TREX-DM: a low-background Micromegas-based TPC for low-mass WIMP detection

• Published in: The European physical journal. C, Particles and fields Vol. 76; no. 10; p. 529
• Main Authors: Iguaz, F. J., Garza, J. G., Aznar, F., Castel, J. F., Cebrián, S., Dafni, T., García, J. A., Irastorza, I. G., Lagraba, A., Luzón, G., Peiró, A.
• Format: Journal Article
• Language: English
• Published: Berlin/Heidelberg Springer Berlin Heidelberg 27.09.2016; Springer; Springer Nature B.V
• Subjects: Astronomy; Astrophysics and Cosmology; Dark matter; Detection equipment; Elementary Particles; Hadrons; Heavy Ions; Measurement Science and Instrumentation; Nuclear Energy; Nuclear Physics; Physics; Physics and Astronomy; Quantum Field Theories; Quantum Field Theory; Regular - Experimental Physics; Regular Article - Experimental Physics; String Theory; Nuclear Recoil; Glow Discharge Mass Spectrometry; Weakly Interact Massive Particle; Energy Threshold; Field Cage
• ISSN: 1434-6044; 1434-6052
• DOI: 10.1140/epjc/s10052-016-4372-6

If Dark Matter is made of Weakly Interacting Massive Particles (WIMPs) with masses below ∼ 20 GeV, the corresponding nuclear recoils in mainstream WIMP experiments are of energies too close, or below, the experimental threshold. Gas Time Projection Chambers (TPCs) can be operated with a variety of target elements, offer good tracking capabilities and, on account of the amplification in gas, very low thresholds are achievable. Recent advances in electronics and in novel radiopure TPC readouts, especially micro-mesh gas structure (Micromegas), are improving the scalability and low-background prospects of gaseous TPCs. Here we present TREX-DM, a prototype to test the concept of a Micromegas-based TPC to search for low-mass WIMPs. The detector is designed to host an active mass of ∼ 0.300  kg of Ar at 10 bar, or alternatively ∼ 0.160 kg of Ne at 10 bar, with an energy threshold below 0.4 keVee, and is fully built with radiopure materials. We will describe the detector in detail, the results from the commissioning phase on surface, as well as a preliminary background model. The anticipated sensitivity of this technique may go beyond current experimental limits for WIMPs of masses of 2–8 GeV.