Limit on the Radiative Neutrinoless Double Electron Capture of Ar from GERDA Phase I

Total Page:16

File Type:pdf, Size:1020Kb

Limit on the Radiative Neutrinoless Double Electron Capture of Ar from GERDA Phase I Eur. Phys. J. C (2016) 76:652 DOI 10.1140/epjc/s10052-016-4454-5 Regular Article - Experimental Physics Limit on the radiative neutrinoless double electron capture of 36Ar from GERDA Phase I GERDA Collaboration1,a M. Agostini1, M. Allardt4, A. M. Bakalyarov13, M. Balata1, I. Barabanov11 , N. Barros4,20, L. Baudis19, C. Bauer7, E. Bellotti8,9, S. Belogurov11,12, S. T. Belyaev13, G. Benato19, A. Bettini16,17, L. Bezrukov11, T. Bode15, D. Borowicz3,5, V. Brudanin5, R. Brugnera16,17, A. Caldwell14, C. Cattadori9, A. Chernogorov12, V. D’Andrea1, E. V. Demidova12, A. di Vacri1, A. Domula4, E. Doroshkevich11, V. Egorov5, R. Falkenstein18, O. Fedorova11, K. Freund18, N. Frodyma3, A. Gangapshev7,11, A. Garfagnini16,17, C. Gooch14, P. Grabmayr18, V. Gurentsov11, K. Gusev5,13,15, J. Hakenmüller7, A. Hegai18,M.Heisel7, S. Hemmer17, G. Heusser7, W. Hofmann7,M.Hult6, L. V. Inzhechik11,21, J. Janicskó Csáthy15, J. Jochum18, M. Junker1, V. Kazalov11,T.Kihm7, I. V. Kirpichnikov12 , A. Kirsch7,A.Kish19, A. Klimenko5,7,22, R. Kneißl14, K. T. Knöpfle7, O. Kochetov5, V. N. Kornoukhov11,12, V. V. K u z m i n o v 11, M. Laubenstein1, A. Lazzaro15, V. I. Lebedev13, B. Lehnert4,H.Y.Liao14, M. Lindner7, I. Lippi17, A. Lubashevskiy5,7 , B. Lubsandorzhiev11, G. Lutter6, C. Macolino1,23, B. Majorovits14, W. Maneschg7, E. Medinaceli16,17, M. Miloradovic19, R. Mingazheva19, M. Misiaszek3, P. Moseev11, I. Nemchenok5, D. Palioselitis14, K. Panas3, L. Pandola2, K. Pelczar3, A. Pullia10, S. Riboldi10, N. Rumyantseva5, C. Sada16,17, F. Salamida9, M. Salathe7, C. Schmitt18, B. Schneider4, S. Schönert15, J. Schreiner7, A.-K. Schütz18, O. Schulz14, B. Schwingenheuer7, O. Selivanenko11, M. Shirchenko5,13, H. Simgen7, A. Smolnikov7, L. Stanco17, M. Stepaniuk7, L. Vanhoefer14, A. A. Vasenko12, A. Veresnikova11, K. von Sturm16,17, V. Wagner7,M.Walter19, A. Wegmann7, T. Wester4, C. Wiesinger15, H. Wilsenach4, M. Wojcik3, E. Yanovich11,I.Zhitnikov5,S.V.Zhukov13, D. Zinatulina5, K. Zuber4, G. Zuzel3 1 INFN Laboratori Nazionali del Gran Sasso and Gran Sasso Science Institute, Assergi, Italy 2 INFN Laboratori Nazionali del Sud, Catania, Italy 3 Institute of Physics, Jagiellonian University, Kra ków, Poland 4 Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden, Germany 5 Joint Institute for Nuclear Research, Dubna, Russia 6 European Commission, JRC-Geel, Geel, Belgium 7 Max-Planck-Institut für Kernphysik, Heidelberg, Germany 8 Dipartimento di Fisica, Università Milano Bicocca, Milan, Italy 9 INFN Milano Bicocca, Milan, Italy 10 Dipartimento di Fisica, Università degli Studi di Milano e INFN Milano, Milan, Italy 11 Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia 12 Institute for Theoretical and Experimental Physics NRC “Kurchatov Institute”, Moscow, Russia 13 National Research Centre “Kurchatov Institute”, Moscow, Russia 14 Max-Planck-Institut für Physik, Munich, Germany 15 Physik Department and Excellence Cluster Universe, Technische Universität München, Munich, Germany 16 Dipartimento di Fisica e Astronomia dell’Università di Padova, Padua, Italy 17 INFN Padova, Padua, Italy 18 Physikalisches Institut, Eberhard Karls Universität Tübingen, Tübingen, Germany 19 Physik Institut der Universität Zürich, Zurich, Switzerland 20 Present address:Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA, USA 21 Also at: Moscow Institute of Physics and Technology, Moscow, Russia 22 Also at: International University for Nature, Society and Man “Dubna”, Dubna, Russia 23 Present address: LAL, CNRS/IN2P3, Université Paris-Saclay, Orsay, France Received: 19 May 2016 / Accepted: 12 October 2016 © The Author(s) 2016. This article is published with open access at Springerlink.com Abstract Neutrinoless double electron capture