Neutrinoless Quadruple Beta Decay (0Ν4β) Is 2 2 2 and Zero, Respectively

Total Page:16

File Type:pdf, Size:1020Kb

Neutrinoless Quadruple Beta Decay (0Ν4β) Is 2 2 2 and Zero, Respectively Neutrinoless Quadruple Beta Decay Julian Heeck∗ and Werner Rodejohann† Max-Planck-Institut f¨ur Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany We point out that lepton number violation is possible even if neutrinos are Dirac particles. We illustrate this by constructing a simple model that allows for lepton number violation by four units only. As a consequence, neutrinoless double beta decay is forbidden, but neutrinoless quadruple beta decay is possible: (A, Z) → (A, Z +4)+4 e−. We identify three candidate isotopes for this decay, the 150 most promising one being Nd due to its high Q0ν4β -value of 2 MeV. Analogous processes, such as neutrinoless quadruple electron capture, are also possible. The expected lifetimes are extremely long, and experimental searches are challenging. INTRODUCTION We will first construct a simple toy model that for- bids Majorana neutrinos but allows for LNV by four Of all the open questions concerning neutrinos—mass units. Then we will search for interesting isotopes that scale and hierarchy, possible CP violation, origin of the can undergo 0ν4β and estimate the expected lifetimes. mixing pattern—the conceptually most interesting has Interestingly, all three isotopes that we identify as po- 96 136 150 to be its very nature: is the neutrino its own antiparti- tential 0ν4β-emitters ( Zr, Xe, and Nd) are fa- cle, and hence a Majorana fermion, or do neutrino and miliar from searches for neutrinoless double beta decay. 150 antineutrino differ, making the neutrino a Dirac particle The most interesting candidate is Nd, with a Q0ν4β- like all the other fermions of the Standard Model (SM). value of 2.079 MeV. We also identify four candidates for The key observation here would be neutrinoless double neutrinoless quadruple electron capture and related pro- 124 130 148 154 beta decay (0ν2β) [1], (A, Z) (A, Z+2)+2 e−, because cesses ( Xe, Ba, Gd, and Dy). More detailed the observation of this ∆L =→ 2 process unambiguously studies regarding model building aspects, collider phe- confirms the Majorana nature of neutrinos [2]. Other nomenology and cosmological aspects will be presented ∆L = 2 signatures, ranging from low-energy processes elsewhere. like neutrinoless double electron capture to collider pro- cesses, have also been proposed and tested (a collection B − L of references can be found in Refs. [1, 3]), but all experi- SIMPLE MODEL FOR ∆( ) = 4 ments came up empty so far. The necessary lepton number violation (LNV) by two We introduce three right-handed neutrinos νR (RHNs) units, ∆L = 2, can be realized directly with a tree level to the SM, which results in Dirac masses for the neutri- Majorana mass term, or indirectly via diagrams contain- nos after spontaneous electroweak symmetry breaking. ing two vertices with ∆L = 1, one example being R- A striking feature of the chiral fermion content of the parity violating supersymmetry [4]. However, it is most SM+νR is the existence of a new, accidental, anomaly- often overlooked that LNV and Majorana neutrinos are free symmetry U(1)B−L, which can therefore be consis- not necessarily connected. For instance, there are non- tently gauged in addition to the SM gauge group. Break- perturbative processes in the SM that violate lepton (and ing B L by a scalar φ with charge B L = 4 can then − | − | ZL baryon) number by three units [5], ∆L = ∆B = 3, which lead to a remaining discrete symmetry group 4 in the obviously do not lead to Majorana neutrinos, and are in lepton sector, which protects the Dirac structure of neu- fact perfectly compatible with Dirac neutrinos. trinos and still allows for LNV processes. Quartic LNV In this letter we will entertain the possibility that LNV operators for Dirac neutrinos were also mentioned in a occurs only by four units, and that ∆L = 2 processes study of anomaly-free discrete R-symmetries in Ref. [6]. For a simple realization of this idea, we work with a arXiv:1306.0580v2 [hep-ph] 25 Jul 2013 are forbidden; neutrinos are then Dirac particles. We gauged U(1) − symmetry, three RHNs ν 1, one will realize those lepton number violating Dirac neutri- B L R ∼ − nos in a simple model based on a spontaneously broken scalar φ 4, and one scalar χ 2, all of which are SM-singlets.