Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment
Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
R. Arnold [verfasserIn] C. Augier [verfasserIn] A. S. Barabash [verfasserIn] A. Basharina-Freshville [verfasserIn] S. Blondel [verfasserIn] S. Blot [verfasserIn] M. Bongrand [verfasserIn] D. Boursette [verfasserIn] V. Brudanin [verfasserIn] J. Busto [verfasserIn] A. J. Caffrey [verfasserIn] S. Calvez [verfasserIn] M. Cascella [verfasserIn] C. Cerna [verfasserIn] J. P. Cesar [verfasserIn] A. Chapon [verfasserIn] E. Chauveau [verfasserIn] A. Chopra [verfasserIn] L. Dawson [verfasserIn] D. Duchesneau [verfasserIn] D. Durand [verfasserIn] V. Egorov [verfasserIn] G. Eurin [verfasserIn] J. J. Evans [verfasserIn] L. Fajt [verfasserIn] D. Filosofov [verfasserIn] R. Flack [verfasserIn] X. Garrido [verfasserIn] H. Gómez [verfasserIn] B. Guillon [verfasserIn] P. Guzowski [verfasserIn] R. Hodák [verfasserIn] A. Huber [verfasserIn] P. Hubert [verfasserIn] C. Hugon [verfasserIn] S. Jullian [verfasserIn] A. Klimenko [verfasserIn] O. Kochetov [verfasserIn] S. I. Konovalov [verfasserIn] V. Kovalenko [verfasserIn] D. Lalanne [verfasserIn] K. Lang [verfasserIn] Y. Lemière [verfasserIn] T. Le Noblet [verfasserIn] Z. Liptak [verfasserIn] X. R. Liu [verfasserIn] P. Loaiza [verfasserIn] G. Lutter [verfasserIn] C. Macolino [verfasserIn] F. Mamedov [verfasserIn] C. Marquet [verfasserIn] F. Mauger [verfasserIn] B. Morgan [verfasserIn] J. Mott [verfasserIn] I. Nemchenok [verfasserIn] M. Nomachi [verfasserIn] F. Nova [verfasserIn] F. Nowacki [verfasserIn] H. Ohsumi [verfasserIn] R. B. Pahlka [verfasserIn] C. Patrick [verfasserIn] F. Perrot [verfasserIn] F. Piquemal [verfasserIn] P. Povinec [verfasserIn] P. Přidal [verfasserIn] Y. A. Ramachers [verfasserIn] A. Remoto [verfasserIn] J. L. Reyss [verfasserIn] C. L. Riddle [verfasserIn] E. Rukhadze [verfasserIn] N. I. Rukhadze [verfasserIn] R. Saakyan [verfasserIn] R. Salazar [verfasserIn] X. Sarazin [verfasserIn] Yu. Shitov [verfasserIn] L. Simard [verfasserIn] F. Šimkovic [verfasserIn] A. Smetana [verfasserIn] K. Smolek [verfasserIn] A. Smolnikov [verfasserIn] S. Söldner-Rembold [verfasserIn] B. Soulé [verfasserIn] I. Štekl [verfasserIn] J. Suhonen [verfasserIn] C. S. Sutton [verfasserIn] G. Szklarz [verfasserIn] J. Thomas [verfasserIn] V. Timkin [verfasserIn] S. Torre [verfasserIn] Vl. I. Tretyak [verfasserIn] V. I. Tretyak [verfasserIn] V. I. Umatov [verfasserIn] I. Vanushin [verfasserIn] C. Vilela [verfasserIn] V. Vorobel [verfasserIn] D. Waters [verfasserIn] F. Xie [verfasserIn] A. Žukauskas [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2018 |
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| Übergeordnetes Werk: |
In: European Physical Journal C: Particles and Fields - SpringerOpen, 2017, 78(2018), 10, Seite 15 |
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| Übergeordnetes Werk: |
volume:78 ; year:2018 ; number:10 ; pages:15 |
| Links: |
Link aufrufen |
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| DOI / URN: |
10.1140/epjc/s10052-018-6295-x |
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| Katalog-ID: |
DOAJ074180428 |
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| 245 | 1 | 0 | |a Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment |
| 264 | 1 | |c 2018 | |
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| 337 | |a Computermedien |b c |2 rdamedia | ||
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| 520 | |a Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. | ||
| 653 | 0 | |a Astrophysics | |
| 653 | 0 | |a Nuclear and particle physics. Atomic energy. Radioactivity | |
| 700 | 0 | |a C. Augier |e verfasserin |4 aut | |
| 700 | 0 | |a A. S. Barabash |e verfasserin |4 aut | |
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| 700 | 0 | |a D. Boursette |e verfasserin |4 aut | |
| 700 | 0 | |a V. Brudanin |e verfasserin |4 aut | |
