European Physical Journal C: Particles and Fields (Jul 2025)
Search for the in-situ production of $$^{77}$$ 77 Ge in the GERDA neutrinoless double-beta decay experiment
- M. Agostini,
- A. Alexander,
- G. Araujo,
- A. M. Bakalyarov,
- M. Balata,
- I. Barabanov,
- L. Baudis,
- C. Bauer,
- S. Belogurov,
- A. Bettini,
- L. Bezrukov,
- V. Biancacci,
- E. Bossio,
- V. Bothe,
- R. Brugnera,
- A. Caldwell,
- S. Calgaro,
- C. Cattadori,
- A. Chernogorov,
- P.-J. Chiu,
- T. Comellato,
- V. D’Andrea,
- E. V. Demidova,
- N. Di Marco,
- E. Doroshkevich,
- M. Fomina,
- A. Gangapshev,
- A. Garfagnini,
- C. Gooch,
- P. Grabmayr,
- V. Gurentsov,
- K. Gusev,
- J. Hakenmüller,
- S. Hemmer,
- W. Hofmann,
- J. Huang,
- M. Hult,
- L. V. Inzhechik,
- J. Janicskó Csáthy,
- J. Jochum,
- M. Junker,
- V. Kazalov,
- Y. Kermaïdic,
- H. Khushbakht,
- T. Kihm,
- K. Kilgus,
- I. V. Kirpichnikov,
- A. Klimenko,
- K. T. Knöpfle,
- O. Kochetov,
- V. N. Kornoukhov,
- P. Krause,
- V. V. Kuzminov,
- M. Laubenstein,
- M. Lindner,
- I. Lippi,
- A. Lubashevskiy,
- B. Lubsandorzhiev,
- G. Lutter,
- C. Macolino,
- B. Majorovits,
- W. Maneschg,
- G. Marshall,
- M. Misiaszek,
- M. Morella,
- Y. Müller,
- I. Nemchenok,
- M. Neuberger,
- L. Pandola,
- K. Pelczar,
- L. Pertoldi,
- P. Piseri,
- A. Pullia,
- C. Ransom,
- L. Rauscher,
- M. Redchuk,
- S. Riboldi,
- N. Rumyantseva,
- C. Sada,
- S. Sailer,
- F. Salamida,
- S. Schönert,
- J. Schreiner,
- A.-K. Schütz,
- O. Schulz,
- M. Schwarz,
- B. Schwingenheuer,
- O. Selivanenko,
- E. Shevchik,
- M. Shirchenko,
- L. Shtembari,
- H. Simgen,
- A. Smolnikov,
- D. Stukov,
- S. Sullivan,
- A. A. Vasenko,
- A. Veresnikova,
- C. Vignoli,
- K. von Sturm,
- T. Wester,
- C. Wiesinger,
- M. Wojcik,
- E. Yanovich,
- B. Zatschler,
- I. Zhitnikov,
- S. V. Zhukov,
- D. Zinatulina,
- A. Zschocke,
- K. Zuber,
- G. Zuzel,
- GERDA collaboration
Affiliations
- M. Agostini
- Department of Physics and Astronomy, University College London
- A. Alexander
- Department of Physics and Astronomy, University College London
- G. Araujo
- Physik-Institut, Universität Zürich
- A. M. Bakalyarov
- National Research Centre “Kurchatov Institute”
- M. Balata
- INFN Laboratori Nazionali del Gran Sasso
- I. Barabanov
- Institute for Nuclear Research, Russian Academy of Sciences
- L. Baudis
- Physik-Institut, Universität Zürich
- C. Bauer
- Max-Planck-Institut für Kernphysik
- S. Belogurov
- Institute for Nuclear Research, Russian Academy of Sciences
- A. Bettini
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova
- L. Bezrukov
- Institute for Nuclear Research, Russian Academy of Sciences
- V. Biancacci
- INFN Laboratori Nazionali del Gran Sasso and Università degli Studi dell’Aquila
- E. Bossio
- Physik Department, Technische Universität München
- V. Bothe
- Max-Planck-Institut für Kernphysik
- R. Brugnera
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova
- A. Caldwell
- Max-Planck-Institut für Physik
- S. Calgaro
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova
- C. Cattadori
- INFN Milano Bicocca
- A. Chernogorov
- Institute for Theoretical and Experimental Physics, NRC “Kurchatov Institute”
- P.-J. Chiu
- Physik-Institut, Universität Zürich
- T. Comellato
- Physik Department, Technische Universität München
- V. D’Andrea
- INFN Laboratori Nazionali del Gran Sasso and Università degli Studi dell’Aquila
- E. V. Demidova
- Institute for Theoretical and Experimental Physics, NRC “Kurchatov Institute”
- N. Di Marco
- INFN Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- E. Doroshkevich
- Institute for Nuclear Research, Russian Academy of Sciences
