English

The NEXT experiment. Towards phase I

Instrumentation and Detectors 2017-08-23 v2

Abstract

Phase I of the NEXT-100 0νββ0\nu\beta\beta experiment (NEW) is scheduled for data taking in 2015 at Laboratorio Subterr\'aneo de Canfranc in the Spanish Pyrenees. Thanks to the light proportional technique, NEW anticipates an outstanding energy resolution nearing the Fano factor in Xenon (0.5-1%FWHM@Qββ,136XeQ_{\beta\beta,^{136}Xe}), with a TPC-design that allows tracking and identification of the double end-blob feature of the 0νββ0\nu\beta\beta decay. When properly mastered, the combination of these two assets can suppress the irreducible 2νββ2\nu\beta\beta and (single-blob) γ\gamma backgrounds from natural radioactivity to minute levels, of the order of 5×1045\times{10^{-4}} ckky. Given our knowledge of the available phase-space as obtained from neutrino oscillation experiments, this feat will expectedly allow for a sensitivity to the effective electron neutrino mass of mββ30m_{\beta\beta}\simeq 30 meV for exposures at the 20 ton ×\times year scale. Hence, ultimately, a full survey of the inverse hierarchy of the neutrino mass ordering appears to be within reach for a ton-scale experiment based on this technology. NEW, with 10 kg of Xenon 90%-enriched in 136^{136}Xe, sets an unprecedented scale for gaseous Xenon TPCs and will be an important milestone for its anticipated upgrades (100 kg and 1 ton). I briefly summarize the status of the NEXT experiment, from the main results obtained with 1\sim 1 kg prototypes that substantiate the concept, to the ongoing works for deploying its first phase.

Keywords

Cite

@article{arxiv.1310.7054,
  title  = {The NEXT experiment. Towards phase I},
  author = {D. Gonzalez-Diaz and the NEXT collaboration},
  journal= {arXiv preprint arXiv:1310.7054},
  year   = {2017}
}

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contribution to ICATPP 2013

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