is a process lation and the Majorana nature of neutrinos. A search for that, if detected, would give evidence of lepton number vio- neutrinoless double electron capture of 36Ar has been per- formed with germanium detectors installed in liquid argon a e-mail: [email protected] using data from Phase I of the GERmanium Detector Array 123 652 Page 2 of 6 Eur. Phys. J. C (2016) 76:652 Gerda ( ) experiment at the Gran Sasso Laboratory of INFN, p + n Italy. No signal was observed and an experimental lower limit W on the half-life of the radiative neutrinoless double electron e− 36 21 bound capture of Ar was established: T1/2 > 3.6 × 10 years at (A,Z+2) x (A,Z) 90% CI. − ebound + p W n 1 Introduction Fig. 1 Diagram for zero neutrino double electron capture with the The observation of neutrinoless double beta decay (0νββ): emission of one photon − (A, Z − 2) → (A, Z) + 2e , (1) geochemical measurement of 130Ba decay into 130Xe [8,9] can provide unambiguous information on lepton number and the second is a large-volume copper proportional counter 78 violation and indicate the Majorana nature of neutrinos, searching for double K-shell capture in Kr [10]. Sev- regardless the physics mechanism responsible for the decay. eral experiments including the latter established limits on Currently many experiments are searching for this decay both neutrino accompanied and neutrinoless double elec- considering different isotopes. Among these there is the tron capture of different isotopes (see Refs. [10–17]). For Gerda (GERmanium Detector Array) experiment [1]imple- some isotopes the possibility of a resonant enhancement ν menting bare germanium detectors enriched in 76Ge. This of the 0 ECEC decay has been predicted in case of mass experiment searches for neutrinoless double beta decay degeneracy between the initial state and an excited final of 76Ge. Recently the best limit on 0νββ decay half- state [4,18]. 36 life of 76Ge has been published by the Gerda collabora- Ar is expected [19] to undergo double electron cap- 36 tion [2]. ture to the ground state of S. The available energy [20] . ± . Another lepton number violating process that can provide of the decay is 432 58 0 19 keV and, therefore, both the the same information as neutrinoless double beta decay is radiative and the internal conversion modes are energetically the double capture of two bound atomic electrons without allowed. A resonance enhancement of the decay is not pos- the emission of neutrinos (0νECEC): sible for this isotope. Calculations based on the quasiparticle random-phase approximation (QRPA) predict a half-life for − 36 38 2e + (A, Z + 2) → (A, Z) + Q, (2) Ar in the order of 10 years for an effective Majorana neutrino mass of 1 eV [21]. So far, an experimental limit on where the quantity Q corresponds to the energy difference the radiative mode obtained during detector characterizations Gerda between the ground state atoms (A, Z +2) and (A, Z) [3,4]. in the Detector Laboratory has been published (T1/2 > . × 18 While in the corresponding process where two neutrinos 1 9 10 years at 68% CL) [22]. ν 36 are emitted (2νECEC) the available energy of the decay is The radiative mode of 0 ECEC in Ar with the emission carried away by neutrinos plus X-rays or Auger electrons, in of one photon provides a clear signature through the discrete the neutrinoless double electron capture the decay must be value of its energy and allows the detector to be separate accompanied by the emission of at least another particle to from the source of the decay. Two cascades of characteristic = . = . ensure energy and momentum conservation. Different modes X-rays with energies of EK 2 47 keV and EL 0 23 keV can be considered in which 0νECEC decay is associated with are emitted [23], corresponding to the capture of the elec- the emission of different particles like e+e− pairs, one or trons from the K - and the L-shell, respectively. The uncer- two photons, or