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Final results on the 0νββ decay half-life limit of 100Mo from the CUPID-Mo experiment
The CUPID-Mo experiment to search for 0 ν β β decay in 100 Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0 ν β β decay experiment. CUPID-Mo was comprised of 20 enriched Li 2 100...
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Published in: | The European physical journal. C, Particles and fields Particles and fields, 2022-11, Vol.82 (11), p.1033 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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container_title | The European physical journal. C, Particles and fields |
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creator | Augier, C. Barabash, A. S. Bellini, F. Benato, G. Beretta, M. Bergé, L. Billard, J. Borovlev, Yu. A. Cardani, L. Casali, N. Cazes, A. Chapellier, M. Chiesa, D. Dafinei, I. Danevich, F. A. De Jesus, M. de Marcillac, P. Dixon, T. Dumoulin, L. Eitel, K. Ferri, F. Fujikawa, B. K. Gascon, J. Gironi, L. Giuliani, A. Grigorieva, V. D. Gros, M. Helis, D. L. Huang, H. Z. Huang, R. Imbert, L. Johnston, J. Juillard, A. Khalife, H. Kleifges, M. Kobychev, V. V. Kolomensky, Yu. G. Konovalov, S. I. Loaiza, P. Ma, L. Makarov, E. P. Mariam, R. Marini, L. Marnieros, S. Navick, X.-F. Nones, C. Norman, E. B. Olivieri, E. Ouellet, J. L. Pagnanini, L. Pattavina, L. Paul, B. Pavan, M. Peng, H. Pessina, G. Pirro, S. Poda, D. V. Polischuk, O. G. Pozzi, S. Previtali, E. Redon, Th Rojas, A. Rozov, S. Sanglard, V. Scarpaci, J. A. Schmidt, B. Shen, Y. Shlegel, V. N. Singh, V. Tomei, C. Tretyak, V. I. Umatov, V. I. Vagneron, L. Velázquez, M. Welliver, B. Winslow, L. Xue, M. Yakushev, E. Zarytskyy, M. Zolotarova, A. S. |
description | The CUPID-Mo experiment to search for 0
ν
β
β
decay in
100
Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0
ν
β
β
decay experiment. CUPID-Mo was comprised of 20 enriched
Li
2
100
MoO
4
scintillating calorimeters, each with a mass of
∼
0.2
kg, operated at
∼
20
mK. We present here the final analysis with the full exposure of CUPID-Mo (
100
Mo exposure of 1.47
kg
×
year
) used to search for lepton number violation via 0
ν
β
β
decay. We report on various analysis improvements since the previous result on a subset of data, reprocessing all data with these new techniques. We observe zero events in the region of interest and set a new limit on the
100
Mo 0
ν
β
β
decay half-life of
T
1
/
2
0
ν
>
1.8
×
10
24
year (stat. + syst.) at 90% CI. Under the light Majorana neutrino exchange mechanism this corresponds to an effective Majorana neutrino mass of
m
β
β
<
(
0.28
-
0.49
)
eV, dependent upon the nuclear matrix element utilized. |
doi_str_mv | 10.1140/epjc/s10052-022-10942-5 |
format | article |
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ν
β
β
decay in
100
Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0
ν
β
β
decay experiment. CUPID-Mo was comprised of 20 enriched
Li
2
100
MoO
4
scintillating calorimeters, each with a mass of
∼
0.2
kg, operated at
∼
20
mK. We present here the final analysis with the full exposure of CUPID-Mo (
100
Mo exposure of 1.47
kg
×
year
) used to search for lepton number violation via 0
ν
β
β
decay. We report on various analysis improvements since the previous result on a subset of data, reprocessing all data with these new techniques. We observe zero events in the region of interest and set a new limit on the
100
Mo 0
ν
β
β
decay half-life of
T
1
/
2
0
ν
>
1.8
×
10
24
year (stat. + syst.) at 90% CI. Under the light Majorana neutrino exchange mechanism this corresponds to an effective Majorana neutrino mass of
