AMoRE (100Mo)

(Advanced Mo based Rare process Experiment)

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References

1 - Neutrinoless Double Beta Decay

[1-1]
Status and performance of the AMoRE-I experiment on neutrinoless double beta decay, H. B. Kim et al., J.Low Temp.Phys. 209 (2022) 962-970, arXiv:2211.02825.
[Kim:2022uce]
[1-2]
First Results from the AMoRE-Pilot neutrinoless double beta decay experiment, V. Alenkov et al. (AMoRE), Eur.Phys.J. C79 (2019) 791, arXiv:1903.09483.
[Alenkov:2019jis]

2 - Detector

[2-1]
A feasibility study of extruded plastic scintillator embedding WLS fiber for AMoRE-II muon veto, J. W. Seo, W. T. Kim, Y. D. Kim, H. Y. Lee, J. Lee, M. H. Lee, P. B. Nyanda, E. S. Yi, Nucl.Instrum.Meth.A 1039 (2022) 167123, arXiv:2201.08034.
[Seo:2022vzr]
[2-2]
Measurement of the Background Activities of a 100Mo-enriched powder sample for AMoRE crystal material using a single high purity germanium detector, Su-yeon Park, Insik Hahn, Woon Gu Kang, Gowoon Kim, Eun Kyung Lee, Douglas S. Leonard, Vladimir Kazalov, Yeong Duk Kim, Moo Hyun Lee, Elena Sala, J.Korean Phys.Soc. 76 (2020) 1060-1066, arXiv:2005.09919.
[Park:2020vxl]
[2-3]
Neutron and muon-induced background studies for the AMoRE double-beta decay experiment, H.W. Bae, E.J. Jeon, Y.D. Kim, S.W. Lee (AMoRE), Astropart.Phys. 114 (2020) 60-67, arXiv:1812.07476.
[Bae:2018taz]
[2-4]
A CaMoO4 Crystal Low Temperature Detector for the AMoRE Neutrinoless Double Beta Decay Search, G.B. Kim et al. (AMoRE), Adv. High Energy Phys. 2015 (2015) 817530, arXiv:1602.07401.
[Kim:2015pua]
[2-5]
Simulations of background sources in AMoRE-I experiment, A. Luqman et al. (AMoRE), Nucl.Instrum.Meth. A855 (2017) 140-147, arXiv:1601.01249.
[Luqman:2016okt]
[2-6]
Technical Design Report for the AMoRE $0\nu\beta\beta$ Decay Search Experiment, V. Alenkov et al. (AMoRE), arXiv:1512.05957, 2015.
[AMoRE:2015asn]
[2-7]
AMoRE: Collaboration for searches for the neutrinoless double-beta decay of the isotope of $^{100}Mo$ with the aid of $^{40}Ca^{100}MoO_{4}$ as a cryogenic scintillation detector, N.D. Khanbekov (AMoRE), Phys.Atom.Nucl. 76 (2013) 1086-1089.
[Khanbekov:2013dja]

3 - Background

[3-1]
Radon Concentration Measurement with a High-Sensitivity Radon Detector at the Yemilab, Kyungmin Seo, Hyunsoo Kim, Yeongduk Kim, Hyeyoung Lee, Jaison Lee, Moo Hyun Lee, Jungho So, Sangcheol Yoon, Youngsoo Yoon, arXiv:2403.07405, 2024.
[Seo:2024rea]
[3-2]
Background study of the AMoRE-pilot experiment, A. Agrawal et al. (AMoRE), arXiv:2401.07476, 2024.
[AMoRE:2024cun]
[3-3]
Alpha backgrounds in the AMoRE-Pilot experiment, V. Alenkov et al., Eur.Phys.J.C 82 (2022) 1140, arXiv:2107.07704.
[Alenkov:2021asw]
[3-4]
Measurement of the Background Activities of a 100Mo-enriched Powder Sample for an AMoRE Crystal Material by using Fourteen High-Purity Germanium Detectors, S. Y. Park, K. I. Hahn, W. G. Kang, V. Kazalov, G. W. Kim, Y. D. Kim, E. K. Lee, M. H. Lee, D. S. Leonard, Nucl.Instrum.Meth. A992 (2021) 165020, arXiv:2009.02021.
[Park:2020vax]

4 - Talks

[4-1]
Growth and development of pure Li2MoO4 crystals for rare event experiment at CUP, J. K. Son et al., JINST 15 (2020) C07035, arXiv:2005.06797. INSTR'20 (Novosibirsk, Feb. 24-28, 2020).
[Son:2020saj]
[4-2]
Purification and recovery of 100MoO3 in crystal production for AMoRE experiment, O. Gileva, J.S. Choe, H.J. Kim, Y.D. Kim, M.H. Lee, H.K. Park, K.A. Shin, JINST 15 (2020) C07032, arXiv:2005.06463. INSTR'20 (Novosibirsk, Feb. 24-28, 2020).
[Gileva:2020dyy]
[4-3]
AMoRE: A search for neutrinoless double-beta decay of 100Mo using low-temperature molybdenum-containing crystal detectors, Moo Hyun Lee (AMoRE), JINST 15 (2020) C08010, arXiv:2005.05567. INSTR'20 (Novosibirsk, Feb. 24-28, 2020).
[Lee:2020rjh]
[4-4]
AMoRE experiment: a search for neutrinoless double beta decay of Mo-100 isotope with Ca-40 MoO-100(4) cryogenic scintillation detector, H. Bhang, R.S. Boiko, D.M. Chernyak, J.H. Choi, S. Choi et al., J. Phys. Conf. Ser. 375 (2012) 042023.
[Bhang:2012gn]

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Authors:
Stefano Gariazzo / gariazzo@to.infn.it
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it
Last Update: Wed 17 Apr 2024, 15:26:17 CET