CUPID: The Next-Generation Neutrinoless Double Beta Decay Experiment

CUPID: The Next-Generation Neutrinoless Double Beta Decay Experiment
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DOI:
10.1007/s10909-022-02909-3
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发表时间:
2022-11
影响因子:
2
通讯作者:
K. Alfonso;A. Armatol;C. Augier;F. Avignone;O. Azzolini;M. Balata;A. Barabash;G. Bari;A. Barresi;D. Baudin;F. Bellini;G. Benato;M. Beretta;M. Bettelli;M. Biassoni;J. Billard;V. Boldrini;A. Branca;C. Brofferio;C. Bucci;J. Camilleri;A. Campani;C. Capelli;S. Capelli;L. Cappelli;L. Cardani;P. Carniti;N. Casali;E. Celi;C. Chang;D. Chiesa;M. Clemenza;I. Colantoni;S. Copello;E. Craft;O. Cremonesi;R. Creswick;A. Cruciani;A. D’Addabbo;G. D’Imperio;S. Dabagov;I. Dafinei;F. Danevich;M. de Jesus;P. de Marcillac;S. Dell’Oro;S. Domizio;S. Lorenzo;T. Dixon;V. Dompè;A. Drobizhev;L. Dumoulin;G. Fantini;M. Faverzani;E. Ferri;F. Ferri;F. Ferroni;E. Figueroa-Feliciano;L. Foggetta;J. Formaggio;A. Franceschi;C. Fu;S. Fu;B. Fujikawa;A. Gallas;J. Gascon;S. Ghislandi;Andrea Giachero;A. Gianvecchio;L. Gironi;A. Giuliani;P. Gorla;C. Gotti;C. Grant;P. Gras;P. Guillaumon;T. Gutierrez;K. Han;E. Hansen;K. Heeger;D. Helis;H. Huang;L. Imbert;J. Johnston;A. Juillard;G. Karapetrov;G. Keppel;H. Khalife;V. Kobychev;Y. Kolomensky;S. Konovalov;R. Kowalski;T. Langford;M. Lefevre;R. Liu;Y. Liu;P. Loaiza;L. Ma;M. Madhukuttan;F. Mancarella;L. Marini;S. Marnieros;M. Martinez;R. Maruyama;P. Mas;B. Mauri;D. Mayer;G. Mazzitelli;Y. Mei;S. Milana;S. Morganti;T. Napolitano;M. Nastasi;J. Nikkel;S. Nisi;C. Nones;E. Norman;V. Novosad;I. Nutini;T. O’Donnell;E. Olivieri;M. Olmi;J. Ouellet;S. Pagan;C. Pagliarone;L. Pagnanini;L. Pattavina;M. Pavan;H. Peng;G. Pessina;V. Pettinacci;C. Pira;S. Pirrò;D. Poda;O. Polischuk;I. Ponce;S. Pozzi;E. Previtali;A. Puiu;S. Quitadamo;A. Ressa;R. Rizzoli;C. Rosenfeld;P. Rosier;J. Scarpaci;B. Schmidt;V. Sharma;V. Shlegel;V. Singh;M. Sisti;P. Slocum;D. Speller;P. T. Surukuchi;L. Taffarello;C. Tomei;J. A. Torres;V. Tretyak;A. Tsymbaliuk;M. Velázquez;K. Vetter;S. Wagaarachchi;G. Wang;Lung-Chuang Wang;R. Wang;B. Welliver;J. Wilson;K. Wilson;L. Winslow;M. Xue;L. Yan;J. Yang;V. Yefremenko;V. Umatov;M. Zarytskyy;J. Zhang;A. Zolotarova;S. Zucchelli
