Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe
Abstract The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $$^{136}$$ 136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target of a time projection chamber which thus contains...
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| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2020-09-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-020-8196-z |
| _version_ | 1818846135198941184 |
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| author | F. Agostini S. E. M. Ahmed Maouloud L. Althueser F. Amaro B. Antunovic E. Aprile L. Baudis D. Baur Y. Biondi A. Bismark P. A. Breur A. Brown G. Bruno R. Budnik C. Capelli J. Cardoso D. Cichon M. Clark A. P. Colijn J. J. Cuenca-García J. P. Cussonneau M. P. Decowski A. Depoian J. Dierle P. Di Gangi A. Di Giovanni S. Diglio J. M. F. dos Santos G. Drexlin K. Eitel R. Engel A. D. Ferella H. Fischer M. Galloway F. Gao F. Girard F. Glück L. Grandi R. Größle R. Gumbsheimer S. Hansmann-Menzemer F. Jörg G. Khundzakishvili A. Kopec F. Kuger L. M. Krauss H. Landsman R. F. Lang S. Lindemann M. Lindner J. A. M. Lopes A. Loya Villalpando C. Macolino A. Manfredini T. Marrodán Undagoitia J. Masbou E. Masson P. Meinhardt S. Milutinovic A. Molinario C. M. B. Monteiro M. Murra U. G. Oberlack M. Pandurovic R. Peres J. Pienaar M. Pierre V. Pizzella J. Qin D. Ramírez García S. Reichard N. Rupp P. Sanchez-Lucas G. Sartorelli D. Schulte M. Schumann L. Scotto Lavina M. Selvi M. Silva H. Simgen M. Steidl A. Terliuk C. Therreau D. Thers K. Thieme R. Trotta C. D. Tunnell K. Valerius G. Volta D. Vorkapic C. Weinheimer C. Wittweg J. Wolf J. P. Zopounidis K. Zuber DARWIN Collaboration |
| author_facet | F. Agostini S. E. M. Ahmed Maouloud L. Althueser F. Amaro B. Antunovic E. Aprile L. Baudis D. Baur Y. Biondi A. Bismark P. A. Breur A. Brown G. Bruno R. Budnik C. Capelli J. Cardoso D. Cichon M. Clark A. P. Colijn J. J. Cuenca-García J. P. Cussonneau M. P. Decowski A. Depoian J. Dierle P. Di Gangi A. Di Giovanni S. Diglio J. M. F. dos Santos G. Drexlin K. Eitel R. Engel A. D. Ferella H. Fischer M. Galloway F. Gao F. Girard F. Glück L. Grandi R. Größle R. Gumbsheimer S. Hansmann-Menzemer F. Jörg G. Khundzakishvili A. Kopec F. Kuger L. M. Krauss H. Landsman R. F. Lang S. Lindemann M. Lindner J. A. M. Lopes A. Loya Villalpando C. Macolino A. Manfredini T. Marrodán Undagoitia J. Masbou E. Masson P. Meinhardt S. Milutinovic A. Molinario C. M. B. Monteiro M. Murra U. G. Oberlack M. Pandurovic R. Peres J. Pienaar M. Pierre V. Pizzella J. Qin D. Ramírez García S. Reichard N. Rupp P. Sanchez-Lucas G. Sartorelli D. Schulte M. Schumann L. Scotto Lavina M. Selvi M. Silva H. Simgen M. Steidl A. Terliuk C. Therreau D. Thers K. Thieme R. Trotta C. D. Tunnell K. Valerius G. Volta D. Vorkapic C. Weinheimer C. Wittweg J. Wolf J. P. Zopounidis K. Zuber DARWIN Collaboration |
| author_sort | F. Agostini |
| collection | DOAJ |
| description | Abstract The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $$^{136}$$ 136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target of a time projection chamber which thus contains about 3.6 t of $$^{136}$$ 136 Xe. Here, we show that its projected half-life sensitivity is $$2.4\times {10}^{27}\,{\hbox {year}}$$ 2.4×1027year , using a fiducial volume of 5 t of natural xenon and 10 year of operation with a background rate of less than 0.2 events/(t $$\cdot $$ · year) in the energy region of interest. This sensitivity is based on a detailed Monte Carlo simulation study of the background and event topologies in the large, homogeneous target. DARWIN will be comparable in its science reach to dedicated double beta decay experiments using xenon enriched in $$^{136}$$ 136 Xe. |
| first_indexed | 2024-12-19T05:40:44Z |
| format | Article |
| id | doaj.art-8578e145f1c346b2ac06e5a732969a72 |
| institution | Directory Open Access Journal |
| issn | 1434-6044 1434-6052 |
| language | English |
| last_indexed | 2024-12-19T05:40:44Z |
| publishDate | 2020-09-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | European Physical Journal C: Particles and Fields |