one internal conversion electron. A detailed tainties for the energies of the X-rays amount to 0.4eV. discussion about double electron capture processes can be The corresponding energy for the monochromatic photon is = − − = . ± . found in Refs. [5–7]. Eγ Q Ek EL 429 88 0 19 keV. γ For 0+ → 0+ transitions the capture of two K -shell This paper reports the search for the 429.88 keV line ν 36 Gerda electrons with the emission of only one photon is forbidden from 0 ECEC decay of Ar with Phase I germanium because of angular momentum conservation. Therefore, the detectors and the determination of a limit on its half-life. most likely process is the capture from the K - and the L-shell. The diagram of this mode is depicted in Fig. 1. The unsta- ble daughter atom relaxes by emission of X-rays or Auger 2 The GERDA experiment electrons. At present, only two experiments found an indication of The Gerda experiment [1] is located at the Laboratori two neutrino double electron capture. The first is based on a Nazionali del Gran Sasso (Lngs) of the INFN. It was 123 Eur. Phys. J. C (2016) 76:652 Page 3 of 6 652 GERDA 16-03 3 GERDA 16-03 4 10 enr 10 39 Coax Ar enrCoax, 17.9 kg yr enrBEGe enr BEGe, 2.3 kg yr nat 103 Coax natCoax, 5.9 kg yr 2 2νββ counts / keV 10 102 counts/(20 keV kg yr) 10 10 1 -1 10 1 500 1000 1500 2000 2500 360 380 400 420 440 460 480 energy [keV] energy [keV] Fig. 2 Energy spectra from the three data sets collected during Gerda region between 360 and 500 keV. The shaded area corresponds to the Phase I. The left panel shows the energy spectra weighted with the prod- ROI defined between 410 and 450 keV uct of life time and detector mass. The right panel displays the energy designed in two phases. During Phase I reprocessed p- fore, data collected from these detectors were discarded. The type semi-coaxial High-Purity Germanium (HPGe) detec- total collected data used for the search for 0νECEC of 36Ar tors enriched in 76Ge (enrGe)toupto86%[24]fromthe correspond to a life time of about 460d.
Recommended publications
  • What Is the Nature of Neutrinos?
    16th Neutrino Platform Week 2019: Hot Topics in Neutrino Physics CERN, Switzerland, Switzerland, 7– 11 October 2019 Matrix Elements for Neutrinoless Double Beta Decay Fedor Šimkovic OUTLINE I. Introduction (Majorana ν’s) II. The 0νββ-decay scenarios due neutrinos exchange (simpliest, sterile ν, LR-symmetric model) III. DBD NMEs – Current status (deformation, scaling relation?, exp. support, ab initio… ) IV. Quenching of gA (Ikeda sum rule, 2νββ-calc., novel approach for effective gA ) V. Looking for a signal of lepton number violation (LHC study, resonant 0νECEC …) Acknowledgements: A. Faessler (Tuebingen), P. Vogel (Caltech), S. Kovalenko (Valparaiso U.), M. Krivoruchenko (ITEP Moscow), D. Štefánik, R. Dvornický (Comenius10/8/2019 U.), A. Babič, A. SmetanaFedor(IEAP SimkovicCTU Prague), … 2 After 89/63 years Fundamental ν properties No answer yet we know • Are ν Dirac or • 3 families of light Majorana? (V-A) neutrinos: •Is there a CP violation ν , ν , ν ν e µ τ e in ν sector? • ν are massive: • Are neutrinos stable? we know mass • What is the magnetic squared differences moment of ν? • relation between • Sterile neutrinos? flavor states • Statistical properties and mass states ν µ of ν? Fermionic or (neutrino mixing) partly bosonic? Currently main issue Nature, Mass hierarchy, CP-properties, sterile ν The observation of neutrino oscillations has opened a new excited era in neutrino physics and represents a big step forward in our knowledge of neutrino10/8/2019 properties Fedor Simkovic 3 Symmetric Theory of Electron and Positron Nuovo Cim. 14 (1937) 171 CNNP 2018, Catania, October 15-21, 2018 10/8/2019 Fedor Simkovic 4 ν ↔ ν- oscillation (neutrinos are Majorana particles) 1968 Gribov, Pontecorvo [PLB 28(1969) 493] oscillations of neutrinos - a solution of deficit10/8/2019 of solar neutrinos in HomestakeFedor Simkovic exp.
