Projected background and sensitivity of AMoRE-II
Abstract AMoRE-II aims to search for neutrinoless double beta decay ( $$0\nu \beta \beta $$ 0 ν β β ) with an array of 423 $$\hbox {Li}_2^{100}\hbox {MoO}_4$$ Li 2 100 MoO 4 crystals operating in the cryogenic system as the main phase of the Advanced Molybdenum-based Rare process Experiment (AMoRE)....
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2025-01-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | https://doi.org/10.1140/epjc/s10052-024-13516-9 |
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| author | A. Agrawal V. V. Alenkov P. Aryal J. Beyer B. Bhandari R. S. Boiko K. Boonin O. Buzanov C. R. Byeon N. Chanthima M. K. Cheoun J. S. Choe Seonho Choi S. Choudhury J. S. Chung F. A. Danevich M. Djamal D. Drung C. Enss A. Fleischmann A. M. Gangapshev L. Gastaldo Y. M. Gavrilyuk A. M. Gezhaev O. Gileva V. D. Grigorieva V. I. Gurentsov C. Ha D. H. Ha E. J. Ha D. H. Hwnag E. J. Jeon J. A. Jeon H. S. Jo J. Kaewkhao C. S. Kang W. G. Kang V. V. Kazalov S. Kempf A. Khan S. Khan D. Y. Kim G. W. Kim H. B. Kim Ho-Jong Kim H. J. Kim H. L. Kim H. S. Kim M. B. Kim S. C. Kim S. K. Kim S. R. Kim W. T. Kim Y. D. Kim Y. H. Kim K. Kirdsiri Y. J. Ko V. V. Kobychev V. Kornoukhov V. V. Kuzminov D. H. Kwon C. H. Lee DongYeup Lee E. K. Lee H. J. Lee H. S. Lee J. Lee J. Y. Lee K. B. Lee M. H. Lee M. K. Lee S. W. Lee Y. C. Lee D. S. Leonard H. S. Lim B. Mailyan E. P. Makarov P. Nyanda Y. Oh S. L. Olsen S. I. Panasenko H. K. Park H. S. Park K. S. Park S. Y. Park O. G. Polischuk H. Prihtiadi S. Ra S. S. Ratkevich G. Rooh E. Sala M. B. Sari J. Seo K. M. Seo B. Sharma K. A. Shin V. N. Shlegel K. Siyeon J. So N. V. Sokur J. K. Son J. W. Song N. Srisittipokakun V. I. Tretyak R. Wirawan K. R. Woo H. J. Yeon Y. S. Yoon Q. Yue The AMoRE Collaboration |
| author_facet | A. Agrawal V. V. Alenkov P. Aryal J. Beyer B. Bhandari R. S. Boiko K. Boonin O. Buzanov C. R. Byeon N. Chanthima M. K. Cheoun J. S. Choe Seonho Choi S. Choudhury J. S. Chung F. A. Danevich M. Djamal D. Drung C. Enss A. Fleischmann A. M. Gangapshev L. Gastaldo Y. M. Gavrilyuk A. M. Gezhaev O. Gileva V. D. Grigorieva V. I. Gurentsov C. Ha D. H. Ha E. J. Ha D. H. Hwnag E. J. Jeon J. A. Jeon H. S. Jo J. Kaewkhao C. S. Kang W. G. Kang V. V. Kazalov S. Kempf A. Khan S. Khan D. Y. Kim G. W. Kim H. B. Kim Ho-Jong Kim H. J. Kim H. L. Kim H. S. Kim M. B. Kim S. C. Kim S. K. Kim S. R. Kim W. T. Kim Y. D. Kim Y. H. Kim K. Kirdsiri Y. J. Ko V. V. Kobychev V. Kornoukhov V. V. Kuzminov D. H. Kwon C. H. Lee DongYeup Lee E. K. Lee H. J. Lee H. S. Lee J. Lee J. Y. Lee K. B. Lee M. H. Lee M. K. Lee S. W. Lee Y. C. Lee D. S. Leonard H. S. Lim B. Mailyan E. P. Makarov P. Nyanda Y. Oh S. L. Olsen S. I. Panasenko H. K. Park H. S. Park K. S. Park S. Y. Park O. G. Polischuk H. Prihtiadi S. Ra S. S. Ratkevich G. Rooh E. Sala M. B. Sari J. Seo K. M. Seo B. Sharma K. A. Shin V. N. Shlegel K. Siyeon J. So N. V. Sokur J. K. Son J. W. Song N. Srisittipokakun V. I. Tretyak R. Wirawan K. R. Woo H. J. Yeon Y. S. Yoon Q. Yue The AMoRE Collaboration |
| author_sort | A. Agrawal |
| collection | DOAJ |
| description | Abstract AMoRE-II aims to search for neutrinoless double beta decay ( $$0\nu \beta \beta $$ 0 ν β β ) with an array of 423 $$\hbox {Li}_2^{100}\hbox {MoO}_4$$ Li 2 100 MoO 4 crystals operating in the cryogenic system as the main phase of the Advanced Molybdenum-based Rare process Experiment (AMoRE). AMoRE has been planned to operate in three phases: AMoRE-pilot, AMoRE-I, and AMoRE-II. AMoRE-II is currently being installed at the Yemi Underground Laboratory, located approximately 1000 m deep in Jeongseon, Korea. The goal of the experiment is to reach an exclusion half-life sensitivity to the $$0\nu \beta \beta $$ 0 ν β β