∼ The Lagrangian takes∼ −the form U(1)B−L. As an interesting consequence, neutrinoless quadruple beta decay (0ν4β), = SM + kinetic(νR,φ,χ)+ Z′ V (H,φ,χ) − L L L L − (2) (A, Z) (A, Z +4)+4 e , (1) c → + yαβLαHνR,β + καβχ νR,ανR,β + h.c. , is allowed. This novel nuclear decay process plays for our H being the SM Higgs doublet. The phenomenology of framework the role that neutrinoless double beta decay ′ the accompanying Z boson, described in ′ , is not plays for Majorana neutrinos: it will be the dominant Z important here. Working in the diagonal chargedL lep- possible LNV process for Dirac neutrinos, which is surely ton basis, the neutrinos obtain the Dirac mass matrix of great conceptual interest even if the decay rates that we estimate are tiny.1 noless beta decay after 0ν2β. This process would however vio- late Lorentz symmetry, similar to neutrinoless single beta decay 1 One might think that 0ν3β should be the next probable neutri- n → p + e−. 2 M H y upon electroweak symmetry breaking. νc φ ν αβ αβ R h i R A bi-unitary≡ |h i| transformation can be used to diagonalize χ this mass matrix via U †M V = diag(m ,m ,m ), where + 1 2 3 χ χ φ U is the lepton mixing matrix relevant for electroweak h i c χ charged-current interactions. Contrary to other models νR νR with Dirac neutrinos, the right-handed transformation Figure 1: Tree-level realization of the ∆L = 4 operator matrix V does not drop out, but can be absorbed by the c 2 c c → (νRνR) describing the scattering νRνR νRνR. complex symmetric Yukawa coupling matrix καβ = κβα, which is non-diagonal in general. The scalar potential of our model is of the simple form lead to an interesting signature in beta decay measure- V (H,φ,χ) µ2 X 2 + λ X 4 ments: four nucleons undergo beta decay, emitting four ≡ X | | X | | X=XH,φ,χ neutrinos; these four meet at the effective ∆L = 4 ver- (3) + λ H 2 φ 2 + λ H 2 χ 2 + λ χ 2 φ 2 tex and remain virtual. We only see four electrons go- Hφ| | | | Hχ| | | | χφ| | | | − 2 ing out, so at parton level we have 4d 4u + 4e , µφχ + h.c. − → − and on hadron level 4n 4p + 4e (Fig. 2). Obvi- → Here, the coefficients µj and λj have mass dimension one ously this neutrinoless quadruple beta decay (0ν4β) is 2 2 2 and zero, respectively. Assuming µH ,µφ < 0 < µχ and highly unlikely—more so than 0ν2β, as it is of fourth appropriate signs and magnitudes of the λj , we can easily order—but one can still perform the exercise of identi- construct a potential that is bounded from below and fying candidate isotopes for the decay and estimating ZL breaks SU(2)L U(1)Y U(1)B−L to U(1)EM 4 . In the lifetime; constraining the lifetime experimentally is order to forbid Majorana× × neutrinos, it is imperative× that of course also possible. Besides 0ν4β, one can imagine χ does not acquire a vacuum expectation value; without analogous processes such as neutrinoless quadruple elec- the last line in Eq. (3), the necessary condition for this tron capture (0ν4EC), neutrinoless quadruple positron would be decay (0ν4β+), neutrinoless double electron capture dou- ble positron decay (0ν2EC2β+), etc. We will find po- m2 µ2 + λ H 2 + λ φ 2 > 0 , (4) c ≡ χ Hχh i χφh i tential candidates for 0ν4β, 0ν2EC2β+, 0ν3ECβ+, and but the µ term modifies this condition. To see how, let us 0ν4EC. first note that we can chose µ and φ real and positive We will now identify those candidate isotopes for ∆L = h i w.l.o.g. using phase and B L gauge transformations. 4 processes. We need to find isotopes which are more sta- − The µ term will then induce a mass splitting between ble after the flip (A, Z) (A, Z 4). Normal beta decay the properly normalized real (pseudo)scalar fields Re (χ) has to be forbidden in order→ to± handle backgrounds and and Im (χ) make the mother nucleus sufficiently stable. Using nu- m2 = m2 2µ φ , m2 = m2 +2µ φ , (5) clear data charts [7], we found seven possible candidates: Re (χ) c − h i Im(χ) c h i three for 0ν4β, four for neutrinoless quadruple electron 2 so the condition χ = 0 becomes equivalent to mRe (χ) > capture and related decays. They are listed in Tab. I, 0, which can beh easilyi satisfied. together with their Q-values, competing decay channels, Neutrinos are hence Dirac particles, but we also obtain and natural abundance. It should be obvious that not effective ∆L = 4 four-neutrino operators by integrating all 0ν2β candidates (A, Z) make good 0ν4β candidates, out χ at energies E mRe (χ), mIm(χ): as (A, Z + 4) can have a larger mass than (A, Z); it is ≪ less obvious that there exist no 0ν4β candidates with ∆L=4 1 −2 −2 c 2 eff mIm(χ) mRe (χ) καβνR,ανR,β + h.c., beta-unstable daughter nuclei. Using the semi-empirical L ⊃ 2 − (6) Bethe–Weizs¨acker mass formula, one can however show see Fig. 1 for the relevant Feynman diagrams. For sim- plicity, we will assume physics at the TeV scale as the d u source of our four-neutrino operators throughout this pa- d u per; a discussion of more constrained light mediators, as well as of other and more complicated models that gen- W − e− erate effective four-neutrino operators with left-handed ν e− neutrinos, will be presented elsewhere.
