2) +3ppmTMAE, the chamber containing WGEM with pin-anode detection system was constructed. In this paper we present the results of an experimental study of these gaseous mixtures exited by an α - source. Mixture of Ar + 40 ppm C2H4 and mixture 50% Xe + 50%CF4 have been investigated. The spatial distributions of photoelectron clouds produced by primary scintillations on α- and β-particle tracks, as well as the distributions of photoelectron clouds due to photons from avalanches at the pin-anode, have been measured for the first time. In our experiments as another filling of the chambers for search of low-mas WIMP (<10 GeV/c2), solar neutrino and solar axions with spin-dependent interaction we propose to use the mixtures: D2 + 3ppmTMAE, 3He + 3%CH4, 21Ne + 10%H2, at pressure 10-17 bar. And in our experiment with liquid gases is used the mixtures with 19F (LAr + CF4, LXe + CF4) and mixture LCH4 + 40ppm TMAE. The time projection chamber (TPC) with the mixture D2 + 3ppmTMAE filling allow to search of spin-dependent interactions of solar axions and deuterium. As well as we present the detecting systems for search of narrow pp-resonances (quarks) in accelerators experiments.


2012 ◽  
Author(s):  
R. Dharmapalan ◽  
S. Habib ◽  
C. Jiang ◽  
I. Stancu ◽  
R.A. Johnson ◽  
...  

2015 ◽  
Vol 650 ◽  
pp. 012005 ◽  
Author(s):  
F J Iguaz ◽  
J G Garza ◽  
F Aznar ◽  
J F Castel ◽  
S Cebrián ◽  
...  

Author(s):  
F. J. Iguaz ◽  
J. G. Garza ◽  
F. Aznar ◽  
J. F. Castel ◽  
S. Cebrián ◽  
...  

2016 ◽  
Vol 718 ◽  
pp. 042048 ◽  
Author(s):  
R Strauss ◽  
G Angloher ◽  
A Bento ◽  
C Bucci ◽  
L Canonica ◽  
...  
Keyword(s):  
Low Mass ◽  

2018 ◽  
Vol 174 ◽  
pp. 01008 ◽  
Author(s):  
J. G. Garza ◽  
S. Aune ◽  
F. Aznar ◽  
J. F. Castel ◽  
S. Cebrián ◽  
...  

The most compelling candidates for Dark Matter to day are WIMPs and axions. The applicability of gasesous Time Projection Chambers (TPCs) with Micromesh Gas Structures (Micromegas) to the search of these particles is explored within this work. Both particles would produce an extremely low rate at very low energies in particle detectors. Micromegas detectors can provide both low background rates and low energy threshold, due to the high granularity, radiopurity and uniformity of the readout. Small (few cm wide) Micromegas detectors are used to image the axion-induced x-ray signal expected in the CERN Axion Solar Telescope (CAST) experiment. We show the background levels obtained in CAST and the prospects to further reduce them to the values required by the Internation Axion Observatory (IAXO). We also present TREX-DM, a scaled-up version of the Micromegas used in axion research, but this time dedicated to the low-mass WIMP detection. TREX-DM is a high-pressure Micromegas-based TPC designed to host a few hundreds of grams of light nuclei (argon or neon) with energy thresholds potentially at the level of 100 eV. The detector is described in detail, as well as the results of the commissioning and characterization phase on surface. Besides, the background model of TREX-DM is presented, along with the anticipated sensitivity of this search, which could go beyond current experimental limits.


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