| 700 | 0 | |a J. Busto |e verfasserin |4 aut | |
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| 700 | 0 | |a S. Calvez |e verfasserin |4 aut | |
| 700 | 0 | |a M. Cascella |e verfasserin |4 aut | |
| 700 | 0 | |a C. Cerna |e verfasserin |4 aut | |
| 700 | 0 | |a J. P. Cesar |e verfasserin |4 aut | |
| 700 | 0 | |a A. Chapon |e verfasserin |4 aut | |
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| 700 | 0 | |a A. Chopra |e verfasserin |4 aut | |
| 700 | 0 | |a L. Dawson |e verfasserin |4 aut | |
| 700 | 0 | |a D. Duchesneau |e verfasserin |4 aut | |
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| 700 | 0 | |a V. Egorov |e verfasserin |4 aut | |
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| 700 | 0 | |a J. J. Evans |e verfasserin |4 aut | |
| 700 | 0 | |a L. Fajt |e verfasserin |4 aut | |
| 700 | 0 | |a D. Filosofov |e verfasserin |4 aut | |
| 700 | 0 | |a R. Flack |e verfasserin |4 aut | |
| 700 | 0 | |a X. Garrido |e verfasserin |4 aut | |
| 700 | 0 | |a H. Gómez |e verfasserin |4 aut | |
| 700 | 0 | |a B. Guillon |e verfasserin |4 aut | |
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| 700 | 0 | |a S. Jullian |e verfasserin |4 aut | |
| 700 | 0 | |a A. Klimenko |e verfasserin |4 aut | |
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| 700 | 0 | |a Y. Lemière |e verfasserin |4 aut | |
| 700 | 0 | |a T. Le Noblet |e verfasserin |4 aut | |
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| 700 | 0 | |a J. Mott |e verfasserin |4 aut | |
| 700 | 0 | |a I. Nemchenok |e verfasserin |4 aut | |
| 700 | 0 | |a M. Nomachi |e verfasserin |4 aut | |
| 700 | 0 | |a F. Nova |e verfasserin |4 aut | |
| 700 | 0 | |a F. Nowacki |e verfasserin |4 aut | |
| 700 | 0 | |a H. Ohsumi |e verfasserin |4 aut | |
| 700 | 0 | |a R. B. Pahlka |e verfasserin |4 aut | |
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| 700 | 0 | |a F. Piquemal |e verfasserin |4 aut | |
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10.1140/epjc/s10052-018-6295-x doi (DE-627)DOAJ074180428 (DE-599)DOAJ495aa51a700542afae9002e1a2f17f9a DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 R. Arnold verfasserin aut Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity C. Augier verfasserin aut A. S. Barabash verfasserin aut A. Basharina-Freshville verfasserin aut S. Blondel verfasserin aut S. Blot verfasserin aut M. Bongrand verfasserin aut D. Boursette verfasserin aut V. Brudanin verfasserin aut J. Busto verfasserin aut A. J. Caffrey verfasserin aut S. Calvez verfasserin aut M. Cascella verfasserin aut C. Cerna verfasserin aut J. P. Cesar verfasserin aut A. Chapon verfasserin aut E. Chauveau verfasserin aut A. Chopra verfasserin aut L. Dawson verfasserin aut D. Duchesneau verfasserin aut D. Durand verfasserin aut V. Egorov verfasserin aut G. Eurin verfasserin aut J. J. Evans verfasserin aut L. Fajt verfasserin aut D. Filosofov verfasserin aut R. Flack verfasserin aut X. Garrido verfasserin aut H. Gómez verfasserin aut B. Guillon verfasserin aut P. Guzowski verfasserin aut R. Hodák verfasserin aut A. Huber verfasserin aut P. Hubert verfasserin aut C. Hugon verfasserin aut S. Jullian verfasserin aut A. Klimenko verfasserin aut O. Kochetov verfasserin aut S. I. Konovalov verfasserin aut V. Kovalenko verfasserin aut D. Lalanne verfasserin aut K. Lang verfasserin aut Y. Lemière verfasserin aut T. Le Noblet verfasserin aut Z. Liptak verfasserin aut X. R. Liu verfasserin aut P. Loaiza verfasserin aut G. Lutter verfasserin aut C. Macolino verfasserin aut F. Mamedov verfasserin aut C. Marquet verfasserin aut F. Mauger verfasserin aut B. Morgan verfasserin aut J. Mott verfasserin aut I. Nemchenok verfasserin aut M. Nomachi verfasserin aut F. Nova verfasserin aut F. Nowacki verfasserin aut H. Ohsumi verfasserin aut R. B. Pahlka verfasserin aut C. Patrick verfasserin aut F. Perrot