    [Show full text]
  • Ivan V. Ani~In Faculty of Physics, University of Belgrade, Belgrade, Serbia and Montenegro
    THE NEUTRINO Its past, present and future Ivan V. Ani~in Faculty of Physics, University of Belgrade, Belgrade, Serbia and Montenegro The review consists of two parts. In the first part the critical points in the past, present and future of neutrino physics (nuclear, particle and astroparticle) are briefly reviewed. In the second part the contributions of Yugoslav physics to the physics of the neutrino are commented upon. The review is meant as a first reading for the newcomers to the field of neutrino physics. Table of contents Introduction A. GENERAL REVIEW OF NEUTRINO a.2. Electromagnetic properties of the neutrino PHYSICS b. Neutrino in branches of knowledge other A.1. Short history of the neutrino than neutrino physics A.1.1. First epoch: 1930-1956 A.2. The present status of the neutrino A.1.2. Second epoch: 1956-1958 A.3. The future of neutrino physics A.1.3. Third epoch: 1958-1983 A.1.4. Fourth epoch: 1983-2001 B. THE YUGOSLAV CONNECTION a. The properties of the neutrino B.1. The Thallium solar neutrino experiment a.1. Neutrino masses B.2. The neutrinoless double beta decay a.1.1. Direct methods Epilogue a.1.2. Indirect methods References a.1.2.1. Neutrinoless double beta decay a.1.2.2. Neutrino oscillations 1 Introduction The neutrinos appear to constitute by number of species not less than one quarter of the particles which make the world, and even half of the stable ones. By number of particles in the Universe they are perhaps second only to photons.
    [Show full text]
  • Electron Capture in Stars
    Electron capture in stars K Langanke1;2, G Mart´ınez-Pinedo1;2;3 and R.G.T. Zegers4;5;6 1GSI Helmholtzzentrum f¨urSchwerionenforschung, D-64291 Darmstadt, Germany 2Institut f¨urKernphysik (Theoriezentrum), Department of Physics, Technische Universit¨atDarmstadt, D-64298 Darmstadt, Germany 3Helmholtz Forschungsakademie Hessen f¨urFAIR, GSI Helmholtzzentrum f¨ur Schwerionenforschung, D-64291 Darmstadt, Germany 4 National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA 5 Joint Institute for Nuclear Astrophysics: Center for the Evolution of the Elements, Michigan State University, East Lansing, Michigan 48824, USA 6 Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA E-mail: [email protected], [email protected], [email protected] Abstract. Electron captures on nuclei play an essential role for the dynamics of several astrophysical objects, including core-collapse and thermonuclear supernovae, the crust of accreting neutron stars in binary systems and the final core evolution of intermediate mass stars. In these astrophysical objects, the capture occurs at finite temperatures and at densities at which the electrons form a degenerate relativistic electron gas. The capture rates can be derived in perturbation theory where allowed nuclear transitions (Gamow-Teller transitions) dominate, except at the higher temperatures achieved in core-collapse supernovae where also forbidden transitions contribute significantly to the rates. There has been decisive progress in recent years in measuring Gamow-Teller (GT) strength distributions using novel experimental techniques based on charge-exchange reactions. These measurements provide not only data for the GT distributions of ground states for many relevant nuclei, but also serve as valuable constraints for nuclear models which are needed to derive the capture rates for the arXiv:2009.01750v1 [nucl-th] 3 Sep 2020 many nuclei, for which no data exist yet.
