학술논문

CUORE sensitivity to $$0\nu \beta \beta $$ 0 ν β β decay
Document Type
article
Author
C. AlduinoK. AlfonsoD. R. ArtusaF. T. AvignoneO. AzzoliniT. I. BanksG. BariJ. W. BeemanF. BelliniG. BenatoA. BersaniM. BiassoniA. BrancaC. BrofferioC. BucciA. CamachoA. CaminataL. CanonicaX. G. CaoS. CapelliL. CappelliL. CarboneL. CardaniP. CarnitiN. CasaliL. CassinaD. ChiesaN. ChottM. ClemenzaS. CopelloC. CosmelliO. CremonesiR. J. CreswickJ. S. CushmanA. D’AddabboI. DafineiC. J. DavisS. Dell’OroM. M. DeninnoS. Di DomizioM. L. Di VacriA. DrobizhevD. Q. FangM. FaverzaniG. FernandesE. FerriF. FerroniE. FioriniM. A. FranceschiS. J. FreedmanB. K. FujikawaA. GiacheroL. GironiA. GiulianiL. GladstoneP. GorlaC. GottiT. D. GutierrezE. E. HallerK. HanE. HansenK. M. HeegerR. Hennings-YeomansK. P. HickersonH. Z. HuangR. KadelG. KeppelYu. G. KolomenskyA. LederC. LigiK. E. LimY. G. MaM. MainoL. MariniM. MartinezR. H. MaruyamaY. MeiN. MoggiS. MorgantiP. J. MosteiroT. NapolitanoM. NastasiC. NonesE. B. NormanV. NovatiA. NucciottiT. O’DonnellJ. L. OuelletC. E. PagliaroneM. PallaviciniV. PalmieriL. PattavinaM. PavanG. PessinaV. PettinacciG. PipernoC. PiraS. PirroS. PozziE. PrevitaliC. RosenfeldC. RusconiM. SakaiS. SangiorgioD. SantoneB. SchmidtJ. SchmidtN. D. ScielzoV. SinghM. SistiA. R. SmithL. TaffarelloM. TenconiF. TerranovaC. TomeiS. TrentalangeM. VignatiS. L. WagaarachchiB. S. WangH. W. WangB. WelliverJ. WilsonL. A. WinslowT. WiseA. WoodcraftL. ZanottiG. Q. ZhangB. X. ZhuS. ZimmermannS. Zucchelli
Source
European Physical Journal C: Particles and Fields, Vol 77, Iss 8, Pp 1-10 (2017)
Subject
Astrophysics
QB460-466
Nuclear and particle physics. Atomic energy. Radioactivity
QC770-798
Language
English
ISSN
1434-6044
1434-6052
Abstract
Abstract We report a study of the CUORE sensitivity to neutrinoless double beta ( $$0\nu \beta \beta $$ 0 ν β β ) decay. We used a Bayesian analysis based on a toy Monte Carlo (MC) approach to extract the exclusion sensitivity to the $$0\nu \beta \beta $$ 0 ν β β decay half-life ( $$T_{1/2}^{\,0\nu }$$ T 1 / 2 0 ν ) at $$90\%$$ 90 % credibility interval (CI) – i.e. the interval containing the true value of $$T_{1/2}^{\,0\nu }$$ T 1 / 2 0 ν with $$90\%$$ 90 % probability – and the $$3~\sigma $$ 3 σ discovery sensitivity. We consider various background levels and energy resolutions, and describe the influence of the data division in subsets with different background levels. If the background level and the energy resolution meet the expectation, CUORE will reach a $$90\%$$ 90 % CI exclusion sensitivity of $$2\cdot 10^{25}$$ 2 · 10 25 year with 3 months, and $$9\cdot 10^{25}$$ 9 · 10 25 year with 5 years of live time. Under the same conditions, the discovery sensitivity after 3 months and 5 years will be $$7\cdot 10^{24}$$ 7 · 10 24 year and $$4\cdot 10^{25}$$ 4 · 10 25 year, respectively.