verfasserin aut F. Piquemal verfasserin aut P. Povinec verfasserin aut P. Přidal verfasserin aut Y. A. Ramachers verfasserin aut A. Remoto verfasserin aut J. L. Reyss verfasserin aut C. L. Riddle verfasserin aut E. Rukhadze verfasserin aut N. I. Rukhadze verfasserin aut R. Saakyan verfasserin aut R. Salazar verfasserin aut X. Sarazin verfasserin aut Yu. Shitov verfasserin aut L. Simard verfasserin aut F. Šimkovic verfasserin aut A. Smetana verfasserin aut K. Smolek verfasserin aut A. Smolnikov verfasserin aut S. Söldner-Rembold verfasserin aut B. Soulé verfasserin aut I. Štekl verfasserin aut J. Suhonen verfasserin aut C. S. Sutton verfasserin aut G. Szklarz verfasserin aut J. Thomas verfasserin aut V. Timkin verfasserin aut S. Torre verfasserin aut Vl. I. Tretyak verfasserin aut V. I. Tretyak verfasserin aut V. I. Umatov verfasserin aut I. Vanushin verfasserin aut C. Vilela verfasserin aut V. Vorobel verfasserin aut D. Waters verfasserin aut F. Xie verfasserin aut A. Žukauskas verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 78(2018), 10, Seite 15 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:78 year:2018 number:10 pages:15 https://doi.org/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/article/495aa51a700542afae9002e1a2f17f9a kostenfrei http://link.springer.com/article/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 78 2018 10 15 |
| spelling |
10.1140/epjc/s10052-018-6295-x doi (DE-627)DOAJ074180428 (DE-599)DOAJ495aa51a700542afae9002e1a2f17f9a DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 R. Arnold verfasserin aut Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity C. Augier verfasserin aut A. S. Barabash verfasserin aut A. Basharina-Freshville verfasserin aut S. Blondel verfasserin aut S. Blot verfasserin aut M. Bongrand verfasserin aut D. Boursette verfasserin aut V. Brudanin verfasserin aut J. Busto verfasserin aut A. J. Caffrey verfasserin aut S. Calvez verfasserin aut M. Cascella verfasserin aut C. Cerna verfasserin aut J. P. Cesar verfasserin aut A. Chapon verfasserin aut E. Chauveau verfasserin aut A. Chopra verfasserin aut L. Dawson verfasserin aut D. Duchesneau verfasserin aut D. Durand verfasserin aut V. Egorov verfasserin aut G. Eurin verfasserin aut J. J. Evans verfasserin aut L. Fajt verfasserin aut D. Filosofov verfasserin aut R. Flack verfasserin aut X. Garrido verfasserin aut H. Gómez verfasserin aut B. Guillon verfasserin aut P. Guzowski verfasserin aut R. Hodák verfasserin aut A. Huber verfasserin aut P. Hubert verfasserin aut C. Hugon verfasserin aut S. Jullian verfasserin aut A. Klimenko verfasserin aut O. Kochetov verfasserin aut S. I. Konovalov verfasserin aut V. Kovalenko verfasserin aut D. Lalanne verfasserin aut K. Lang verfasserin aut Y. Lemière verfasserin aut T. Le Noblet verfasserin aut Z. Liptak verfasserin aut X. R. Liu verfasserin aut P. Loaiza verfasserin aut G. Lutter verfasserin aut C. Macolino verfasserin aut F. Mamedov verfasserin aut C. Marquet verfasserin aut F. Mauger verfasserin aut B. Morgan verfasserin aut J. Mott verfasserin aut I. Nemchenok verfasserin aut M. Nomachi verfasserin aut F. Nova verfasserin aut F. Nowacki verfasserin aut H. Ohsumi verfasserin aut R. B. Pahlka verfasserin aut C. Patrick verfasserin aut F. Perrot verfasserin aut F. Piquemal verfasserin aut P. Povinec verfasserin aut P. Přidal verfasserin aut Y. A. Ramachers verfasserin aut A. Remoto verfasserin aut J. L. Reyss verfasserin aut C. L. Riddle verfasserin aut E. Rukhadze verfasserin aut N. I. Rukhadze verfasserin aut R. Saakyan verfasserin aut R. Salazar verfasserin aut X. Sarazin verfasserin aut Yu. Shitov verfasserin aut L. Simard verfasserin aut F. Šimkovic verfasserin aut A. Smetana verfasserin aut K. Smolek verfasserin aut A. Smolnikov verfasserin aut S. Söldner-Rembold verfasserin aut B. Soulé verfasserin aut I. Štekl verfasserin aut J. Suhonen