    [Show full text]
  • 2.3 Neutrino-Less Double Electron Capture - Potential Tool to Determine the Majorana Neutrino Mass by Z.Sujkowski, S Wycech
    DEPARTMENT OF NUCLEAR SPECTROSCOPY AND TECHNIQUE 39 The above conservatively large systematic hypothesis. TIle quoted uncertainties will be soon uncertainty reflects the fact that we did not finish reduced as our analysis progresses. evaluating the corrections fully in the current analysis We are simultaneously recording a large set of at the time of this writing, a situation that will soon radiative decay events for the processes t e'v y change. This result is to be compared with 1he and pi-+eN v y. The former will be used to extract previous most accurate measurement of McFarlane the ratio FA/Fv of the axial and vector form factors, a et al. (Phys. Rev. D 1984): quantity of great and longstanding interest to low BR = (1.026 ± 0.039)'1 I 0 energy effective QCD theory. Both processes are as well as with the Standard Model (SM) furthermore very sensitive to non- (V-A) admixtures in prediction (Particle Data Group - PDG 2000): the electroweak lagLangian, and thus can reveal BR = (I 038 - 1.041 )*1 0-s (90%C.L.) information on physics beyond the SM. We are currently analyzing these data and expect results soon. (1.005 - 1.008)* 1W') - excl. rad. corr. Tale 1 We see that even working result strongly confirms Current P1IBETA event sxpelilnentstatistics, compared with the the validity of the radiative corrections. Another world data set. interesting comparison is with the prediction based on Decay PIBETA World data set the most accurate evaluation of the CKM matrix n >60k 1.77k element V d based on the CVC hypothesis and ihce >60 1.77_ _ _ results
    [Show full text]
  • Double-Beta Decay of 96Zr and Double-Electron Capture of 156Dy to Excited Final States
    Double-Beta Decay of 96Zr and Double-Electron Capture of 156Dy to Excited Final States by Sean W. Finch Department of Physics Duke University Date: Approved: Werner Tornow, Supervisor Calvin Howell Kate Scholberg Berndt Mueller Albert Chang Dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of Physics in the Graduate School of Duke University 2015 Abstract Double-Beta Decay of 96Zr and Double-Electron Capture of 156Dy to Excited Final States by Sean W. Finch Department of Physics Duke University Date: Approved: Werner Tornow, Supervisor Calvin Howell Kate Scholberg Berndt Mueller Albert Chang An abstract of a dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of Physics in the Graduate School of Duke University 2015 Copyright c 2015 by Sean W. Finch All rights reserved except the rights granted by the Creative Commons Attribution-Noncommercial License Abstract Two separate experimental searches for second-order weak nuclear decays to excited final states were conducted. Both experiments were carried out at the Kimballton Underground Research Facility to provide shielding from cosmic rays. The first search is for the 2νββ decay of 96Zr to excited final states of the daughter nucleus, 96Mo. As a byproduct of this experiment, the β decay of 96Zr was also investigated. Two coaxial high-purity germanium detectors were used in coincidence to detect γ rays produced by the daughter nucleus as it de-excited to the ground state. After collecting 1.92 years of data with 17.91 g of enriched 96Zr, half-life limits at the level of 1020 yr were produced.
