European Physical Journal C: Particles and Fields (Jan 2025)
Projected background and sensitivity of AMoRE-II
- 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
Affiliations
- A. Agrawal
- Indian Institute of Science
- V. V. Alenkov
- JSC FOMOS-Materials
- P. Aryal
- Department of Physics, Kyungpook National University
- J. Beyer
- Physikalisch-Technische Bundesanstalt
- B. Bhandari
- Department of Physics and Astronomy, Sejong University
- R. S. Boiko
- Institute for Nuclear Research of NASU
- K. Boonin
- Nakhon Pathom Rajabhat University
- O. Buzanov
- JSC FOMOS-Materials
- C. R. Byeon
- Department of Physics, Kyungpook National University
- N. Chanthima
- Nakhon Pathom Rajabhat University
- M. K. Cheoun
- Department of Physics, Soongsil University
- J. S. Choe
- Center for Underground Physics, Institute for Basic Science (IBS)
- Seonho Choi
- Department of Physics and Astronomy, Seoul National University
- S. Choudhury
- Indian Institute of Science
- J. S. Chung
- Department of Physics, Chung-Ang University
- F. A. Danevich
- Institute for Nuclear Research of NASU
- M. Djamal
- Department of Physics, Institut Teknologi
- D. Drung
- Physikalisch-Technische Bundesanstalt
- C. Enss
- Kirchhoff-Institute for Physics
- A. Fleischmann
- Kirchhoff-Institute for Physics
- A. M. Gangapshev
- Neutrino Observatory of INR RAS
- L. Gastaldo
- Kirchhoff-Institute for Physics
- Y. M. Gavrilyuk
- Neutrino Observatory of INR RAS
- A. M. Gezhaev
- Neutrino Observatory of INR RAS
- O. Gileva
- Center for Underground Physics, Institute for Basic Science (IBS)
- V. D. Grigorieva
- Nikolaev Institute of Inorganic Chemistry, Siberian Branch of Russian Academy of Science
- V. I. Gurentsov
- Neutrino Observatory of INR RAS
- C. Ha
- Department of Physics, Chung-Ang University
- D. H. Ha
- Department of Physics, Kyungpook National University
- E. J. Ha
- Department of Physics, Soongsil University
- D. H. Hwnag
- Center for Underground Physics, Institute for Basic Science (IBS)
- E. J. Jeon
- University of Science and Technology (UST)
- J. A. Jeon
- Center for Underground Physics, Institute for Basic Science (IBS)
- H. S. Jo
- Department of Physics, Kyungpook National University
- J. Kaewkhao
- Nakhon Pathom Rajabhat University
- C. S. Kang
- Center for Underground Physics, Institute for Basic Science (IBS)
- W. G. Kang
- Center for Underground Physics, Institute for Basic Science (IBS)
- V. V. Kazalov
- Neutrino Observatory of INR RAS
- S. Kempf
- Institute of Micro- and Nanoelectronic Systems (IMS), Karlsruhe Institute of Technology (KIT)
- A. Khan
- Department of Physics, Kyungpook National University
- S. Khan
- Department of Physics, Kohat University of Science and Technology
- D. Y. Kim
- Center for Underground Physics, Institute for Basic Science (IBS)
- G. W. Kim
- Center for Underground Physics, Institute for Basic Science (IBS)
- H. B. Kim
- Department of Physics and Astronomy, Seoul National University
- Ho-Jong Kim
- Center for Underground Physics, Institute for Basic Science (IBS)
- H. J. Kim
- Department of Physics, Kyungpook National University
- H. L. Kim
- Department of Physics, Kyungpook National University
- H. S. Kim
- Department of Physics and Astronomy, Sejong University
- M. B. Kim
- Center for Underground Physics, Institute for Basic Science (IBS)
- S. C. Kim
- Center for Underground Physics, Institute for Basic Science (IBS)
- S. K. Kim
- Department of Physics and Astronomy, Seoul National University
- S. R. Kim
- Center for Underground Physics, Institute for Basic Science (IBS)
- W. T. Kim
- University of Science and Technology (UST)
- Y. D. Kim
- University of Science and Technology (UST)
- Y. H. Kim
- University of Science and Technology (UST)
- K. Kirdsiri
- Nakhon Pathom Rajabhat University