verfasserin aut C. S. Sutton verfasserin aut G. Szklarz verfasserin aut J. Thomas verfasserin aut V. Timkin verfasserin aut S. Torre verfasserin aut Vl. I. Tretyak verfasserin aut V. I. Tretyak verfasserin aut V. I. Umatov verfasserin aut I. Vanushin verfasserin aut C. Vilela verfasserin aut V. Vorobel verfasserin aut D. Waters verfasserin aut F. Xie verfasserin aut A. Žukauskas verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 78(2018), 10, Seite 15 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:78 year:2018 number:10 pages:15 https://doi.org/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/article/495aa51a700542afae9002e1a2f17f9a kostenfrei http://link.springer.com/article/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 78 2018 10 15 |
| allfields_unstemmed |
10.1140/epjc/s10052-018-6295-x doi (DE-627)DOAJ074180428 (DE-599)DOAJ495aa51a700542afae9002e1a2f17f9a DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 R. Arnold verfasserin aut Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity C. Augier verfasserin aut A. S. Barabash verfasserin aut A. Basharina-Freshville verfasserin aut S. Blondel verfasserin aut S. Blot verfasserin aut M. Bongrand verfasserin aut D. Boursette verfasserin aut V. Brudanin verfasserin aut J. Busto verfasserin aut A. J. Caffrey verfasserin aut S. Calvez verfasserin aut M. Cascella verfasserin aut C. Cerna verfasserin aut J. P. Cesar verfasserin aut A. Chapon verfasserin aut E. Chauveau verfasserin aut A. Chopra verfasserin aut L. Dawson verfasserin aut D. Duchesneau verfasserin aut D. Durand verfasserin aut V. Egorov verfasserin aut G. Eurin verfasserin aut J. J. Evans verfasserin aut L. Fajt verfasserin aut D. Filosofov verfasserin aut R. Flack verfasserin aut X. Garrido verfasserin aut H. Gómez verfasserin aut B. Guillon verfasserin aut P. Guzowski verfasserin aut R. Hodák verfasserin aut A. Huber verfasserin aut P. Hubert verfasserin aut C. Hugon verfasserin aut S. Jullian verfasserin aut A. Klimenko verfasserin aut O. Kochetov verfasserin aut S. I. Konovalov verfasserin aut V. Kovalenko verfasserin aut D. Lalanne verfasserin aut K. Lang verfasserin aut Y. Lemière verfasserin aut T. Le Noblet verfasserin aut Z. Liptak verfasserin aut X. R. Liu verfasserin aut P. Loaiza verfasserin aut G. Lutter verfasserin aut C. Macolino verfasserin aut F. Mamedov verfasserin aut C. Marquet verfasserin aut F. Mauger verfasserin aut B. Morgan verfasserin aut J. Mott verfasserin aut I. Nemchenok verfasserin aut M. Nomachi verfasserin aut F. Nova verfasserin aut F. Nowacki verfasserin aut H. Ohsumi verfasserin aut R. B. Pahlka verfasserin aut C. Patrick verfasserin aut F. Perrot verfasserin aut F. Piquemal verfasserin aut P. Povinec verfasserin aut P. Přidal verfasserin aut Y. A. Ramachers verfasserin aut A. Remoto verfasserin aut J. L. Reyss verfasserin aut C. L. Riddle verfasserin aut E. Rukhadze verfasserin aut N. I. Rukhadze verfasserin aut R. Saakyan verfasserin aut R. Salazar verfasserin aut X. Sarazin verfasserin aut Yu. Shitov verfasserin aut L. Simard verfasserin aut F. Šimkovic verfasserin aut A. Smetana verfasserin aut K. Smolek verfasserin aut A. Smolnikov verfasserin aut S. Söldner-Rembold verfasserin aut B. Soulé verfasserin aut I. Štekl verfasserin aut J. Suhonen verfasserin aut C. S. Sutton verfasserin aut G. Szklarz verfasserin aut J. Thomas verfasserin aut V. Timkin verfasserin aut S. Torre verfasserin aut Vl. I. Tretyak verfasserin aut V. I. Tretyak verfasserin aut V. I. Umatov verfasserin aut I. Vanushin verfasserin aut C. Vilela verfasserin aut V. Vorobel verfasserin aut D. Waters verfasserin aut F. Xie verfasserin aut A. Žukauskas verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 78(2018), 10, Seite 15 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:78 year:2018 number:10 pages:15 https://doi.org/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/article/495aa51a700542afae9002e1a2f17f9a kostenfrei http://link.springer.com/article/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 78 2018 10 15 |