Recommended publications
  • CME Search Before Isobar Collisions and Blind Analysis from STAR
    CME Search Before Isobar Collisions and Blind Analysis From STAR Prithwish Tribedy for the STAR collaboration The 36th Winter Workshop on Nuclear Dynamics 1-7th March, 2020, Puerto Vallarta, Mexico In part supported by Introduction Solenoidal Tracker at RHIC (STAR) RHIC has collided multiple ion species; year 2018 was dedicated to search for effects driven by strong electromagnetic fields by STAR Isobars: Ru+Ru, Zr+Zr @ 200GeV (2018) Low energy: Au+Au 27 GeV (2018) Large systems : U+U, Au+Au @ 200 GeV P.Tribedy, WWND 2 The Chiral Magnetic Effect (Cartoon Picture) Quarks Quarks randomly aligned oriented along B antiquarks I II III IV More More right left handed handed quarks quarks J || B J || -B CME converts chiral imbalance to observable electric current P.Tribedy, WWND 2020 3 New Theory Guidance : Complexity Of An Event Magnetic field map Pb+Pb @ 2.76 TeV Axial charge profile b=11.4 fm, Npart=56 Pb+Pb 2.76 TeV, b=11.4 fm, dN5/dxT [a.u.] 0.3 6 uR>uL 0.2 4 uR<uL 0.1 2 0 0 y [fm] -2 -0.1 -4 -0.2 -6 -0.3 -6 -4 -2 0 2 4 6 x [fm] Based on: Chatterjee, Tribedy, Phys. Rev. C 92, Based on: Lappi, Schlichting, Phys. Rev. D 97, 011902 (2015) 034034 (2018) Going beyond cartoon picture: 1) Fluctuations dominate e-by-e physics, 2) B-field & domain size of axial-charge change with √s P.Tribedy, WWND 2020 4 New Theory Guidance : Complexity Of An Event Pb+Pb @ 2.76 TeV Magnetic field b=11.4 fm, N Axial charge profile Pb+Pb 2.76 TeV, b=11.4 fm, dN5/dxT [a.u.] 0.3 6 u 0.2 4 u 0.1 2 0 0 y [fm] -2 -0.1 -4 -0.2 -6 -0.3 -6 -4 -2 0 2 4 6 x [fm] Based on: Chatterjee,
    [Show full text]
  • Neutrinoless Double Beta Decay
    REPORT TO THE NUCLEAR SCIENCE ADVISORY COMMITTEE Neutrinoless Double Beta Decay NOVEMBER 18, 2015 NLDBD Report November 18, 2015 EXECUTIVE SUMMARY In March 2015, DOE and NSF charged NSAC Subcommittee on neutrinoless double beta decay (NLDBD) to provide additional guidance related to the development of next generation experimentation for this field. The new charge (Appendix A) requests a status report on the existing efforts in this subfield, along with an assessment of the necessary R&D required for each candidate technology before a future downselect. The Subcommittee membership was augmented to replace several members who were not able to continue in this phase (the present Subcommittee membership is attached as Appendix B). The Subcommittee solicited additional written input from the present worldwide collaborative efforts on double beta decay projects in order to collect the information necessary to address the new charge. An open meeting was held where these collaborations were invited to present material related to their current projects, conceptual designs for next generation experiments, and the critical R&D required before a potential down-select. We also heard presentations related to nuclear theory and the impact of future cosmological data on the subject of NLDBD. The Subcommittee presented its principal findings and comments in response to the March 2015 charge at the NSAC meeting in October 2015. The March 2015 charge requested the Subcommittee to: Assess the status of ongoing R&D for NLDBD candidate technology demonstrations for a possible future ton-scale NLDBD experiment. For each candidate technology demonstration, identify the major remaining R&D tasks needed ONLY to demonstrate downselect criteria, including the sensitivity goals, outlined in the NSAC report of May 2014.
