European Physical Journal C: Particles and Fields (Sep 2024)
Searches for new physics below twice the electron mass with GERDA
- GERDA Collaboration,
- 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
Affiliations
- GERDA Collaboration
- Max-Planck-Institut für Kernphysik
- 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 of the Russian Academy of Sciences
- L. Baudis
- Physik-Institut, Universität Zürich
- C. Bauer
- Max-Planck-Institut für Kernphysik
- S. Belogurov
- Institute for Nuclear Research of the Russian Academy of Sciences
- A. Bettini
- Dipartimento di Fisica e Astronomia, Università degli Studi di Padova
- L. Bezrukov
- Institute for Nuclear Research of the 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 of the 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 of the 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 of the 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 of the 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 of the Russian Academy of Sciences
- P. Krause
- Physik Department, Technische Universität München
- V. V. Kuzminov
- Institute for Nuclear Research of the 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 of the 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 and INFN Milano
- A. Pullia
- Dipartimento di Fisica, Università degli Studi di Milano and 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 and 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 of the 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 of the 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 of the 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
- DOI
- https://doi.org/10.1140/epjc/s10052-024-13020-0
- Journal volume & issue
-
Vol. 84,
no. 9
pp. 1 – 19
Abstract
Abstract A search for full energy depositions from bosonic keV-scale dark matter candidates of masses between 65 and 1021 keV has been performed with data collected during Phase II of the GERmanium Detector Array (Gerda) experiment. Our analysis includes direct dark matter absorption as well as dark Compton scattering. With a total exposure of 105.5 kg years, no evidence for a signal above the background has been observed. The resulting exclusion limits deduced with either Bayesian or Frequentist statistics are the most stringent direct constraints in the major part of the 140–1021 keV mass range. As an example, at a mass of 150 keV the dimensionless coupling of dark photons and axion-like particles to electrons has been constrained to $$\alpha '/\alpha 1.5 \times 10^{24}$$ τ n > 1.5 × 10 24 years and for a proton $$\tau _\textrm{p} > 1.3 \times 10^{24}$$ τ p > 1.3 × 10 24 years at 90% CI. For the electron decay $$e^\text {-} \rightarrow \nu _\textrm{e} \gamma $$ e - → ν e γ a lower limit of $$\tau _\textrm{e} > 5.4\times 10^{25}$$ τ e > 5.4 × 10 25 years at 90% CI has been determined.