| allfieldsGer |
10.1140/epjc/s10052-018-6295-x doi (DE-627)DOAJ074180428 (DE-599)DOAJ495aa51a700542afae9002e1a2f17f9a DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 R. Arnold verfasserin aut Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity C. Augier verfasserin aut A. S. Barabash verfasserin aut A. Basharina-Freshville verfasserin aut S. Blondel verfasserin aut S. Blot verfasserin aut M. Bongrand verfasserin aut D. Boursette verfasserin aut V. Brudanin verfasserin aut J. Busto verfasserin aut A. J. Caffrey verfasserin aut S. Calvez verfasserin aut M. Cascella verfasserin aut C. Cerna verfasserin aut J. P. Cesar verfasserin aut A. Chapon verfasserin aut E. Chauveau verfasserin aut A. Chopra verfasserin aut L. Dawson verfasserin aut D. Duchesneau verfasserin aut D. Durand verfasserin aut V. Egorov verfasserin aut G. Eurin verfasserin aut J. J. Evans verfasserin aut L. Fajt verfasserin aut D. Filosofov verfasserin aut R. Flack verfasserin aut X. Garrido verfasserin aut H. Gómez verfasserin aut B. Guillon verfasserin aut P. Guzowski verfasserin aut R. Hodák verfasserin aut A. Huber verfasserin aut P. Hubert verfasserin aut C. Hugon verfasserin aut S. Jullian verfasserin aut A. Klimenko verfasserin aut O. Kochetov verfasserin aut S. I. Konovalov verfasserin aut V. Kovalenko verfasserin aut D. Lalanne verfasserin aut K. Lang verfasserin aut Y. Lemière verfasserin aut T. Le Noblet verfasserin aut Z. Liptak verfasserin aut X. R. Liu verfasserin aut P. Loaiza verfasserin aut G. Lutter verfasserin aut C. Macolino verfasserin aut F. Mamedov verfasserin aut C. Marquet verfasserin aut F. Mauger verfasserin aut B. Morgan verfasserin aut J. Mott verfasserin aut I. Nemchenok verfasserin aut M. Nomachi verfasserin aut F. Nova verfasserin aut F. Nowacki verfasserin aut H. Ohsumi verfasserin aut R. B. Pahlka verfasserin aut C. Patrick verfasserin aut F. Perrot verfasserin aut F. Piquemal verfasserin aut P. Povinec verfasserin aut P. Přidal verfasserin aut Y. A. Ramachers verfasserin aut A. Remoto verfasserin aut J. L. Reyss verfasserin aut C. L. Riddle verfasserin aut E. Rukhadze verfasserin aut N. I. Rukhadze verfasserin aut R. Saakyan verfasserin aut R. Salazar verfasserin aut X. Sarazin verfasserin aut Yu. Shitov verfasserin aut L. Simard verfasserin aut F. Šimkovic verfasserin aut A. Smetana verfasserin aut K. Smolek verfasserin aut A. Smolnikov verfasserin aut S. Söldner-Rembold verfasserin aut B. Soulé verfasserin aut I. Štekl verfasserin aut J. Suhonen verfasserin aut C. S. Sutton verfasserin aut G. Szklarz verfasserin aut J. Thomas verfasserin aut V. Timkin verfasserin aut S. Torre verfasserin aut Vl. I. Tretyak verfasserin aut V. I. Tretyak verfasserin aut V. I. Umatov verfasserin aut I. Vanushin verfasserin aut C. Vilela verfasserin aut V. Vorobel verfasserin aut D. Waters verfasserin aut F. Xie verfasserin aut A. Žukauskas verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 78(2018), 10, Seite 15 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:78 year:2018 number:10 pages:15 https://doi.org/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/article/495aa51a700542afae9002e1a2f17f9a kostenfrei http://link.springer.com/article/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 78 2018 10 15 |
