The MAJORANA Project

Clicks: 219
ID: 116007
2009
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Abstract
Building a Ovββ experiment with the ability to probe neutrino mass in the inverted hierarchy region requires the combination of a large detector mass sensitive to Ovββ, on the order of 1-tonne, and unprecedented background levels, on the order of or less than 1 count per year in the Ovβ β signal region. The MAJORANA Collaboration proposes a design based on using high-purity enriched 76Ge crystals deployed in ultralow background electroformed Cu cryostats and using modern analysis techniques that should be capable of reaching the required sensitivity while also being scalable to a 1-tonne size. To demonstrate feasibility, the collaboration plans to construct a prototype system, the MAJORANA DEMONSTRATOR, consisting of 30 kg of 86% enriched 76Ge detectors and 30 kg of natural or isotope-76-depleted Ge detectors. We plan to deploy and evaluate two different Ge detector technologies, one based on a p-type configuration and the other on n-type.
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Authors Steven R. Elliott,C E Aalseth,M Akashi-Ronquest,Mark Amman,J F Amsbaugh,F T Avignone,H O Back,C Baktash,A S Barabash,P Barbeau,J R Beene,M Bergevin,F E Bertrand,M Boswell,V Brudanin,W Bugg,T H Burritt,Y-D Chan,T V Cianciolo,J Collar,R Creswick,M Cromaz,J A Detwiler,P J Doe,J A Dunmore,Yu Efremenko,V Egorov,H Ejiri,J Ely,J Esterline,H Farach,T Farmer,J Fast,P Finnerty,B Fujikawa,V M Gehman,C Greenberg,V E Guiseppe,K Gusey,A L Hallin,R Hazama,R Henning,A Hime,Todd W. Hossbach,E Hoppe,M A Howe,D Hurley,B Hyronimus,R A Johnson,Martin E. Keillor,C Keller,J Kephart,M Kidd,O Kochetov,S I Konovalov,R T Kouzes,K T Lesko,L Leviner,P Luke,S MacMullin,Michael Marino,A B McDonald,D-M Mei,H S Miley,A W Myers,M Nomachi,B. C. Odom,J Orrell,A W P Poon,G Prior,D C Radford,J H Reeves,Keith Rielage,Nathan Riley,R G H Robertson,L Rodríguez,K P Rykaczewski,A G Schubert,T Shima,M Shirchenko,V Timkin,R Thompson,W Tornow,C Tull,T D Van Wechel,I Vanyushin,R L Varner,K Vetter,R Warner,John F. Wilkerson,J M Wouters,Evgeny Yakushev,A R Young,C-H Yu,V Yumatov,Z-B Yin;Steven R. Elliott;C E Aalseth;M Akashi-Ronquest;Mark Amman;J F Amsbaugh;F T Avignone;H O Back;C Baktash;A S Barabash;P Barbeau;J R Beene;M Bergevin;F E Bertrand;M Boswell;V Brudanin;W Bugg;T H Burritt;Y-D Chan;T V Cianciolo;J Collar;R Creswick;M Cromaz;J A Detwiler;P J Doe;J A Dunmore;Yu Efremenko;V Egorov;H Ejiri;J Ely;J Esterline;H Farach;T Farmer;J Fast;P Finnerty;B Fujikawa;V M Gehman;C Greenberg;V E Guiseppe;K Gusey;A L Hallin;R Hazama;R Henning;A Hime;Todd W. Hossbach;E Hoppe;M A Howe;D Hurley;B Hyronimus;R A Johnson;Martin E. Keillor;C Keller;J Kephart;M Kidd;O Kochetov;S I Konovalov;R T Kouzes;K T Lesko;L Leviner;P Luke;S MacMullin;Michael Marino;A B McDonald;D-M Mei;H S Miley;A W Myers;M Nomachi;B. C. Odom;J Orrell;A W P Poon;G Prior;D C Radford;J H Reeves;Keith Rielage;Nathan Riley;R G H Robertson;L Rodríguez;K P Rykaczewski;A G Schubert;T Shima;M Shirchenko;V Timkin;R Thompson;W Tornow;C Tull;T D Van Wechel;I Vanyushin;R L Varner;K Vetter;R Warner;John F. Wilkerson;J M Wouters;Evgeny Yakushev;A R Young;C-H Yu;V Yumatov;Z-B Yin;
Journal journal of physics: conference series
Year 2009
DOI
10.1088/1742-6596/173/1/012007
URL
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