m
β
β
<
(
0.28
-
0.49
)
eV, dependent upon the nuclear matrix element utilized.</description><identifier>ISSN: 1434-6044</identifier><identifier>EISSN: 1434-6052</identifier><identifier>DOI: 10.1140/epjc/s10052-022-10942-5</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Astronomy ; Astrophysics and Cosmology ; Decay ; Elementary Particles ; Experiments ; Hadrons ; Half-life ; Heavy Ions ; Leptons ; Measurement Science and Instrumentation ; Neutrinos ; Nuclear Energy ; Nuclear Physics ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Regular Article - Experimental Physics ; Reprocessing ; String Theory</subject><ispartof>The European physical journal. C, Particles and fields, 2022-11, Vol.82 (11), p.1033</ispartof><rights>The Author(s) 2022</rights><rights>The Author(s) 2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><orcidid>0000-0002-0515-3773</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/2736485035/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/2736485035?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25753,27924,27925,37012,44590,75126</link.rule.ids></links><search><creatorcontrib>Augier, C.</creatorcontrib><creatorcontrib>Barabash, A. S.</creatorcontrib><creatorcontrib>Bellini, F.</creatorcontrib><creatorcontrib>Benato, G.</creatorcontrib><creatorcontrib>Beretta, M.</creatorcontrib><creatorcontrib>Bergé, L.</creatorcontrib><creatorcontrib>Billard, J.</creatorcontrib><creatorcontrib>Borovlev, Yu. A.</creatorcontrib><creatorcontrib>Cardani, L.</creatorcontrib><creatorcontrib>Casali, N.</creatorcontrib><creatorcontrib>Cazes, A.</creatorcontrib><creatorcontrib>Chapellier, M.</creatorcontrib><creatorcontrib>Chiesa, D.</creatorcontrib><creatorcontrib>Dafinei, I.</creatorcontrib><creatorcontrib>Danevich, F. A.</creatorcontrib><creatorcontrib>De Jesus, M.</creatorcontrib><creatorcontrib>de Marcillac, P.</creatorcontrib><creatorcontrib>Dixon, T.</creatorcontrib><creatorcontrib>Dumoulin, L.</creatorcontrib><creatorcontrib>Eitel, K.</creatorcontrib><creatorcontrib>Ferri, F.</creatorcontrib><creatorcontrib>Fujikawa, B. K.</creatorcontrib><creatorcontrib>Gascon, J.</creatorcontrib><creatorcontrib>Gironi, L.</creatorcontrib><creatorcontrib>Giuliani, A.</creatorcontrib><creatorcontrib>Grigorieva, V. D.</creatorcontrib><creatorcontrib>Gros, M.</creatorcontrib><creatorcontrib>Helis, D. L.</creatorcontrib><creatorcontrib>Huang, H. Z.</creatorcontrib><creatorcontrib>Huang, R.</creatorcontrib><creatorcontrib>Imbert, L.</creatorcontrib><creatorcontrib>Johnston, J.</creatorcontrib><creatorcontrib>Juillard, A.</creatorcontrib><creatorcontrib>Khalife, H.</creatorcontrib><creatorcontrib>Kleifges, M.</creatorcontrib><creatorcontrib>Kobychev, V. V.</creatorcontrib><creatorcontrib>Kolomensky, Yu. G.</creatorcontrib><creatorcontrib>Konovalov, S. I.</creatorcontrib><creatorcontrib>Loaiza, P.</creatorcontrib><creatorcontrib>Ma, L.</creatorcontrib><creatorcontrib>Makarov, E. P.</creatorcontrib><creatorcontrib>Mariam, R.</creatorcontrib><creatorcontrib>Marini, L.</creatorcontrib><creatorcontrib>Marnieros, S.</creatorcontrib><creatorcontrib>Navick, X.-F.</creatorcontrib><creatorcontrib>Nones, C.</creatorcontrib><creatorcontrib>Norman, E. B.</creatorcontrib><creatorcontrib>Olivieri, E.</creatorcontrib><creatorcontrib>Ouellet, J. L.</creatorcontrib><creatorcontrib>Pagnanini, L.</creatorcontrib><creatorcontrib>Pattavina, L.</creatorcontrib><creatorcontrib>Paul, B.</creatorcontrib><creatorcontrib>Pavan, M.</creatorcontrib><creatorcontrib>Peng, H.