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10.1140/epjc/s10052-018-6295-x doi (DE-627)DOAJ074180428 (DE-599)DOAJ495aa51a700542afae9002e1a2f17f9a DE-627 ger DE-627 rakwb eng QB460-466 QC770-798 R. Arnold verfasserin aut Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. Astrophysics Nuclear and particle physics. Atomic energy. Radioactivity C. Augier verfasserin aut A. S. Barabash verfasserin aut A. Basharina-Freshville verfasserin aut S. Blondel verfasserin aut S. Blot verfasserin aut M. Bongrand verfasserin aut D. Boursette verfasserin aut V. Brudanin verfasserin aut J. Busto verfasserin aut A. J. Caffrey verfasserin aut S. Calvez verfasserin aut M. Cascella verfasserin aut C. Cerna verfasserin aut J. P. Cesar verfasserin aut A. Chapon verfasserin aut E. Chauveau verfasserin aut A. Chopra verfasserin aut L. Dawson verfasserin aut D. Duchesneau verfasserin aut D. Durand verfasserin aut V. Egorov verfasserin aut G. Eurin verfasserin aut J. J. Evans verfasserin aut L. Fajt verfasserin aut D. Filosofov verfasserin aut R. Flack verfasserin aut X. Garrido verfasserin aut H. Gómez verfasserin aut B. Guillon verfasserin aut P. Guzowski verfasserin aut R. Hodák verfasserin aut A. Huber verfasserin aut P. Hubert verfasserin aut C. Hugon verfasserin aut S. Jullian verfasserin aut A. Klimenko verfasserin aut O. Kochetov verfasserin aut S. I. Konovalov verfasserin aut V. Kovalenko verfasserin aut D. Lalanne verfasserin aut K. Lang verfasserin aut Y. Lemière verfasserin aut T. Le Noblet verfasserin aut Z. Liptak verfasserin aut X. R. Liu verfasserin aut P. Loaiza verfasserin aut G. Lutter verfasserin aut C. Macolino verfasserin aut F. Mamedov verfasserin aut C. Marquet verfasserin aut F. Mauger verfasserin aut B. Morgan verfasserin aut J. Mott verfasserin aut I. Nemchenok verfasserin aut M. Nomachi verfasserin aut F. Nova verfasserin aut F. Nowacki verfasserin aut H. Ohsumi verfasserin aut R. B. Pahlka verfasserin aut C. Patrick verfasserin aut F. Perrot verfasserin aut F. Piquemal verfasserin aut P. Povinec verfasserin aut P. Přidal verfasserin aut Y. A. Ramachers verfasserin aut A. Remoto verfasserin aut J. L. Reyss verfasserin aut C. L. Riddle verfasserin aut E. Rukhadze verfasserin aut N. I. Rukhadze verfasserin aut R. Saakyan verfasserin aut R. Salazar verfasserin aut X. Sarazin verfasserin aut Yu. Shitov verfasserin aut L. Simard verfasserin aut F. Šimkovic verfasserin aut A. Smetana verfasserin aut K. Smolek verfasserin aut A. Smolnikov verfasserin aut S. Söldner-Rembold verfasserin aut B. Soulé verfasserin aut I. Štekl verfasserin aut J. Suhonen verfasserin aut C. S. Sutton verfasserin aut G. Szklarz verfasserin aut J. Thomas verfasserin aut V. Timkin verfasserin aut S. Torre verfasserin aut Vl. I. Tretyak verfasserin aut V. I. Tretyak verfasserin aut V. I. Umatov verfasserin aut I. Vanushin verfasserin aut C. Vilela verfasserin aut V. Vorobel verfasserin aut D. Waters verfasserin aut F. Xie verfasserin aut A. Žukauskas verfasserin aut In European Physical Journal C: Particles and Fields SpringerOpen, 2017 78(2018), 10, Seite 15 (DE-627)253722934 (DE-600)1459069-4 14346052 nnns volume:78 year:2018 number:10 pages:15 https://doi.org/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/article/495aa51a700542afae9002e1a2f17f9a kostenfrei http://link.springer.com/article/10.1140/epjc/s10052-018-6295-x kostenfrei https://doaj.org/toc/1434-6044 Journal toc kostenfrei https://doaj.org/toc/1434-6052 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 78 2018 10 15 |
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R. Arnold @@aut@@ C. Augier @@aut@@ A. S. Barabash @@aut@@ A. Basharina-Freshville @@aut@@ S. Blondel @@aut@@ S. Blot @@aut@@ M. Bongrand @@aut@@ D. Boursette @@aut@@ V. Brudanin @@aut@@ J. Busto @@aut@@ A. J. Caffrey @@aut@@ S. Calvez @@aut@@ M. Cascella @@aut@@ C. Cerna @@aut@@ J. P. Cesar @@aut@@ A. Chapon @@aut@@ E. Chauveau @@aut@@ A. Chopra @@aut@@ L. Dawson @@aut@@ D. Duchesneau @@aut@@ D. Durand @@aut@@ V. Egorov @@aut@@ G. Eurin @@aut@@ J. J. Evans @@aut@@ L. Fajt @@aut@@ D. Filosofov @@aut@@ R. Flack @@aut@@ X. Garrido @@aut@@ H. Gómez @@aut@@ B. Guillon @@aut@@ P. Guzowski @@aut@@ R. Hodák @@aut@@ A. Huber @@aut@@ P. Hubert @@aut@@ C. Hugon @@aut@@ S. Jullian @@aut@@ A. Klimenko @@aut@@ O. Kochetov @@aut@@ S. I. Konovalov @@aut@@ V. Kovalenko @@aut@@ D. Lalanne @@aut@@ K. Lang @@aut@@ Y. Lemière @@aut@@ T. Le Noblet @@aut@@ Z. Liptak @@aut@@ X. R. Liu @@aut@@ P. Loaiza @@aut@@ G. Lutter @@aut@@ C. Macolino @@aut@@ F. Mamedov @@aut@@ C. Marquet @@aut@@ F. Mauger @@aut@@ B. Morgan @@aut@@ J. Mott @@aut@@ I. Nemchenok @@aut@@ M. Nomachi @@aut@@ F. Nova @@aut@@ F. Nowacki @@aut@@ H. Ohsumi @@aut@@ R. B. Pahlka @@aut@@ C. Patrick @@aut@@ F. Perrot @@aut@@ F. Piquemal @@aut@@ P. Povinec @@aut@@ P. Přidal @@aut@@ Y. A. Ramachers @@aut@@ A. Remoto @@aut@@ J. L. Reyss @@aut@@ C. L. Riddle @@aut@@ E. Rukhadze @@aut@@ N. I. Rukhadze @@aut@@ R. Saakyan @@aut@@ R. Salazar @@aut@@ X. Sarazin @@aut@@ Yu. Shitov @@aut@@ L. Simard @@aut@@ F. Šimkovic @@aut@@ A. Smetana @@aut@@ K. Smolek @@aut@@ A. Smolnikov @@aut@@ S. Söldner-Rembold @@aut@@ B. Soulé @@aut@@ I. Štekl @@aut@@ J. Suhonen @@aut@@ C. S. Sutton @@aut@@ G. Szklarz @@aut@@ J. Thomas @@aut@@ V. Timkin @@aut@@ S. Torre @@aut@@ Vl. I. Tretyak @@aut@@ V. I. Tretyak @@aut@@ V. I. Umatov @@aut@@ I. Vanushin @@aut@@ C. Vilela @@aut@@ V. Vorobel @@aut@@ D. Waters @@aut@@ F. Xie @@aut@@ A. Žukauskas @@aut@@ |
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Flack</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">X. Garrido</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">H. Gómez</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">B. Guillon</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">P. Guzowski</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">R. Hodák</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. Huber</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">P. Hubert</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">C. Hugon</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Jullian</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. Klimenko</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">O. Kochetov</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. I. Konovalov</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">V. Kovalenko</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">D. Lalanne</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">K. Lang</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Y. Lemière</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">T. Le Noblet</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">Z. Liptak</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">X. R. Liu</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">P. Loaiza</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">G. Lutter</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">C. Macolino</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">F. Mamedov</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">C. Marquet</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">F. Mauger</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">B. Morgan</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">J. Mott</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">I. Nemchenok</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. Nomachi</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">F. 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QB460-466 QC770-798 Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment |
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R. Arnold C. Augier A. S. Barabash A. Basharina-Freshville S. Blondel S. Blot M. Bongrand D. Boursette V. Brudanin J. Busto A. J. Caffrey S. Calvez M. Cascella C. Cerna J. P. Cesar A. Chapon E. Chauveau A. Chopra L. Dawson D. Duchesneau D. Durand V. Egorov G. Eurin J. J. Evans L. Fajt D. Filosofov R. Flack X. Garrido H. Gómez B. Guillon P. Guzowski R. Hodák A. Huber P. Hubert C. Hugon S. Jullian A. Klimenko O. Kochetov S. I. Konovalov V. Kovalenko D. Lalanne K. Lang Y. Lemière T. Le Noblet Z. Liptak X. R. Liu P. Loaiza G. Lutter C. Macolino F. Mamedov C. Marquet F. Mauger B. Morgan J. Mott I. Nemchenok M. Nomachi F. Nova F. Nowacki H. Ohsumi R. B. Pahlka C. Patrick F. Perrot F. Piquemal P. Povinec P. Přidal Y. A. Ramachers A. Remoto J. L. Reyss C. L. Riddle E. Rukhadze N. I. Rukhadze R. Saakyan R. Salazar X. Sarazin Yu. Shitov L. Simard F. Šimkovic A. Smetana K. Smolek A. Smolnikov S. Söldner-Rembold B. Soulé I. Štekl J. Suhonen C. S. Sutton G. Szklarz J. Thomas V. Timkin S. Torre Vl. I. Tretyak V. I. Tretyak V. I. Umatov I. Vanushin C. Vilela V. Vorobel D. Waters F. Xie A. Žukauskas |
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final results on $${}^\mathbf{82 }{\hbox {se}}$$ 82se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {kr}}$$ 82kr from the nemo-3 experiment |
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Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment |
| abstract |
Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. |
| abstractGer |
Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. |
| abstract_unstemmed |
Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set. |
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Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment |
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Arnold</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Final results on $${}^\mathbf{82 }{\hbox {Se}}$$ 82Se double beta decay to the ground state of $${}^\mathbf{82 }{\hbox {Kr}}$$ 82Kr from the NEMO-3 experiment</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2018</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Using data from the NEMO-3 experiment, we have measured the two-neutrino double beta decay ($$2\nu \beta \beta $$ 2νββ ) half-life of $$^{82}$$ 82 Se as $$T_{\smash {1/2}}^{2\nu } \!=\! \left[ 9.39 \pm 0.17\left( \text{ stat }\right) \pm 0.58\left( \text{ syst }\right) \right] \times 10^{19}$$ T1/22ν=9.39±0.17stat±0.58syst×1019 y under the single-state dominance hypothesis for this nuclear transition. The corresponding nuclear matrix element is $$\left| M^{2\nu }\right| = 0.0498 \pm 0.0016$$ M2ν=0.0498±0.0016 . In addition, a search for neutrinoless double beta decay ($$0\nu \beta \beta $$ 0νββ ) using 0.93 kg of $$^{82}$$ 82 Se observed for a total of 5.25 y has been conducted and no evidence for a signal has been found. The resulting half-life limit of $$T_{1/2}^{0\nu } < 2.5 \times 10^{23} \,\text{ y } \,(90\%\,\text{ C.L. })$$ T1/20ν<2.5×1023y(90%C.L.) for the light neutrino exchange mechanism leads to a constraint on the effective Majorana neutrino mass of $$\langle m_{\nu } \rangle < \left( 1.2{-}3.0\right) \,\text{ eV }$$ ⟨mν⟩<1.2-3.0eV , where the range reflects $$0\nu \beta \beta $$ 0νββ nuclear matrix element values from different calculations. Furthermore, constraints on lepton number violating parameters for other $$0\nu \beta \beta $$ 0νββ mechanisms, such as right-handed currents, majoron emission and R-parity violating supersymmetry modes have been set.</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Astrophysics</subfield></datafield><datafield tag="653" ind1=" " ind2="0"><subfield code="a">Nuclear and particle physics. Atomic energy. Radioactivity</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">C. Augier</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. S. Barabash</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">A. Basharina-Freshville</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Blondel</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">S. Blot</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">M. Bongrand</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">D. Boursette</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="0" ind2=" "><subfield code="a">V. 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| score |
7.3998823 |