- M. Fomina
- Joint Institute for Nuclear Research
- A. Gangapshev
- Max-Planck-Institut für Kernphysik
- A. Garfagnini
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova
- C. Gooch
- Max-Planck-Institut für Physik
- P. Grabmayr
- Physikalisches Institut, Eberhard Karls Universität Tübingen
- V. Gurentsov
- Institute for Nuclear Research, Russian Academy of Sciences
- K. Gusev
- Joint Institute for Nuclear Research
- J. Hakenmüller
- Max-Planck-Institut für Kernphysik
- S. Hemmer
- INFN Padova
- W. Hofmann
- Max-Planck-Institut für Kernphysik
- J. Huang
- Physik-Institut, Universität Zürich
- M. Hult
- European Commission, JRC-Geel
- L. V. Inzhechik
- Institute for Nuclear Research, Russian Academy of Sciences
- J. Janicskó Csáthy
- Physik Department, Technische Universität München
- J. Jochum
- Physikalisches Institut, Eberhard Karls Universität Tübingen
- M. Junker
- INFN Laboratori Nazionali del Gran Sasso
- V. Kazalov
- Institute for Nuclear Research, Russian Academy of Sciences
- Y. Kermaïdic
- Max-Planck-Institut für Kernphysik
- H. Khushbakht
- Physikalisches Institut, Eberhard Karls Universität Tübingen
- T. Kihm
- Max-Planck-Institut für Kernphysik
- K. Kilgus
- Physikalisches Institut, Eberhard Karls Universität Tübingen
- I. V. Kirpichnikov
- Institute for Theoretical and Experimental Physics, NRC “Kurchatov Institute”
- A. Klimenko
- Joint Institute for Nuclear Research
- K. T. Knöpfle
- Max-Planck-Institut für Kernphysik
- O. Kochetov
- Joint Institute for Nuclear Research
- V. N. Kornoukhov
- Institute for Nuclear Research, Russian Academy of Sciences
- P. Krause
- Physik Department, Technische Universität München
- V. V. Kuzminov
- Institute for Nuclear Research, Russian Academy of Sciences
- M. Laubenstein
- INFN Laboratori Nazionali del Gran Sasso
- M. Lindner
- Max-Planck-Institut für Kernphysik
- I. Lippi
- INFN Padova
- A. Lubashevskiy
- Joint Institute for Nuclear Research
- B. Lubsandorzhiev
- Institute for Nuclear Research, Russian Academy of Sciences
- G. Lutter
- European Commission, JRC-Geel
- C. Macolino
- INFN Laboratori Nazionali del Gran Sasso and Università degli Studi dell’Aquila
- B. Majorovits
- Max-Planck-Institut für Physik
- W. Maneschg
- Max-Planck-Institut für Kernphysik
- G. Marshall
- Department of Physics and Astronomy, University College London
- M. Misiaszek
- Institute of Physics, Jagiellonian University
- M. Morella
- INFN Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute
- Y. Müller
- Physik-Institut, Universität Zürich
- I. Nemchenok
- Joint Institute for Nuclear Research
- M. Neuberger
- Physik Department, Technische Universität München
- L. Pandola
- INFN Laboratori Nazionali del Sud
- K. Pelczar
- European Commission, JRC-Geel
- L. Pertoldi
- Physik Department, Technische Universität München
- P. Piseri
- Dipartimento di Fisica, Università degli Studi di Milano, INFN Milano
- A. Pullia
- Dipartimento di Fisica, Università degli Studi di Milano, INFN Milano
- C. Ransom
- Physik-Institut, Universität Zürich
- L. Rauscher
- Physikalisches Institut, Eberhard Karls Universität Tübingen
- M. Redchuk
- INFN Padova
- S. Riboldi
- Dipartimento di Fisica, Università degli Studi di Milano, INFN Milano
- N. Rumyantseva
- Joint Institute for Nuclear Research
- C. Sada
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova
- S. Sailer
- Max-Planck-Institut für Kernphysik
- F. Salamida
- INFN Laboratori Nazionali del Gran Sasso and Università degli Studi dell’Aquila
- S. Schönert
- Physik Department, Technische Universität München
- J. Schreiner