</creatorcontrib><creatorcontrib>Pessina, G.</creatorcontrib><creatorcontrib>Pirro, S.</creatorcontrib><creatorcontrib>Poda, D. V.</creatorcontrib><creatorcontrib>Polischuk, O. G.</creatorcontrib><creatorcontrib>Pozzi, S.</creatorcontrib><creatorcontrib>Previtali, E.</creatorcontrib><creatorcontrib>Redon, Th</creatorcontrib><creatorcontrib>Rojas, A.</creatorcontrib><creatorcontrib>Rozov, S.</creatorcontrib><creatorcontrib>Sanglard, V.</creatorcontrib><creatorcontrib>Scarpaci, J. A.</creatorcontrib><creatorcontrib>Schmidt, B.</creatorcontrib><creatorcontrib>Shen, Y.</creatorcontrib><creatorcontrib>Shlegel, V. N.</creatorcontrib><creatorcontrib>Singh, V.</creatorcontrib><creatorcontrib>Tomei, C.</creatorcontrib><creatorcontrib>Tretyak, V. I.</creatorcontrib><creatorcontrib>Umatov, V. I.</creatorcontrib><creatorcontrib>Vagneron, L.</creatorcontrib><creatorcontrib>Velázquez, M.</creatorcontrib><creatorcontrib>Welliver, B.</creatorcontrib><creatorcontrib>Winslow, L.</creatorcontrib><creatorcontrib>Xue, M.</creatorcontrib><creatorcontrib>Yakushev, E.</creatorcontrib><creatorcontrib>Zarytskyy, M.</creatorcontrib><creatorcontrib>Zolotarova, A. S.</creatorcontrib><title>Final results on the 0νββ decay half-life limit of 100Mo from the CUPID-Mo experiment</title><title>The European physical journal. C, Particles and fields</title><addtitle>Eur. Phys. J. C</addtitle><description>The CUPID-Mo experiment to search for 0
ν
β
β
decay in
100
Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0
ν
β
β
decay experiment. CUPID-Mo was comprised of 20 enriched
Li
2
100
MoO
4
scintillating calorimeters, each with a mass of
∼
0.2
kg, operated at
∼
20
mK. We present here the final analysis with the full exposure of CUPID-Mo (
100
Mo exposure of 1.47
kg
×
year
) used to search for lepton number violation via 0
ν
β
β
decay. We report on various analysis improvements since the previous result on a subset of data, reprocessing all data with these new techniques. We observe zero events in the region of interest and set a new limit on the
100
Mo 0
ν
β
β
decay half-life of
T
1
/
2
0
ν
>
1.8
×
10
24
year (stat. + syst.) at 90% CI. Under the light Majorana neutrino exchange mechanism this corresponds to an effective Majorana neutrino mass of
m
β
β
<
(
0.28
-
0.49
)
eV, dependent upon the nuclear matrix element utilized.</description><subject>Astronomy</subject><subject>Astrophysics and Cosmology</subject><subject>Decay</subject><subject>Elementary Particles</subject><subject>Experiments</subject><subject>Hadrons</subject><subject>Half-life</subject><subject>Heavy Ions</subject><subject>Leptons</subject><subject>Measurement Science and Instrumentation</subject><subject>Neutrinos</subject><subject>Nuclear Energy</subject><subject>Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Regular Article - Experimental Physics</subject><subject>Reprocessing</subject><subject>String Theory</subject><issn>1434-6044</issn><issn>1434-6052</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNpFkN9KwzAUh4MoOKfPYMDruJN_bXop083BRC8meBeaJnEdXVubDvS1du8r7JnMNtGrc_jxcX6cD6FrCreUChi5dlWMAgWQjABjhEImGJEnaEAFFySJ-enfLsQ5ughhBQBMgBqgt0lZ5xXuXNhUfcBNjfulw7D73m13W2xdkX_hZV55UpXe4apclz1uPI51Tw32XbM-8OPXl9k9iYn7bF1Xrl3dX6Izn1fBXf3OIVpMHhbjRzJ_ns7Gd3PSpqkkhTW5tBmPPQoKZqWhTAie-EyoAlSaGssz6QqeZtYAT5yx3nuTguPK8NzwIbo5nm275mPjQq9XzaaLLwXNUp4IJYHLSKkjFdqurN9d909R0HuNeq9RHzXqqFEfNGrJfwBlr2ir</recordid><startdate>20221115</startdate><enddate>20221115</enddate><creator>Augier, C.</creator><creator>Barabash, A. S.</creator><creator>Bellini, F.</creator><creator>Benato, G.</creator><creator>Beretta, M.