of $$^{100}$$ 100 Mo on the level of $$T^{0\nu \beta \beta }_{1/2} > 6 \times 10^{26}$$ T 1 / 2 0 ν β β > 6 × 10 26 year that covers completely the inverted Majorana neutrino mass hierarchy region of (15–46) meV. To achieve this, the background level of the experimental configurations and possible background sources of gamma and beta events should be well understood. We have intensively performed Monte Carlo simulations using the GEANT4 toolkit in all the experimental configurations with potential sources. We report the estimated background level that meets the $$10^{-4}$$ 10 - 4 counts/(keV $$\cdot $$ · kg $$\cdot $$ · year) requirement for AMoRE-II in the Region Of Interest (ROI) and show the projected half-life sensitivity based on the simulation study. |
| format | Article |
| id | doaj-art-763e546ead37430fbfdb60abf952fc31 |
| institution | Kabale University |
| issn | 1434-6052 |
| language | English |
| publishDate | 2025-01-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | European Physical Journal C: Particles and Fields |
| spelling | doaj-art-763e546ead37430fbfdb60abf952fc312025-01-12T12:36:51ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-01-0185111410.1140/epjc/s10052-024-13516-9Projected background and sensitivity of AMoRE-IIA. Agrawal0V. V. Alenkov1P. Aryal2J. Beyer3B. Bhandari4R. S. Boiko5K. Boonin6O. Buzanov7C. R. Byeon8N. Chanthima9M. K. Cheoun10J. S. Choe11Seonho Choi12S. Choudhury13J. S. Chung14F. A. Danevich15M. Djamal16D. Drung17C. Enss18A. Fleischmann19A. M. Gangapshev20L. Gastaldo21Y. M. Gavrilyuk22A. M. Gezhaev23O. Gileva24V. D. Grigorieva25V. I. Gurentsov26C. Ha27D. H. Ha28E. J. Ha29D. H. Hwnag30E. J. Jeon31J. A. Jeon32H. S. Jo33J. Kaewkhao34C. S. Kang35W. G. Kang36V. V. Kazalov37S. Kempf38A. Khan39S. Khan40D. Y. Kim41G. W. Kim42H. B. Kim43Ho-Jong Kim44H. J. Kim45H. L. Kim46H. S. Kim47M. B. Kim48S. C. Kim49S. K. Kim50S. R. Kim51W. T. Kim52Y. D. Kim53Y. H. Kim54K. Kirdsiri55Y. J. Ko56V. V. Kobychev57V. Kornoukhov58V. V. Kuzminov59D. H. Kwon60C. H. Lee61DongYeup Lee62E. K. Lee63H. J. Lee64H. S. Lee65J. Lee66J. Y. Lee67K. B. Lee68M. H. Lee69M. K. Lee70S. W. Lee71Y. C. Lee72D. S. Leonard73H. S. Lim74B. Mailyan75E. P. Makarov76P. Nyanda77Y. Oh78S. L. Olsen79S. I. Panasenko80H. K. Park81H. S. Park82K. S. Park83S. Y. Park84O. G. Polischuk85H. Prihtiadi86S. Ra87S. S. Ratkevich88G. Rooh89E. Sala90M. B. Sari91J. Seo92K. M. Seo93B. Sharma94K. A. Shin95V. N. Shlegel96K. Siyeon97J. So98N. V. Sokur99J. K. Son100J. W. Song101N. Srisittipokakun102V. I. Tretyak103R. Wirawan104K. R. Woo105H. J. Yeon106Y. S. Yoon107Q. Yue108The AMoRE CollaborationIndian Institute of ScienceJSC FOMOS-MaterialsDepartment of Physics, Kyungpook National UniversityPhysikalisch-Technische BundesanstaltDepartment of Physics and Astronomy, Sejong UniversityInstitute for Nuclear Research of NASUNakhon Pathom Rajabhat UniversityJSC FOMOS-MaterialsDepartment of Physics, Kyungpook National UniversityNakhon Pathom Rajabhat UniversityDepartment of Physics, Soongsil UniversityCenter for Underground Physics, Institute for Basic Science (IBS)Department of Physics and Astronomy, Seoul National UniversityIndian Institute of ScienceDepartment of Physics, Chung-Ang UniversityInstitute for Nuclear Research of NASUDepartment of Physics, Institut TeknologiPhysikalisch-Technische BundesanstaltKirchhoff-Institute for PhysicsKirchhoff-Institute for PhysicsNeutrino Observatory of INR RASKirchhoff-Institute for PhysicsNeutrino Observatory of INR RASNeutrino Observatory of INR RASCenter for Underground Physics, Institute for Basic Science (IBS)Nikolaev Institute of Inorganic Chemistry, Siberian Branch of Russian Academy of ScienceNeutrino Observatory of INR RASDepartment of Physics, Chung-Ang UniversityDepartment of Physics, Kyungpook