K. Alfonso;A. Armatol;C. Augier;F. Avignone;O. Azzolini;M. Balata;A. Barabash;G. Bari;A. Barresi;D. Baudin;F. Bellini;G. Benato;M. Beretta;M. Bettelli;M. Biassoni;J. Billard;V. Boldrini;A. Branca;C. Brofferio;C. Bucci;J. Camilleri;A. Campani;C. Capelli;S. Capelli;L. Cappelli;L. Cardani;P. Carniti;N. Casali;E. Celi;C. Chang;D. Chiesa;M. Clemenza;I. Colantoni;S. Copello;E. Craft;O. Cremonesi;R. Creswick;A. Cruciani;A. D’Addabbo;G. D’Imperio;S. Dabagov;I. Dafinei;F. Danevich;M. de Jesus;P. de Marcillac;S. Dell’Oro;S. Domizio;S. Lorenzo;T. Dixon;V. Dompè;A. Drobizhev;L. Dumoulin;G. Fantini;M. Faverzani;E. Ferri;F. Ferri;F. Ferroni;E. Figueroa-Feliciano;L. Foggetta;J. Formaggio;A. Franceschi;C. Fu;S. Fu;B. Fujikawa;A. Gallas;J. Gascon;S. Ghislandi;Andrea Giachero;A. Gianvecchio;L. Gironi;A. Giuliani;P. Gorla;C. Gotti;C. Grant;P. Gras;P. Guillaumon;T. Gutierrez;K. Han;E. Hansen;K. Heeger;D. Helis;H. Huang;L. Imbert;J. Johnston;A. Juillard;G. Karapetrov;G. Keppel;H. Khalife;V. Kobychev;Y. Kolomensky;S. Konovalov;R. Kowalski;T. Langford;M. Lefevre;R. Liu;Y. Liu;P. Loaiza;L. Ma;M. Madhukuttan;F. Mancarella;L. Marini;S. Marnieros;M. Martinez;R. Maruyama;P. Mas;B. Mauri;D. Mayer;G. Mazzitelli;Y. Mei;S. Milana;S. Morganti;T. Napolitano;M. Nastasi;J. Nikkel;S. Nisi;C. Nones;E. Norman;V. Novosad;I. Nutini;T. O’Donnell;E. Olivieri;M. Olmi;J. Ouellet;S. Pagan;C. Pagliarone;L. Pagnanini;L. Pattavina;M. Pavan;H. Peng;G. Pessina;V. Pettinacci;C. Pira;S. Pirrò;D. Poda;O. Polischuk;I. Ponce;S. Pozzi;E. Previtali;A. Puiu;S. Quitadamo;A. Ressa;R. Rizzoli;C. Rosenfeld;P. Rosier;J. Scarpaci;B. Schmidt;V. Sharma;V. Shlegel;V. Singh;M. Sisti;P. Slocum;D. Speller;P. T. Surukuchi;L. Taffarello;C. Tomei;J. A. Torres;V. Tretyak;A. Tsymbaliuk;M. Velázquez;K. Vetter;S. Wagaarachchi;G. Wang;Lung-Chuang Wang;R. Wang;B. Welliver;J. Wilson;K. Wilson;L. Winslow;M. Xue;L. Yan;J. Yang;V. Yefremenko;V. Umatov;M. Zarytskyy;J. Zhang;A. Zolotarova;S. Zucchelli
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
K. Alfonso;A. Armatol;C. Augier;F. Avignone;O. Azzolini;M. Balata;A. Barabash;G. Bari;A. Barresi;D. Baudin;F. Bellini;G. Benato;M. Beretta;M. Bettelli;M. Biassoni;J. Billard;V. Boldrini;A. Branca;C. Brofferio;C. Bucci;J. Camilleri;A. Campani;C. Capelli;S. Capelli;L. Cappelli;L. Cardani;P. Carniti;N. Casali;E. Celi;C. Chang;D. Chiesa;M. Clemenza;I. Colantoni;S. Copello;E. Craft;O. Cremonesi;R. Creswick;A. Cruciani;A. D’Addabbo;G. D’Imperio;S. Dabagov;I. Dafinei;F. Danevich;M. de Jesus;P. de Marcillac;S. Dell’Oro;S. Domizio;S. Lorenzo;T. Dixon;V. Dompè;A. Drobizhev;L. Dumoulin;G. Fantini;M. Faverzani;E. Ferri;F. Ferri;F. Ferroni;E. Figueroa-Feliciano;L. Foggetta;J. Formaggio;A. Franceschi;C. Fu;S. Fu;B. Fujikawa;A. Gallas;J. Gascon;S. Ghislandi;Andrea