TY - JOUR AU - NEXT Collaboration (Alvarez, V. et al AU - Carcel, S. AU - Cervera-Villanueva, A. AU - Diaz, J. AU - Ferrario, P. AU - Gil, A. AU - Gomez-Cadenas, J. J. AU - Gonzalez, K. AU - Liubarsky, I. AU - Lorca, D. AU - Martin-Albo, J. AU - Martinez, A. AU - Monrabal, F. AU - Muñoz Vidal, J. AU - Nebot-Guinot, M. AU - Rodriguez, J. AU - Serra, L. AU - Sorel, M. AU - Yahlali, N. PY - 2012 DA - 2012// TI - NEXT-100 Technical Design Report (TDR). Executive summary T2 - J. Instrum. JO - Journal of Instrumentation SP - T06001 - 34pp VL - 7 PB - Iop Publishing Ltd KW - Detector design and construction technologies and materials KW - Time projection chambers AB - In this Technical Design Report (TDR) we describe the NEXT-100 detector that will search for neutrinoless double beta decay (beta beta 0v) in Xe-136 at the Laboratorio Subterraneo de Canfranc (LSC), in Spain. The document formalizes the design presented in our Conceptual Design Report (CDR): an electroluminescence time projection chamber, with separate readout planes for calorimetry and tracking, located, respectively, behind cathode and anode. The detector is designed to hold a maximum of about 150 kg of xenon at 15 bar, or 100 kg at 10 bar. This option builds in the capability to increase the total isotope mass by 50% while keeping the operating pressure at a manageable level. The readout plane performing the energy measurement is composed of Hamamatsu R11410-10 photomultipliers, specially designed for operation in low-background, xenon-based detectors. Each individual PMT will be isolated from the gas by an individual, pressure resistant enclosure and will be coupled to the sensitive volume through a sapphire window. The tracking plane consists in an array of Hamamatsu S10362-11-050P MPPCs used as tracking pixels. They will be arranged in square boards holding 64 sensors (8 x 8) with a 1-cm pitch. The inner walls of the TPC, the sapphire windows and the boards holding the MPPCs will be coated with tetraphenyl butadiene (TPB), a wavelength shifter, to improve the light collection. SN - 1748-0221 UR - http://arxiv.org/abs/arXiv:1202.0721 UR - https://doi.org/10.1088/1748-0221/7/06/T06001 DO - 10.1088/1748-0221/7/06/T06001 LA - English N1 - WOS:000306072000030 ID - NEXTCollaborationAlvarez_etal2012 ER -