- Y. J. Ko
- Center for Underground Physics, Institute for Basic Science (IBS)
- V. V. Kobychev
- Institute for Nuclear Research of NASU
- V. Kornoukhov
- National Research Nuclear University MEPhI
- V. V. Kuzminov
- Neutrino Observatory of INR RAS
- D. H. Kwon
- University of Science and Technology (UST)
- C. H. Lee
- Center for Underground Physics, Institute for Basic Science (IBS)
- DongYeup Lee
- Department of Accelerator Science
- E. K. Lee
- Center for Underground Physics, Institute for Basic Science (IBS)
- H. J. Lee
- Center for Underground Physics, Institute for Basic Science (IBS)
- H. S. Lee
- University of Science and Technology (UST)
- J. Lee
- Center for Underground Physics, Institute for Basic Science (IBS)
- J. Y. Lee
- Department of Physics, Kyungpook National University
- K. B. Lee
- Korea Research Institute of Standards and Science
- M. H. Lee
- University of Science and Technology (UST)
- M. K. Lee
- Korea Research Institute of Standards and Science
- S. W. Lee
- Department of Physics, Kyungpook National University
- Y. C. Lee
- Department of Physics and Astronomy, Seoul National University
- D. S. Leonard
- Center for Underground Physics, Institute for Basic Science (IBS)
- H. S. Lim
- Department of Physics, Kyungpook National University
- B. Mailyan
- Florida Institute of Technology
- E. P. Makarov
- Nikolaev Institute of Inorganic Chemistry, Siberian Branch of Russian Academy of Science
- P. Nyanda
- University of Science and Technology (UST)
- Y. Oh
- Center for Underground Physics, Institute for Basic Science (IBS)
- S. L. Olsen
- Center for Underground Physics, Institute for Basic Science (IBS)
- S. I. Panasenko
- Neutrino Observatory of INR RAS
- H. K. Park
- Department of Accelerator Science
- H. S. Park
- Korea Research Institute of Standards and Science
- K. S. Park
- Center for Underground Physics, Institute for Basic Science (IBS)
- S. Y. Park
- Center for Underground Physics, Institute for Basic Science (IBS)
- O. G. Polischuk
- Institute for Nuclear Research of NASU
- H. Prihtiadi
- Department of Physics, Universitas Negeri Malang
- S. Ra
- Center for Underground Physics, Institute for Basic Science (IBS)
- S. S. Ratkevich
- Neutrino Observatory of INR RAS
- G. Rooh
- Department of Physics, Abdul Wali Khan University
- E. Sala
- Center for Underground Physics, Institute for Basic Science (IBS)
- M. B. Sari
- Department of Physics, Institut Teknologi
- J. Seo
- University of Science and Technology (UST)
- K. M. Seo
- Department of Physics and Astronomy, Sejong University
- B. Sharma
- University of Science and Technology (UST)
- K. A. Shin
- Center for Underground Physics, Institute for Basic Science (IBS)
- V. N. Shlegel
- Nikolaev Institute of Inorganic Chemistry, Siberian Branch of Russian Academy of Science
- K. Siyeon
- Department of Physics, Chung-Ang University
- J. So
- Center for Underground Physics, Institute for Basic Science (IBS)
- N. V. Sokur
- Institute for Nuclear Research of NASU
- J. K. Son
- Center for Underground Physics, Institute for Basic Science (IBS)
- J. W. Song
- Nakhon Pathom Rajabhat University
- N. Srisittipokakun
- Nakhon Pathom Rajabhat University
- V. I. Tretyak
- Institute for Nuclear Research of NASU
- R. Wirawan
- Department of Physics, University of Mataram
- K. R. Woo
- Center for Underground Physics, Institute for Basic Science (IBS)
- H. J. Yeon
- Center for Underground Physics, Institute for Basic Science (IBS)
- Y. S. Yoon
- Korea Research Institute of Standards and Science
- Q. Yue
- Tsinghua University
- The AMoRE Collaboration
- DOI
- https://doi.org/10.1140/epjc/s10052-024-13516-9
- Journal volume & issue
-
Vol. 85,
no. 1
pp. 1 – 14
Abstract
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.