Giachero;A. Gianvecchio;L. Gironi;A. Giuliani;P. Gorla;C. Gotti;C. Grant;P. Gras;P. Guillaumon;T. Gutierrez;K. Han;E. Hansen;K. Heeger;D. Helis;H. Huang;L. Imbert;J. Johnston;A. Juillard;G. Karapetrov;G. Keppel;H. Khalife;V. Kobychev;Y. Kolomensky;S. Konovalov;R. Kowalski;T. Langford;M. Lefevre;R. Liu;Y. Liu;P. Loaiza;L. Ma;M. Madhukuttan;F. Mancarella;L. Marini;S. Marnieros;M. Martinez;R. Maruyama;P. Mas;B. Mauri;D. Mayer;G. Mazzitelli;Y. Mei;S. Milana;S. Morganti;T. Napolitano;M. Nastasi;J. Nikkel;S. Nisi;C. Nones;E. Norman;V. Novosad;I. Nutini;T. O’Donnell;E. Olivieri;M. Olmi;J. Ouellet;S. Pagan;C. Pagliarone;L. Pagnanini;L. Pattavina;M. Pavan;H. Peng;G. Pessina;V. Pettinacci;C. Pira;S. Pirrò;D. Poda;O. Polischuk;I. Ponce;S. Pozzi;E. Previtali;A. Puiu;S. Quitadamo;A. Ressa;R. Rizzoli;C. Rosenfeld;P. Rosier;J. Scarpaci;B. Schmidt;V. Sharma;V. Shlegel;V. Singh;M. Sisti;P. Slocum;D. Speller;P. T. Surukuchi;L. Taffarello;C. Tomei;J. A. Torres;V. Tretyak;A. Tsymbaliuk;M. Velázquez;K. Vetter;S. Wagaarachchi;G. Wang;Lung-Chuang Wang;R. Wang;B. Welliver;J. Wilson;K. Wilson;L. Winslow;M. Xue;L. Yan;J. Yang;V. Yefremenko;V. Umatov;M. Zarytskyy;J. Zhang;A. Zolotarova;S. Zucchelli

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丘比特是下一代吨尺度的无中微子双β衰变实验,它将探测中微子的马约拉纳性质,并在观察这一奇异过程的情况下发现轻子数违反。丘比特将以CUORE的经验、专门知识和教训为基础,并将安装在格兰萨索地下实验室目前的CUORE基础设施中。在丘比特-钼实验中成功测试的丘比特探测器技术,是基于富集感兴趣的同位素mo的limoo闪烁辐射热计。为了实现其雄心勃勃的科学目标,丘比特合作旨在将感兴趣地区的背景减少100倍。这一性能将通过引入cuvid -0和cuvid - mo实验所证明的高效/分辨,以及使用高跃迁能的双β衰变核(如mo)来最小化伽马背景的影响来实现。丘比特将由大约1500个混合热光探测器组成,总同位素质量为250千克。丘比特的科学范围得到了基于CUORE,丘比特- mo和丘比特-0结果的详细和安全的背景模型的支持。所需的表演已经展示,并将呈现。
CUPID is a next-generation tonne-scale bolometric neutrinoless double beta decay experiment that will probe the Majorana nature of neutrinos and discover lepton number violation in case of observation of this singular process. CUPID will be built on experience, expertise and lessons learned in CUORE and will be installed in the current CUORE infra-structure in the Gran Sasso underground laboratory. The CUPID detector technology, successfully tested in the CUPID-Mo experiment, is based on scintillating bolometers of LiMoOenriched in the isotope of interestMo. In order to achieve its ambitious science goals, the CUPID collaboration aims to reduce the backgrounds in the region of interest by a factor 100 with respect to CUORE. This performance will be achieved by introducing the high efficient/discrimination demonstrated by the CUPID-0 and CUPID-Mo experiments, and using a high transition energy double beta decay nucleus such asMo to minimize the impact of the gamma background. CUPID will consist of about 1500 hybrid heat-light detectors for a total isotope mass of 250 kg. The CUPID scientific reach is supported by a detailed and safe background model based on CUORE, CUPID-Mo and CUPID-0 results. The required performances have already been demonstrated and will be presented.