    [Show full text]
  • «Nucleus-2020»
    NRC «Kurchatov Institute» Saint Petersburg State University Joint Institute for Nuclear Research LXX INTERNATIONAL CONFERENCE «NUCLEUS-2020» NUCLEAR PHYSICS AND ELEMENTARY PARTICLE PHYSICS. NUCLEAR PHYSICS TECHNOLOGIES. BOOK OF ABSTRACTS Online part. 12 – 17 October 2020 Saint Petersburg НИЦ «Курчатовский институт» Санкт-Петербургский государственный университет Объединенный институт ядерных исследований LXX МЕЖДУНАРОДНАЯ КОНФЕРЕНЦИЯ «ЯДРО-2020» ЯДЕРНАЯ ФИЗИКА И ФИЗИКА ЭЛЕМЕНТАРНЫХ ЧАСТИЦ. ЯДЕРНО-ФИЗИЧЕСКИЕ ТЕХНОЛОГИИ. СБОРНИК ТЕЗИСОВ Онлайн часть. 12 – 17 октября 2020 Санкт-Петербург Organisers NRC «Kurchatov Institute» Saint Petersburg State University Joint Institute for Nuclear Research Chairs M. Kovalchuk (Chairman, NRC “Kurchatov Institute”) V. Zherebchevsky (Co-Chairman, SPbU) P. Forsh (Vice-Chairman, NRC “Kurchatov Institute”) Yu. Dyakova (Vice-Chairman, NRC “Kurchatov Institute”) A. Vlasnikov (Vice-Chairman, SPbU) S. Torilov (Scientific Secretary, SPbU) The contributions are reproduced directly from the originals. The responsibility for misprints in the report and paper texts is held by the authors of the reports. International Conference “NUCLEUS – 2020. Nuclear physics and elementary particle physics. Nuclear physics technologies” (LXX; 2020; Online part). LXX International conference “NUCLEUS – 2020. Nuclear physics and elementary particle physics. Nuclear physics technologies” (Saint Petersburg, Russia, 12–17 October 2020): Book of Abstracts /Ed. by V. N. Kovalenko and E. V. Andronov. – Saint Petersburg: VVM, 2020. – 324p. ISBN Международная Конференция «ЯДРО – 2020. Ядерная физика и физика элементарных частиц. Ядерно-физические технологии» (LXX; 2020; Онлайн часть). LXX Международная Конференция «ЯДРО – 2020. Ядерная физика и физика элементарных частиц. Ядерно-физические технологии» (Санкт-Петербург, Россия, 12–17 Октября 2020): Аннот. докл./под ред. В.Н. Коваленко, Е.В. Андронова. – Санкт-Петербург: ВВМ , 2020. – 324 c. ISBN 978-5-9651-0587-8 ISBN 978-5-9651-0587-8 ii Program Committee V.
    [Show full text]
  • Nuclear Physics and Astrophysics SPA5302, 2019 Chris Clarkson, School of Physics & Astronomy [email protected]
    Nuclear Physics and Astrophysics SPA5302, 2019 Chris Clarkson, School of Physics & Astronomy [email protected] These notes are evolving, so please let me know of any typos, factual errors etc. They will be updated weekly on QM+ (and may include updates to early parts we have already covered). Note that material in purple ‘Digression’ boxes is not examinable. Updated 16:29, on 05/12/2019. Contents 1 Basic Nuclear Properties4 1.1 Length Scales, Units and Dimensions............................7 2 Nuclear Properties and Models8 2.1 Nuclear Radius and Distribution of Nucleons.......................8 2.1.1 Scattering Cross Section............................... 12 2.1.2 Matter Distribution................................. 18 2.2 Nuclear Binding Energy................................... 20 2.3 The Nuclear Force....................................... 24 2.4 The Liquid Drop Model and the Semi-Empirical Mass Formula............ 26 2.5 The Shell Model........................................ 33 2.5.1 Nuclei Configurations................................ 44 3 Radioactive Decay and Nuclear Instability 48 3.1 Radioactive Decay...................................... 49 CONTENTS CONTENTS 3.2 a Decay............................................. 56 3.2.1 Decay Mechanism and a calculation of t1/2(Q) .................. 58 3.3 b-Decay............................................. 62 3.3.1 The Valley of Stability................................ 64 3.3.2 Neutrinos, Leptons and Weak Force........................ 68 3.4 g-Decay...........................................