</creator><creator>Bergé, L.</creator><creator>Billard, J.</creator><creator>Borovlev, Yu. A.</creator><creator>Cardani, L.</creator><creator>Casali, N.</creator><creator>Cazes, A.</creator><creator>Chapellier, M.</creator><creator>Chiesa, D.</creator><creator>Dafinei, I.</creator><creator>Danevich, F. A.</creator><creator>De Jesus, M.</creator><creator>de Marcillac, P.</creator><creator>Dixon, T.</creator><creator>Dumoulin, L.</creator><creator>Eitel, K.</creator><creator>Ferri, F.</creator><creator>Fujikawa, B. K.</creator><creator>Gascon, J.</creator><creator>Gironi, L.</creator><creator>Giuliani, A.</creator><creator>Grigorieva, V. D.</creator><creator>Gros, M.</creator><creator>Helis, D. L.</creator><creator>Huang, H. 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S.</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>7U5</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><orcidid>https://orcid.org/0000-0002-0515-3773</orcidid></search><sort><creationdate>20221115</creationdate><title>Final results on the 0νββ decay half-life limit of 100Mo from the CUPID-Mo experiment</title><author>Augier, C. ; Barabash, A. S. ; Bellini, F. ; Benato, G. ; Beretta, M. ; Bergé, L. ; Billard, J. ; Borovlev, Yu. A. ; Cardani, L. ; Casali, N. ; Cazes, A. ; Chapellier, M. ; Chiesa, D. ; Dafinei, I. ; Danevich, F. A. ; De Jesus, M. ; de Marcillac, P. ; Dixon, T. ; Dumoulin, L. ; Eitel, K. ; Ferri, F. ; Fujikawa, B. K. ; Gascon, J. ; Gironi, L. ; Giuliani, A. ; Grigorieva, V. D. ; Gros, M. ; Helis, D. L. ; Huang, H. Z. ; Huang, R. ; Imbert, L. ; Johnston, J. ; Juillard, A. ; Khalife, H. ; Kleifges, M. ; Kobychev, V. V. ; Kolomensky, Yu. G. ; Konovalov, S. I. ; Loaiza, P. ; Ma, L. ; Makarov, E. P. ; Mariam, R. ; Marini, L. ; Marnieros, S. ; Navick, X.-F. ; Nones, C. ; Norman, E. B. ; Olivieri, E. ; Ouellet, J. L. ; Pagnanini, L. ; Pattavina, L. ; Paul, B. ; Pavan, M. ; Peng, H. ; Pessina, G. ; Pirro, S. ; Poda, D. V. ; Polischuk, O. G. ; Pozzi, S. ; Previtali, E. ; Redon, Th ; Rojas, A. ; Rozov, S. ; Sanglard, V. ; Scarpaci, J. A. ; Schmidt, B. ; Shen, Y. ; Shlegel, V. N. ; Singh, V. ; Tomei, C. ; Tretyak, V. I. ; Umatov, V. I. ; Vagneron, L. ; Velázquez, M. ; Welliver, B. ; Winslow, L. ; Xue, M. ; Yakushev, E. ; Zarytskyy, M. ; Zolotarova, A. S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p775-cdba5d93eca80c2d5b124436f948c0877bd395ec379db036ebdfffb70e38b3ab3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Astronomy</topic><topic>Astrophysics and Cosmology</topic><topic>Decay</topic><topic>Elementary Particles</topic><topic>Experiments</topic><topic>Hadrons</topic><topic>Half-life</topic><topic>Heavy Ions</topic><topic>Leptons</topic><topic>Measurement Science and Instrumentation</topic><topic>Neutrinos</topic><topic>Nuclear Energy</topic><topic>Nuclear Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Regular Article - Experimental Physics</topic><topic>Reprocessing</topic><topic>String Theory</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Augier, C.</creatorcontrib><creatorcontrib>Barabash, A. S.</creatorcontrib><creatorcontrib>Bellini, F.</creatorcontrib><creatorcontrib>Benato, G.</creatorcontrib><creatorcontrib>Beretta, M.</creatorcontrib><creatorcontrib>Bergé, L.</creatorcontrib><creatorcontrib>Billard, J.</creatorcontrib><creatorcontrib>Borovlev, Yu. A.</creatorcontrib><creatorcontrib>Cardani, L.</creatorcontrib><creatorcontrib>Casali, N.</creatorcontrib><creatorcontrib>Cazes, A.</creatorcontrib><creatorcontrib>Chapellier, M.</creatorcontrib><creatorcontrib>Chiesa, D.</creatorcontrib><creatorcontrib>Dafinei, I.