| spelling | doaj.art-8578e145f1c346b2ac06e5a732969a722022-12-21T20:34:01ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-09-0180911110.1140/epjc/s10052-020-8196-zSensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 XeF. Agostini0S. E. M. Ahmed Maouloud1L. Althueser2F. Amaro3B. Antunovic4E. Aprile5L. Baudis6D. Baur7Y. Biondi8A. Bismark9P. A. Breur10A. Brown11G. Bruno12R. Budnik13C. Capelli14J. Cardoso15D. Cichon16M. Clark17A. P. Colijn18J. J. Cuenca-García19J. P. Cussonneau20M. P. Decowski21A. Depoian22J. Dierle23P. Di Gangi24A. Di Giovanni25S. Diglio26J. M. F. dos Santos27G. Drexlin28K. Eitel29R. Engel30A. D. Ferella31H. Fischer32M. Galloway33F. Gao34F. Girard35F. Glück36L. Grandi37R. Größle38R. Gumbsheimer39S. Hansmann-Menzemer40F. Jörg41G. Khundzakishvili42A. Kopec43F. Kuger44L. M. Krauss45H. Landsman46R. F. Lang47S. Lindemann48M. Lindner49J. A. M. Lopes50A. Loya Villalpando51C. Macolino52A. Manfredini53T. Marrodán Undagoitia54J. Masbou55E. Masson56P. Meinhardt57S. Milutinovic58A. Molinario59C. M. B. Monteiro60M. Murra61U. G. Oberlack62M. Pandurovic63R. Peres64J. Pienaar65M. Pierre66V. Pizzella67J. Qin68D. Ramírez García69S. Reichard70N. Rupp71P. Sanchez-Lucas72G. Sartorelli73D. Schulte74M. Schumann75L. Scotto Lavina76M. Selvi77M. Silva78H. Simgen79M. Steidl80A. Terliuk81C. Therreau82D. Thers83K. Thieme84R. Trotta85C. D. Tunnell86K. Valerius87G. Volta88D. Vorkapic89C. Weinheimer90C. Wittweg91J. Wolf92J. P. Zopounidis93K. Zuber94DARWIN CollaborationDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaLPNHE, Université Pierre et Marie Curie, Université Paris Diderot, CNRS/IN2P3Institut für Kernphysik, Westfälische Wilhelms-Universität MünsterLIBPhys, Department of Physics, University of CoimbraVinca Institute of Nuclear Science, University of BelgradePhysics Department, Columbia UniversityPhysik-Institut, University of ZurichPhysikalisches Institut, Universität FreiburgPhysik-Institut, University of ZurichPhysik-Institut, University of ZurichNikhef and the University of Amsterdam, Science ParkPhysik-Institut, University of ZurichNew York University Abu DhabiDepartment of Particle Physics and Astrophysics, Weizmann Institute of SciencePhysik-Institut, University of ZurichLIBPhys, Department of Physics, University of CoimbraMax-Planck-Institut für KernphysikDepartment of Physics and Astronomy, Purdue UniversityNikhef and the University of Amsterdam, Science ParkInstitute for Nuclear Physics (IKP), Karlsruhe Institute of Technology (KIT)SUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesNikhef and the University of Amsterdam, Science ParkDepartment of Physics and Astronomy, Purdue UniversityPhysikalisches Institut, Universität FreiburgDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaNew York University Abu DhabiSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesLIBPhys, Department of Physics, University of CoimbraInstitute of Experimental Particle Physics (ETP), Karlsruhe Institute of Technology (KIT)Institute for Nuclear Physics (IKP), Karlsruhe Institute of Technology (KIT)Institute for Nuclear Physics (IKP), Karlsruhe Institute of Technology (KIT)Department of Physics and Chemistry, University of L’AquilaPhysikalisches Institut, Universität FreiburgPhysik-Institut, University of ZurichPhysics Department, Columbia UniversityPhysik-Institut, University of ZurichInstitute for Nuclear Physics (IKP), Karlsruhe Institute of Technology (KIT)Department of Physics & Kavli Institute for Cosmological Physics, University of ChicagoInstitute for Nuclear Physics (IKP), Karlsruhe Institute of Technology (KIT)Institute for Nuclear Physics (IKP), Karlsruhe Institute of Technology (KIT)Physikalisches Institut, Ruprecht-Karls-Universität HeidelbergMax-Planck-Institut für KernphysikDepartment of Physics and Astronomy, Purdue UniversityDepartment of Physics and Astronomy, Purdue UniversityPhysikalisches Institut, Universität FreiburgThe Origins Project FoundationDepartment of Particle Physics and Astrophysics, Weizmann Institute of ScienceDepartment of Physics and Astronomy, Purdue UniversityPhysikalisches Institut, Universität FreiburgMax-Planck-Institut für KernphysikLIBPhys, Department of Physics, University of CoimbraNikhef and the University of Amsterdam, Science ParkUniversité Paris-Saclay, CNRS/IN2P3, IJCLabPhysik-Institut, University of ZurichMax-Planck-Institut für KernphysikSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesUniversité Paris-Saclay, CNRS/IN2P3, IJCLabPhysikalisches Institut, Universität FreiburgVinca Institute of Nuclear Science, University of BelgradeINFN-Laboratori Nazionali del Gran Sasso and Gran Sasso Science InstituteLIBPhys, Department of Physics, University of CoimbraInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterInstitut für Physik & Exzellenzcluster PRISMA+, Johannes Gutenberg-Universität MainzVinca Institute of Nuclear