    [Show full text]
  • Two-Neutrino Double Electron Capture on 124Xe Based on an Effective
    Physics Letters B 797 (2019) 134885 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb 124 Two-neutrino double electron capture on Xe based on an effective theory and the nuclear shell model ∗ E.A. Coello Pérez a,b, , J. Menéndez c, A. Schwenk a,b,d a Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany b ExtreMe Matter Institute EMMI, Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany c Center for Nuclear Study, The University of Tokyo, Tokyo 113-0033, Japan d Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany a r t i c l e i n f o a b s t r a c t Article history: We study the two-neutrino double electron capture on 124Xe based on an effective theory (ET) and Received 22 March 2019 large-scale shell model calculations, two modern nuclear structure approaches that have been tested Received in revised form 31 July 2019 against Gamow-Teller and double-beta decay data. In the ET, the low-energy constants are fit to electron Accepted 21 August 2019 − capture and β transitions around xenon. For the nuclear shell model, we use an interaction in a large Available online 23 August 2019 configuration space that reproduces the spectroscopy of nuclei in this mass region. For the dominant Editor: J.-P. Blaizot 124 2νECEC = − × 22 transition to the Te ground state, we find half-lives T1/2 (1.3 18) 10 y for the ET and 2νECEC = − × 22 T1/2 (0.43 2.9) 10 y for the shell model.
    [Show full text]
  • Status and Perspectives of 2, + and 2+ Decays
    Review Status and Perspectives of 2e, eb+ and 2b+ Decays Pierluigi Belli 1,2,*,† , Rita Bernabei 1,2,*,† and Vincenzo Caracciolo 1,2,3,*,† 1 Istituto Nazionale di Fisica Nucleare (INFN), sezione di Roma “Tor Vergata”, I-00133 Rome, Italy 2 Dipartimento di Fisica, Università di Roma “Tor Vergata”, I-00133 Rome, Italy 3 INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy * Correspondence: [email protected] (P.B.); [email protected] (R.B.); [email protected] (V.C.) † These authors contributed equally to this work. Abstract: This paper reviews the main experimental techniques and the most significant results in the searches for the 2e, eb+ and 2b+ decay modes. Efforts related to the study of these decay modes are important, since they can potentially offer complementary information with respect to the cases of 2b− decays, which allow a better constraint of models for the nuclear structure calculations. Some positive results that have been claimed will be mentioned, and some new perspectives will be addressed shortly. Keywords: positive double beta decay; double electron capture; resonant effect; rare events; neutrino 1. Introduction The double beta decay (DBD) is a powerful tool for studying the nuclear instability, the electroweak interaction, the nature of the neutrinos, and physics beyond the Standard Model (SM) of Particle Physics. The theoretical interpretations of the double beta decay Citation: Belli, P.; Bernabei, R.; with the emission of two neutrinos is well described in the SM; the process is characterized Caracciolo, V. Status and Perspectives by a nuclear transition changing the atomic number Z of two units while leaving the atomic of 2e, eb+ and 2b+ Decays.
    [Show full text]
  • Search for Double Beta Decay of 106Cd with an Enriched 106 Cdwo4 Crystal Scintillator in Coincidence with Cdwo4 Scintillation Counters
    Article Search for double beta decay of 106Cd with an enriched 106 CdWO4 crystal scintillator in coincidence with CdWO4 scintillation counters P. Belli1,2 , R. Bernabei 1,2* , V.B. Brudanin3 , F. Cappella4,5 , V. Caracciolo1,2,6 , R. Cerulli1,2 , F.A. Danevich7 , A. Incicchitti4,5 , D.V. Kasperovych7 , V.R. Klavdiienko7 , V.V. Kobychev7 , V. Merlo1,2 ,O.G. Polischuk7 , V.I. Tretyak7 and M.M. Zarytskyy7 1 INFN, sezione di Roma “Tor Vergata”, I-00133 Rome, Italy 2 Dipartimento di Fisica, Università di Roma “Tor Vergata”, I-00133 Rome, Italy 3 Joint Institute for Nuclear Research, 141980 Dubna, Russia 4 INFN, sezione Roma “La Sapienza”, I-00185 Rome, Italy 5 Dipartimento di Fisica, Università di Roma “La Sapienza”, I-00185 Rome, Italy 6 INFN, Laboratori Nazionali del Gran Sasso, 67100 Assergi (AQ), Italy 7 Institute for Nuclear Research of NASU, 03028 Kyiv, Ukraine * Correspondence: Dipartimento di Fisica, Università di Roma “Tor Vergata”, I-00133 Rome, Italy. E-mail address: [email protected] (Rita Bernabei) Received: date; Accepted: date; Published: date Abstract: Studies on double beta decay processes in 106Cd were performed by using a cadmium tungstate 106 106 scintillator enriched in Cd at 66% ( CdWO4) with two CdWO4 scintillation counters (with natural Cd composition). No effect was observed in the data accumulated over 26033 h. New improved half-life limits were set on the different channels and modes of the 106Cd double beta decay at level of 20 22 106 lim T1/2 ∼ 10 − 10 yr. The limit for the two neutrino electron capture with positron emission in Cd + 106 2nECb ≥ × 21 106 to the ground state of Pd, T1/2 2.1 10 yr, was set by the analysis of the CdWO4 data in coincidence with the energy release 511 keV in both CdWO4 counters.