</creatorcontrib><creatorcontrib>Danevich, F. A.</creatorcontrib><creatorcontrib>De Jesus, M.</creatorcontrib><creatorcontrib>de Marcillac, P.</creatorcontrib><creatorcontrib>Dixon, T.</creatorcontrib><creatorcontrib>Dumoulin, L.</creatorcontrib><creatorcontrib>Eitel, K.</creatorcontrib><creatorcontrib>Ferri, F.</creatorcontrib><creatorcontrib>Fujikawa, B. K.</creatorcontrib><creatorcontrib>Gascon, J.</creatorcontrib><creatorcontrib>Gironi, L.</creatorcontrib><creatorcontrib>Giuliani, A.</creatorcontrib><creatorcontrib>Grigorieva, V. D.</creatorcontrib><creatorcontrib>Gros, M.</creatorcontrib><creatorcontrib>Helis, D. L.</creatorcontrib><creatorcontrib>Huang, H. Z.</creatorcontrib><creatorcontrib>Huang, R.</creatorcontrib><creatorcontrib>Imbert, L.</creatorcontrib><creatorcontrib>Johnston, J.</creatorcontrib><creatorcontrib>Juillard, A.</creatorcontrib><creatorcontrib>Khalife, H.</creatorcontrib><creatorcontrib>Kleifges, M.</creatorcontrib><creatorcontrib>Kobychev, V. V.</creatorcontrib><creatorcontrib>Kolomensky, Yu. G.</creatorcontrib><creatorcontrib>Konovalov, S. I.</creatorcontrib><creatorcontrib>Loaiza, P.</creatorcontrib><creatorcontrib>Ma, L.</creatorcontrib><creatorcontrib>Makarov, E. P.</creatorcontrib><creatorcontrib>Mariam, R.</creatorcontrib><creatorcontrib>Marini, L.</creatorcontrib><creatorcontrib>Marnieros, S.</creatorcontrib><creatorcontrib>Navick, X.-F.</creatorcontrib><creatorcontrib>Nones, C.</creatorcontrib><creatorcontrib>Norman, E. B.</creatorcontrib><creatorcontrib>Olivieri, E.</creatorcontrib><creatorcontrib>Ouellet, J. L.</creatorcontrib><creatorcontrib>Pagnanini, L.</creatorcontrib><creatorcontrib>Pattavina, L.</creatorcontrib><creatorcontrib>Paul, B.</creatorcontrib><creatorcontrib>Pavan, M.</creatorcontrib><creatorcontrib>Peng, H.</creatorcontrib><creatorcontrib>Pessina, G.</creatorcontrib><creatorcontrib>Pirro, S.</creatorcontrib><creatorcontrib>Poda, D. V.</creatorcontrib><creatorcontrib>Polischuk, O. G.</creatorcontrib><creatorcontrib>Pozzi, S.</creatorcontrib><creatorcontrib>Previtali, E.</creatorcontrib><creatorcontrib>Redon, Th</creatorcontrib><creatorcontrib>Rojas, A.</creatorcontrib><creatorcontrib>Rozov, S.</creatorcontrib><creatorcontrib>Sanglard, V.</creatorcontrib><creatorcontrib>Scarpaci, J. A.</creatorcontrib><creatorcontrib>Schmidt, B.</creatorcontrib><creatorcontrib>Shen, Y.</creatorcontrib><creatorcontrib>Shlegel, V. N.</creatorcontrib><creatorcontrib>Singh, V.</creatorcontrib><creatorcontrib>Tomei, C.</creatorcontrib><creatorcontrib>Tretyak, V. I.</creatorcontrib><creatorcontrib>Umatov, V. I.</creatorcontrib><creatorcontrib>Vagneron, L.</creatorcontrib><creatorcontrib>Velázquez, M.</creatorcontrib><creatorcontrib>Welliver, B.</creatorcontrib><creatorcontrib>Winslow, L.</creatorcontrib><creatorcontrib>Xue, M.</creatorcontrib><creatorcontrib>Yakushev, E.</creatorcontrib><creatorcontrib>Zarytskyy, M.</creatorcontrib><creatorcontrib>Zolotarova, A. S.</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest advanced technologies & aerospace journals</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><jtitle>The European physical journal. C, Particles and fields</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Augier, C.</au><au>Barabash, A. S.</au><au>Bellini, F.</au><au>Benato, G.</au><au>Beretta, M.</au><au>Bergé, L.</au><au>Billard, J.</au><au>Borovlev, Yu. A.</au><au>Cardani, L.</au><au>Casali, N.</au><au>Cazes, A.</au><au>Chapellier, M.</au><au>Chiesa, D.</au><au>Dafinei, I.</au><au>Danevich, F. A.</au><au>De Jesus, M.</au><au>de Marcillac, P.</au><au>Dixon, T.</au><au>Dumoulin, L.