    [Show full text]
  • 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]
  • RIB Production by Photofission in the Framework of the ALTO Project
    Available online at www.sciencedirect.com NIM B Beam Interactions with Materials & Atoms Nuclear Instruments and Methods in Physics Research B 266 (2008) 4092–4096 www.elsevier.com/locate/nimb RIB production by photofission in the framework of the ALTO project: First experimental measurements and Monte-Carlo simulations M. Cheikh Mhamed *, S. Essabaa, C. Lau, M. Lebois, B. Roussie`re, M. Ducourtieux, S. Franchoo, D. Guillemaud Mueller, F. Ibrahim, J.F. LeDu, J. Lesrel, A.C. Mueller, M. Raynaud, A. Said, D. Verney, S. Wurth Institut de Physique Nucle´aire, IN2P3-CNRS/Universite´ Paris-Sud, F-91406 Orsay Cedex, France Available online 11 June 2008 Abstract The ALTO facility (Acce´le´rateur Line´aire aupre`s du Tandem d’Orsay) has been built and is now under commissioning. The facility is intended for the production of low energy neutron-rich ion-beams by ISOL technique. This will open new perspectives in the study of nuclei very far from the valley of stability. Neutron-rich nuclei are produced by photofission in a thick uranium carbide target (UCx) using a 10 lA, 50 MeV electron beam. The target is the same as that already had been used on the previous deuteron based fission ISOL setup (PARRNE [F. Clapier et al., Phys. Rev. ST-AB (1998) 013501.]). The intended nominal fission rate is about 1011 fissions/s. We have studied the adequacy of a thick carbide uranium target to produce neutron-rich nuclei by photofission by means of Monte-Carlo simulations. We present the production rates in the target and after extraction and mass separation steps.
    [Show full text]
  • Nuclear Physics
    Nuclear Physics Overview One of the enduring mysteries of the universe is the nature of matter—what are its basic constituents and how do they interact to form the properties we observe? The largest contribution by far to the mass of the visible matter we are familiar with comes from protons and heavier nuclei. The mission of the Nuclear Physics (NP) program is to discover, explore, and understand all forms of nuclear matter. Although the fundamental particles that compose nuclear matter—quarks and gluons—are themselves relatively well understood, exactly how they interact and combine to form the different types of matter observed in the universe today and during its evolution remains largely unknown. Nuclear physicists seek to understand not just the familiar forms of matter we see around us, but also exotic forms such as those that existed in the first moments after the Big Bang and that exist today inside neutron stars, and to understand why matter takes on the specific forms now observed in nature. Nuclear physics addresses three broad, yet tightly interrelated, scientific thrusts: Quantum Chromodynamics (QCD); Nuclei and Nuclear Astrophysics; and Fundamental Symmetries: . QCD seeks to develop a complete understanding of how the fundamental particles that compose nuclear matter, the quarks and gluons, assemble themselves into composite nuclear particles such as protons and neutrons, how nuclear forces arise between these composite particles that lead to nuclei, and how novel forms of bulk, strongly interacting matter behave, such as the quark-gluon plasma that formed in the early universe. Nuclei and Nuclear Astrophysics seeks to understand how protons and neutrons combine to form atomic nuclei, including some now being observed for the first time, and how these nuclei have arisen during the 13.8 billion years since the birth of the cosmos.
