Cosmogenic background study for a Mo-based bolometric demonstration experiment at China JinPing underground Laboratory

W. Chen; L. Ma; J. H. Chen; H. Z. Huang; Y. G. Ma

doi:10.1140/epjc/s10052-022-10501-y

2024 Impact factor 4.8

Particles and Fields

Open Access

Eur. Phys. J. C (2022) 82: 549
https://doi.org/10.1140/epjc/s10052-022-10501-y

Regular Article - Theoretical Physics

Cosmogenic background study for a $^{100}$ $^{100}$ Mo-based bolometric demonstration experiment at China JinPing underground Laboratory

W. Chen¹, L. Ma¹^b, J. H. Chen¹, H. Z. Huang¹^,2 and Y. G. Ma¹

¹ Key Laboratory of Nuclear Physics and Ion-beam Application (MOE), Institute of Modern Physics, Fudan University, Shanghai, China
² Department of Physics and Astronomy, University of California, Los Angeles, CA, USA

^b malong@fudan.edu.cn

Received: 19 January 2022
Accepted: 7 June 2022
Published online: 22 June 2022

Abstract

We perform simulation study for a 10-kg $^{100}$ $^{100}$ Mo-based bolometeric demonstration experiment for neutrinoless double-beta decay ( $0 ν β β$ $0\nu \beta \beta$ ) search at China JinPing underground Laboratory (CJPL). Cosmogenic production of radionuclides in $^{100}$ $^{100}$ Mo-enriched lithium molybdate crystals and copper components of the detector system are studied using Geant4 toolkit based on the simulated cosmic ray data from the CRY library. Background energy spectra of the cosmogenic radionuclides including $^{56}$ $^{56}$ Co, $^{82}$ $^{82}$ Rb and $^{88}$ $^{88}$ Y which are harmful for the $^{100}$ $^{100}$ Mo-based $0 ν β β$ $0\nu \beta \beta$ experiment are investigated. We then evaluate the total cosmogenic background level in the $^{100}$ $^{100}$ Mo $0 ν β β$ $0\nu \beta \beta$ search energy region of interest (ROI) for the demonstration experiment. After one year of cooling down underground, the residual background contribution is found to be 1.8 $\times$ $\times$ 10 $^{- 6}$ $^{-6}$ cts/kg/keV/yr and 3.3 $\times$ $\times$ 10 $^{- 4}$ $^{-4}$ cts/kg/keV/yr from crystals and copper components, respectively. Furthermore, underground cosmogenic activation of copper and lithium molybdate crystal is calculated based on the simulation spectra of neutron and proton in CJPL. The underground cosmogenic background is found to be negligible in the ROI.

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