    [Show full text]
  • Radioactivity
    AccessScience from McGraw-Hill Education Page 1 of 43 www.accessscience.com Radioactivity Contributed by: Joseph H. Hamilton Publication year: 2014 A phenomenon resulting from an instability of the atomic nucleus in certain atoms whereby the nucleus experiences a spontaneous but measurably delayed nuclear transition or transformation with the resulting emission of radiation. The discovery of radioactivity by Henri Becquerel in 1896 was an indirect consequence of the discovery of x-rays a few months earlier by Wilhelm Roentgen, and marked the birth of nuclear physics. See also: X-RAYS. On the other hand, nuclear physics can also be said to begin with the proposal by Ernest Rutherford in 1911 that atoms have a nucleus. On the basis of the scattering of alpha particles (emitted in radioactive decay) by gold foils, Rutherford proposed a solar model of atoms, where negatively charged electrons orbit the tiny nucleus, which contains all the positive charge and essentially all the mass of the atom, as planets orbit around the Sun. The attractive Coulomb electrical force holds the electrons in orbit about the nucleus. Atoms have radii of about 10,−10 m and the nuclei of atoms have radii about 2 × 10,−15 m, so atoms are mostly empty space, like the solar system. Niels Bohr proposed a theoretical model for the atom that removed certain difficulties of the Rutherford model. See also: ATOMIC STRUCTURE AND SPECTRA. However, it was only after the discovery of the neutron in 1932 that a proper understanding was achieved of the particles that compose the nucleus of the atom.
    [Show full text]
  • Status and Perspectives on Rare Decay Searches in Tellurium Isotopes
    universe Review Status and Perspectives on Rare Decay Searches in Tellurium Isotopes Alice Campani 1,2,† , Valentina Dompè 3,4,† and Guido Fantini 3,4,*,† 1 Dipartimento di Fisica, Università di Genova, I-16146 Genova, Italy; [email protected] 2 INFN—Sezione di Genova, I-16146 Genova, Italy 3 Dipartimento di Fisica, Sapienza Università di Roma, I-00185 Roma, Italy; [email protected] 4 INFN—Sezione di Roma, I-00185 Roma, Italy * Correspondence: [email protected] † These authors contributed equally to this work. Abstract: Neutrinoless double beta decay (0nbb) is a posited lepton number violating decay whose search is an increasingly active field in modern astroparticle physics. A discovery would imply neutrinos are Majorana particles and inform neutrino physics, cosmology and beyond-standard- model theories. Among the few nuclei where double beta decay (bb) is allowed, tellurium isotopes stand for their high natural abundance and are currently employed in multiple experiments. The search for 0nbb will provide large exposure data sets in the coming years, paving the way for unprecedented sensitivities. We review the latest rare decay searches in tellurium isotopes and compare past results with theories and prospects from running experiments. Keywords: double beta decay; tellurium; 120Te; 123Te; 128Te; 130Te Citation: Campani, A.; Dompè, V.; Fantini, G. Status and Perspectives on 1. Introduction Rare Decay Searches in Tellurium Double beta decay is a rare second order standard model (SM) weak interaction Isotopes. Universe 2021, 7, 212. process where a nucleus transforms into a member of the same isobaric multiplet. The https://doi.org/10.3390/ investigation of rare decays is an active topic of research.
    [Show full text]