National UniversityDepartment of Physics, Soongsil UniversityCenter for Underground Physics, Institute for Basic Science (IBS)University of Science and Technology (UST)Center for Underground Physics, Institute for Basic Science (IBS)Department of Physics, Kyungpook National UniversityNakhon Pathom Rajabhat UniversityCenter for Underground Physics, Institute for Basic Science (IBS)Center for Underground Physics, Institute for Basic Science (IBS)Neutrino Observatory of INR RASInstitute of Micro- and Nanoelectronic Systems (IMS), Karlsruhe Institute of Technology (KIT)Department of Physics, Kyungpook National UniversityDepartment of Physics, Kohat University of Science and TechnologyCenter for Underground Physics, Institute for Basic Science (IBS)Center for Underground Physics, Institute for Basic Science (IBS)Department of Physics and Astronomy, Seoul National UniversityCenter for Underground Physics, Institute for Basic Science (IBS)Department of Physics, Kyungpook National UniversityDepartment of Physics, Kyungpook National UniversityDepartment of Physics and Astronomy, Sejong UniversityCenter for Underground Physics, Institute for Basic Science (IBS)Center for Underground Physics, Institute for Basic Science (IBS)Department of Physics and Astronomy, Seoul National UniversityCenter for Underground Physics, Institute for Basic Science (IBS)University of Science and Technology (UST)University of Science and Technology (UST)University of Science and Technology (UST)Nakhon Pathom Rajabhat UniversityCenter for Underground Physics, Institute for Basic Science (IBS)Institute for Nuclear Research of NASUNational Research Nuclear University MEPhINeutrino Observatory of INR RASUniversity of Science and Technology (UST)Center for Underground Physics, Institute for Basic Science (IBS)Department of Accelerator ScienceCenter for Underground Physics, Institute for Basic Science (IBS)Center for Underground Physics, Institute for Basic Science (IBS)University of Science and Technology (UST)Center for Underground Physics, Institute for Basic Science (IBS)Department of Physics, Kyungpook National UniversityKorea Research Institute of Standards and ScienceUniversity of Science and Technology (UST)Korea Research Institute of Standards and ScienceDepartment of Physics, Kyungpook National UniversityDepartment of Physics and Astronomy, Seoul National UniversityCenter for Underground Physics, Institute for Basic Science (IBS)Department of Physics, Kyungpook National UniversityFlorida Institute of TechnologyNikolaev Institute of Inorganic Chemistry, Siberian Branch of Russian Academy of ScienceUniversity of Science and Technology (UST)Center for Underground Physics, Institute for Basic Science (IBS)Center for Underground Physics, Institute for Basic Science (IBS)Neutrino Observatory of INR RASDepartment of Accelerator ScienceKorea Research Institute of Standards and ScienceCenter for Underground Physics, Institute for Basic Science (IBS)Center for Underground Physics, Institute for Basic Science (IBS)Institute for Nuclear Research of NASUDepartment of Physics, Universitas Negeri MalangCenter for Underground Physics, Institute for Basic Science (IBS)Neutrino Observatory of INR RASDepartment of Physics, Abdul Wali Khan UniversityCenter for Underground Physics, Institute for Basic Science (IBS)Department of Physics, Institut TeknologiUniversity of Science and Technology (UST)Department of Physics and Astronomy, Sejong UniversityUniversity of Science and Technology (UST)Center for Underground Physics, Institute for Basic Science (IBS)Nikolaev Institute of Inorganic Chemistry, Siberian Branch of Russian Academy of ScienceDepartment of Physics, Chung-Ang UniversityCenter for Underground Physics, Institute for Basic Science (IBS)Institute for Nuclear Research of NASUCenter for Underground Physics, Institute for Basic Science (IBS)Nakhon Pathom Rajabhat UniversityNakhon Pathom Rajabhat UniversityInstitute for Nuclear Research of NASUDepartment of Physics, University of MataramCenter for Underground Physics, Institute for Basic Science (IBS)Center for Underground Physics, Institute for Basic Science (IBS)Korea Research Institute of Standards and ScienceTsinghua UniversityAbstract AMoRE-II aims to search for neutrinoless double beta decay ( $$0\nu \beta \beta $$ 0 ν β β ) with an array of 423 $$\hbox {Li}_2^{100}\hbox {MoO}_4$$ Li 2 100 MoO 4 crystals operating in the cryogenic system as the main phase of the Advanced Molybdenum-based Rare process Experiment (AMoRE). AMoRE has been planned to operate in three phases: AMoRE-pilot, AMoRE-I, and AMoRE-II. AMoRE-II is currently being installed at the Yemi Underground Laboratory, located approximately 1000 m deep in Jeongseon, Korea. The goal of the experiment is to reach an exclusion half-life sensitivity to the $$0\nu \beta \beta $$ 0 ν β β of $$^{100}$$ 100 Mo on the level of $$T^{0\nu \beta \beta }_{1/2} > 6 \times 10^{26}$$ T 1 / 2 0 ν β β > 6 × 10 26 year that covers completely the inverted Majorana neutrino mass hierarchy region of (15–46) meV. To achieve this, the background level of the experimental configurations and possible background sources of gamma and beta events should be well understood. We have intensively performed Monte Carlo simulations using the GEANT4 toolkit in all the experimental configurations with potential sources. We report the estimated background level that meets the $$10^{-4}$$ 10 - 4 counts/(keV $$\cdot $$ · kg $$\cdot $$ · year) requirement for AMoRE-II in the Region Of Interest (ROI) and show the projected half-life sensitivity based on the simulation study.https://doi.org/10.1140/epjc/s10052-024-13516-9 |
| spellingShingle | A. Agrawal V. V. Alenkov P. Aryal J. Beyer B. Bhandari R. S. Boiko K. Boonin O. Buzanov C. R. Byeon N. Chanthima M. K. Cheoun J. S. Choe Seonho Choi S. Choudhury J. S. Chung F. A. Danevich M. Djamal D. Drung C. Enss A. Fleischmann A. M. Gangapshev L. Gastaldo Y. M. Gavrilyuk A. M. Gezhaev O. Gileva V. D. Grigorieva V. I. Gurentsov C. Ha D. H. Ha E. J. Ha D. H. Hwnag E. J. Jeon J. A. Jeon H. S. Jo J. Kaewkhao C. S. Kang W. G. Kang V. V. Kazalov S. Kempf A. Khan S. Khan D. Y. Kim G. W. Kim H. B. Kim Ho-Jong Kim H. J. Kim H. L. Kim H. S. Kim M. B. Kim S. C. Kim S. K. Kim S. R. Kim W. T. Kim Y. D. Kim Y. H. Kim K. Kirdsiri Y. J. Ko V. V. Kobychev V. Kornoukhov V. V. Kuzminov D. H. Kwon C. H. Lee DongYeup Lee E. K. Lee H. J. Lee H. S. Lee J. Lee J. Y. Lee K. B. Lee M. H. Lee M. K. Lee S. W. Lee Y. C. Lee D. S. Leonard H. S. Lim B. Mailyan E. P. Makarov P. Nyanda Y. Oh S. L. Olsen S. I. Panasenko H. K. Park H. S. Park K. S. Park S. Y. Park O. G. Polischuk H. Prihtiadi S. Ra S. S. Ratkevich G. Rooh E. Sala M. B. Sari J. Seo K. M. Seo B. Sharma K. A. Shin V. N. Shlegel K. Siyeon J. So N. V. Sokur J. K. Son J. W. Song N. Srisittipokakun V. I. Tretyak R. Wirawan K. R. Woo H. J. Yeon Y. S. Yoon Q. Yue The AMoRE Collaboration Projected background and sensitivity of AMoRE-II European Physical Journal C: Particles and Fields |
| title | Projected background and sensitivity of AMoRE-II |
| title_full | Projected background and sensitivity of AMoRE-II |
| title_fullStr | Projected background and sensitivity of AMoRE-II |
| title_full_unstemmed | Projected background and sensitivity of AMoRE-II |
| title_short | Projected background and sensitivity of AMoRE-II |
| title_sort | projected background and sensitivity of amore ii |
| url | https://doi.org/10.1140/epjc/s10052-024-13516-9 |
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