- Max-Planck-Institut für Kernphysik
- A.-K. Schütz
- Physikalisches Institut, Eberhard Karls Universität Tübingen
- O. Schulz
- Max-Planck-Institut für Physik
- M. Schwarz
- Physik Department, Technische Universität München
- B. Schwingenheuer
- Max-Planck-Institut für Kernphysik
- O. Selivanenko
- Institute for Nuclear Research, Russian Academy of Sciences
- E. Shevchik
- Joint Institute for Nuclear Research
- M. Shirchenko
- Joint Institute for Nuclear Research
- L. Shtembari
- Max-Planck-Institut für Physik
- H. Simgen
- Max-Planck-Institut für Kernphysik
- A. Smolnikov
- Joint Institute for Nuclear Research
- D. Stukov
- National Research Centre “Kurchatov Institute”
- S. Sullivan
- Max-Planck-Institut für Kernphysik
- A. A. Vasenko
- Institute for Theoretical and Experimental Physics, NRC “Kurchatov Institute”
- A. Veresnikova
- Institute for Nuclear Research, Russian Academy of Sciences
- C. Vignoli
- INFN Laboratori Nazionali del Gran Sasso
- K. von Sturm
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova
- T. Wester
- Institut für Kern- und Teilchenphysik, Technische Universität Dresden
- C. Wiesinger
- Physik Department, Technische Universität München
- M. Wojcik
- Institute of Physics, Jagiellonian University
- E. Yanovich
- Institute for Nuclear Research, Russian Academy of Sciences
- B. Zatschler
- Institut für Kern- und Teilchenphysik, Technische Universität Dresden
- I. Zhitnikov
- Joint Institute for Nuclear Research
- S. V. Zhukov
- National Research Centre “Kurchatov Institute”
- D. Zinatulina
- Joint Institute for Nuclear Research
- A. Zschocke
- Physikalisches Institut, Eberhard Karls Universität Tübingen
- K. Zuber
- Institut für Kern- und Teilchenphysik, Technische Universität Dresden
- G. Zuzel
- Institute of Physics, Jagiellonian University
- GERDA collaboration
- Department of Physics and Astronomy, University College London
- DOI
- https://doi.org/10.1140/epjc/s10052-025-14445-x
- Journal volume & issue
-
Vol. 85,
no. 7
pp. 1 – 10
Abstract
Abstract The beta decay of $$^{77}$$ 77 Ge and $$^{77\textrm{m}}$$ 77 m Ge, both produced by neutron capture on $$^{76}$$ 76 Ge, is a potential background for Germanium based neutrinoless double-beta decay search experiments such as GERDA or the LEGEND experiment. In this work we present a search for $$^{77}$$ 77 Ge decays in the full GERDA Phase II data set. A delayed coincidence method was employed to identify the decay of $$^{77}$$ 77 Ge via the isomeric state of $$^{77}$$ 77 As ( $$9/2^+$$ 9 / 2 + , $${475}\,\hbox {keV}$$ 475 keV , $${T_{1/2} = {114}\,{\upmu }\hbox {s}}$$ T 1 / 2 = 114 μ s , $$^{77\textrm{m}}$$ 77 m As). New digital signal processing methods were employed to select and analyze pile-up signals. No signal was observed, and an upper limit on the production rate of $$^{77}$$ 77 Ge was set at $$<0.216$$ < 0.216 nuc/(kg $$\cdot $$ · yr) (90% CL). This corresponds to a total production rate of $$^{77}$$ 77 Ge and $$^{77\textrm{m}}$$ 77 m Ge of $$<{0.38}$$ < 0.38 nuc/(kg $$\cdot $$ · yr) (90% CL), assuming equal production rates. A previous Monte Carlo study predicted a value for in-situ $$^{77}$$ 77 Ge and $$^{77\textrm{m}}$$ 77 m Ge production of (0.21 ± 0.07) nuc/(kg.yr), a prediction that is now further corroborated by our experimental limit. Moreover, tagging the isomeric state of $$^{77\textrm{m}}$$ 77 m As can be utilised to further suppress the $$^{77}$$ 77 Ge background. Considering the similar experimental configurations of LEGEND-1000 and GERDA, the cosmogenic background in LEGEND-1000 at LNGS is estimated to remain at a sub-dominant level.