</au><au>Eitel, K.</au><au>Ferri, F.</au><au>Fujikawa, B. K.</au><au>Gascon, J.</au><au>Gironi, L.</au><au>Giuliani, A.</au><au>Grigorieva, V. D.</au><au>Gros, M.</au><au>Helis, D. L.</au><au>Huang, H. Z.</au><au>Huang, R.</au><au>Imbert, L.</au><au>Johnston, J.</au><au>Juillard, A.</au><au>Khalife, H.</au><au>Kleifges, M.</au><au>Kobychev, V. V.</au><au>Kolomensky, Yu. G.</au><au>Konovalov, S. I.</au><au>Loaiza, P.</au><au>Ma, L.</au><au>Makarov, E. P.</au><au>Mariam, R.</au><au>Marini, L.</au><au>Marnieros, S.</au><au>Navick, X.-F.</au><au>Nones, C.</au><au>Norman, E. B.</au><au>Olivieri, E.</au><au>Ouellet, J. L.</au><au>Pagnanini, L.</au><au>Pattavina, L.</au><au>Paul, B.</au><au>Pavan, M.</au><au>Peng, H.</au><au>Pessina, G.</au><au>Pirro, S.</au><au>Poda, D. V.</au><au>Polischuk, O. G.</au><au>Pozzi, S.</au><au>Previtali, E.</au><au>Redon, Th</au><au>Rojas, A.</au><au>Rozov, S.</au><au>Sanglard, V.</au><au>Scarpaci, J. A.</au><au>Schmidt, B.</au><au>Shen, Y.</au><au>Shlegel, V. N.</au><au>Singh, V.</au><au>Tomei, C.</au><au>Tretyak, V. I.</au><au>Umatov, V. I.</au><au>Vagneron, L.</au><au>Velázquez, M.</au><au>Welliver, B.</au><au>Winslow, L.</au><au>Xue, M.</au><au>Yakushev, E.</au><au>Zarytskyy, M.</au><au>Zolotarova, A. S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Final results on the 0νββ decay half-life limit of 100Mo from the CUPID-Mo experiment</atitle><jtitle>The European physical journal. C, Particles and fields</jtitle><stitle>Eur. Phys. J. C</stitle><date>2022-11-15</date><risdate>2022</risdate><volume>82</volume><issue>11</issue><spage>1033</spage><pages>1033-</pages><issn>1434-6044</issn><eissn>1434-6052</eissn><abstract>The CUPID-Mo experiment to search for 0
ν
β
β
decay in
100
Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0
ν
β
β
decay experiment. CUPID-Mo was comprised of 20 enriched
Li
2
100
MoO
4
scintillating calorimeters, each with a mass of
∼
0.2
kg, operated at
∼
20
mK. We present here the final analysis with the full exposure of CUPID-Mo (
100
Mo exposure of 1.47
kg
×
year
) used to search for lepton number violation via 0
ν
β
β
decay. We report on various analysis improvements since the previous result on a subset of data, reprocessing all data with these new techniques. We observe zero events in the region of interest and set a new limit on the
100
Mo 0
ν
β
β
decay half-life of
T
1
/
2
0
ν
>
1.8
×
10
24
year (stat. + syst.) at 90% CI. Under the light Majorana neutrino exchange mechanism this corresponds to an effective Majorana neutrino mass of
m
β
β
<
(
0.28
-
0.49
)
eV, dependent upon the nuclear matrix element utilized.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1140/epjc/s10052-022-10942-5</doi><orcidid>https://orcid.org/0000-0002-0515-3773</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1434-6044 |
ispartof | The European physical journal. C, Particles and fields, 2022-11, Vol.82 (11), p.1033 |
issn | 1434-6044 1434-6052 |
language | eng |
recordid | cdi_proquest_journals_2736485035 |
source | Publicly Available Content Database; Springer Nature - SpringerLink Journals - Fully Open Access |
subjects | Astronomy Astrophysics and Cosmology Decay Elementary Particles Experiments Hadrons Half-life Heavy Ions Leptons Measurement Science and Instrumentation Neutrinos Nuclear Energy Nuclear Physics Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Regular Article - Experimental Physics Reprocessing String Theory |
title | Final results on the 0νββ decay half-life limit of 100Mo from the CUPID-Mo experiment |
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