Science, University of BelgradePhysik-Institut, University of ZurichDepartment of Physics & Kavli Institute for Cosmological Physics, University of ChicagoSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesMax-Planck-Institut für KernphysikDepartment of Physics and Astronomy, Purdue UniversityPhysikalisches Institut, Universität FreiburgPhysik-Institut, University of ZurichMax-Planck-Institut für KernphysikPhysikalisches Institut, Universität FreiburgDepartment of Physics and Astronomy, University of Bologna and INFN-BolognaInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterPhysikalisches Institut, Universität FreiburgLPNHE, Université Pierre et Marie Curie, Université Paris Diderot, CNRS/IN2P3Department of Physics and Astronomy, University of Bologna and INFN-BolognaLIBPhys, Department of Physics, University of CoimbraMax-Planck-Institut für KernphysikInstitute for Nuclear Physics (IKP), Karlsruhe Institute of Technology (KIT)Physikalisches Institut, Ruprecht-Karls-Universität HeidelbergSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesSUBATECH, IMT Atlantique, CNRS/IN2P3, Université de NantesPhysik-Institut, University of ZurichDepartment of Physics, Imperial Centre for Inference and Cosmology, Imperial College LondonDepartment of Physics and Astronomy, Rice UniversityInstitute for Nuclear Physics (IKP), Karlsruhe Institute of Technology (KIT)Physik-Institut, University of ZurichVinca Institute of Nuclear Science, University of BelgradeInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterInstitute of Experimental Particle Physics (ETP), Karlsruhe Institute of Technology (KIT)LPNHE, Université Pierre et Marie Curie, Université Paris Diderot, CNRS/IN2P3Institute for Nuclear and Particle Physics, TU DresdenAbstract The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $$^{136}$$ 136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target of a time projection chamber which thus contains about 3.6 t of $$^{136}$$ 136 Xe. Here, we show that its projected half-life sensitivity is $$2.4\times {10}^{27}\,{\hbox {year}}$$ 2.4×1027year , using a fiducial volume of 5 t of natural xenon and 10 year of operation with a background rate of less than 0.2 events/(t $$\cdot $$ · year) in the energy region of interest. This sensitivity is based on a detailed Monte Carlo simulation study of the background and event topologies in the large, homogeneous target. DARWIN will be comparable in its science reach to dedicated double beta decay experiments using xenon enriched in $$^{136}$$ 136 Xe.http://link.springer.com/article/10.1140/epjc/s10052-020-8196-z |
| spellingShingle | F. Agostini S. E. M. Ahmed Maouloud L. Althueser F. Amaro B. Antunovic E. Aprile L. Baudis D. Baur Y. Biondi A. Bismark P. A. Breur A. Brown G. Bruno R. Budnik C. Capelli J. Cardoso D. Cichon M. Clark A. P. Colijn J. J. Cuenca-García J. P. Cussonneau M. P. Decowski A. Depoian J. Dierle P. Di Gangi A. Di Giovanni S. Diglio J. M. F. dos Santos G. Drexlin K. Eitel R. Engel A. D. Ferella H. Fischer M. Galloway F. Gao F. Girard F. Glück L. Grandi R. Größle R. Gumbsheimer S. Hansmann-Menzemer F. Jörg G. Khundzakishvili A. Kopec F. Kuger L. M. Krauss H. Landsman R. F. Lang S. Lindemann M. Lindner J. A. M. Lopes A. Loya Villalpando C. Macolino A. Manfredini T. Marrodán Undagoitia J. Masbou E. Masson P. Meinhardt S. Milutinovic A. Molinario C. M. B. Monteiro M. Murra U. G. Oberlack M. Pandurovic R. Peres J. Pienaar M. Pierre V. Pizzella J. Qin D. Ramírez García S. Reichard N. Rupp P. Sanchez-Lucas G. Sartorelli D. Schulte M. Schumann L. Scotto Lavina M. Selvi M. Silva H. Simgen M. Steidl A. Terliuk C. Therreau D. Thers K. Thieme R. Trotta C. D. Tunnell K. Valerius G. Volta D. Vorkapic C. Weinheimer C. Wittweg J. Wolf J. P. Zopounidis K. Zuber DARWIN Collaboration Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe European Physical Journal C: Particles and Fields |
| title | Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe |
| title_full | Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe |
| title_fullStr | Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe |
| title_full_unstemmed | Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe |
| title_short | Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$ 136 Xe |
| title_sort | sensitivity of the darwin observatory to the neutrinoless double beta decay of 136 136 xe |
| url | http://link.springer.com/article/10.1140/epjc/s10052-020-8196-z |
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