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Detector

In order for NEXT to be competitive with the new generation of ββ0ν experiments already in operation or in construction, we need a detector with very good energy resolution (< 1%), very low background contamination (~ 10^-4 counts/(keV kg y)) and large target mass. In addition, it needs to be operational as soon as possible.

The NEXT design optimizes energy resolution thanks to the use of proportional electroluminescent ampli fication (EL), which provides a large yield of photons as a signal; it is compact, as the Xe gas is under high pressure; and it allows the measurement of the topological signature of the event to further reduce the background contamination: the two electrons of 0νββ leave a track with almost constant energy deposition and two big “blobs” of energy at the ends, caused by the higher energy deposition per unit length that the electrons leaves when they have low energy left. On the contrary, background is constituted by single electrons, which present only one  “blob” at one end.

The SOFT (Separated Optimized FuncTion) design takes advantage of di fferent sensors for tracking and calorimetry. On the tracking side, we'll make use of SiPMs coated with a suitable wavelength shifter, while radiopure photomultipliers will be installed for the measurement of the energy and the primary scintillation needed to estimate the t0.

In the figure an asymmetric SOFT TPC is illustrated. An event, shown as a wiggly track, generates primary scintillation recorded at both planes (this is called the S1 signal, following the slang used by the experiments searching for direct detection of Dark Matter). EL light generated at the anode (S2) is recorded in the SiPMs plane right behind it and used for tracking. It is also recorded in the photosensor plane behind the transparent cathode and used for a precise energy measurement.

From 2009 to today an intense R&D program has been carried out by the Collaboration. The feasibility of the technology has been demonstrated with the NEXT prototypes which have shown the excellent performance (energy resolution, electron reconstruction) of the apparatus, as well as the robustness of the EL technology. The LSC Scientific Committee has recommended that a first-phase of the NEXT detector, deploying 20 % of the sensors of the final apparatus is installed and operated at the Underground Canfranc Laboratory (LSC), with the double target of assessing the NEXT background model from the data themselves, and measuring the mode with two neutrinos double beta decay, which will allow a clear demonstration of the unique NEXT topological signal. As a consequence, the collaboration has decided to deploy a first stage of the NEXT detector, the NEW (NEXT-WHITE) apparatus (the name honours the memory of Professor James White, recently deceased and one of the key scientists of the NEXT Collaboration).

 

 

Institutions

 

Co-spokespersons

Juan José Gómez Cadenas: Juan.Jose.Gomez.Cadenas@ific.uv.es

Dave Nygren: nygren@uta.edu

Links

  • Report from LSC - May 2016

  • Report from LSC - Nov 2015

  • Report from LSC - Nov 2014

  • Report to the Nuclear Science Advisory Committee - May 2014

  • Report from Consolider - CUP

  • arXiv:1202.0721v1 [physics.ins-det] - Technical Design Report

  • arXiv:1106.3630v1 [physics.ins-det] - Conceptual Design Report

  • arXiv:0907.4054 [hep-ex] - Letter of Intent to LSC

  • Laboratorio Subterráneo de Canfranc (LSC)

     

    Starting from March 2013, NEXT is a Recognized Experiment at CERN!