    [Show full text]
  • Search for Isobar Nuclei in Mass Distributions of Heavy Fission Fragments of 235U Nuclei by Thermal Neutrons
    International Conference “Nuclear Science and its Application”, Samarkand, Uzbekistan, September 25-28, 2012 SEARCH FOR ISOBAR NUCLEI IN MASS DISTRIBUTIONS OF HEAVY FISSION FRAGMENTS OF 235U NUCLEI BY THERMAL NEUTRONS Abdullaeva G.A., Koblik Yu.N., Nebesniy A.F., Pikul V.P. Institute of Nuclear Physics, Tashkent, Uzbekistan To search for isobar nuclei in mass distributions of 235U nuclei heavy fission fragments (FF) caused by thermal neutrons we used experimental data from [1]. In [1] experimental data of yields for each value of mass number in FF mass numbers range from A=125 to A=155 a.m.u. depending on effective charge state z* are published. In figure 1 such experimental dependence of FF yields Yi (Ai) =f(z*) and processing of this dependence by Gauss distribution with an error to one σ for each z* is presented. The basic difficulty consisted in correct transition from measured z* to charges of heavy fragments at the moment of nuclear fission. For this purpose we used the modified expression from [2] in the form of: k * α k1 i i ii VzV1zz 0 . Here zi* and zi - the measured effective charge of the i-th ion with mass number Ai and a charge of corresponding fragment, Vi - velocity of ion, Vo - average velocity of electrons interacting with fragment in the target matter and influencing to formation of an effective charge of the ion. Velocity Vi was defined with use of measured value Ek for each fragment. Velocity Vo can 8 changes in limits from Vo = 2.2×10 cm/s - electron velocity in the first orbit of hydrogen atom to 3.6×108 cm/s [2], constants: α =0.45 and k =0.6 are taken as from [2].
    [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]
  • Chapter 3 the Fundamentals of Nuclear Physics Outline Natural
    Outline Chapter 3 The Fundamentals of Nuclear • Terms: activity, half life, average life • Nuclear disintegration schemes Physics • Parent-daughter relationships Radiation Dosimetry I • Activation of isotopes Text: H.E Johns and J.R. Cunningham, The physics of radiology, 4th ed. http://www.utoledo.edu/med/depts/radther Natural radioactivity Activity • Activity – number of disintegrations per unit time; • Particles inside a nucleus are in constant motion; directly proportional to the number of atoms can escape if acquire enough energy present • Most lighter atoms with Z<82 (lead) have at least N Average one stable isotope t / ta A N N0e lifetime • All atoms with Z > 82 are radioactive and t disintegrate until a stable isotope is formed ta= 1.44 th • Artificial radioactivity: nucleus can be made A N e0.693t / th A 2t / th unstable upon bombardment with neutrons, high 0 0 Half-life energy protons, etc. • Units: Bq = 1/s, Ci=3.7x 1010 Bq Activity Activity Emitted radiation 1 Example 1 Example 1A • A prostate implant has a half-life of 17 days. • A prostate implant has a half-life of 17 days. If the What percent of the dose is delivered in the first initial dose rate is 10cGy/h, what is the total dose day? N N delivered? t /th t 2 or e Dtotal D0tavg N0 N0 A. 0.5 A. 9 0.693t 0.693t B. 2 t /th 1/17 t 2 2 0.96 B. 29 D D e th dt D h e th C. 4 total 0 0 0.693 0.693t /th 0.6931/17 C.
    [Show full text]
  • Henry Primakoff Lecture: Neutrinoless Double-Beta Decay
    Henry Primakoff Lecture: Neutrinoless Double-Beta Decay CENPA J.F. Wilkerson Center for Experimental Nuclear Physics and Astrophysics University of Washington April APS Meeting 2007 Renewed Impetus for 0νββ The recent discoveries of atmospheric, solar, and reactor neutrino oscillations and the corresponding realization that neutrinos are not massless particles, provides compelling arguments for performing neutrinoless double-beta decay (0νββ) experiments with increased sensitivity. 0νββ decay probes fundamental questions: • Tests one of nature's fundamental symmetries, Lepton number conservation. • The only practical technique able to determine if neutrinos might be their own anti-particles — Majorana particles. • If 0νββ is observed: • Provides a promising laboratory method for determining the overall absolute neutrino mass scale that is complementary to other measurement techniques. • Measurements in a series of different isotopes potentially can reveal the underlying interaction process(es). J.F. Wilkerson Primakoff Lecture: Neutrinoless Double-Beta Decay April APS Meeting 2007 Double-Beta Decay In a number of even-even nuclei, β-decay is energetically forbidden, while double-beta decay, from a nucleus of (A,Z) to (A,Z+2), is energetically allowed. A, Z-1 A, Z+1 0+ A, Z+3 A, Z ββ 0+ A, Z+2 J.F. Wilkerson Primakoff Lecture: Neutrinoless Double-Beta Decay April APS Meeting 2007 Double-Beta Decay In a number of even-even nuclei, β-decay is energetically forbidden, while double-beta decay, from a nucleus of (A,Z) to (A,Z+2), is energetically allowed. 2- 76As 0+ 76 Ge 0+ ββ 2+ Q=2039 keV 0+ 76Se 48Ca, 76Ge, 82Se, 96Zr 100Mo, 116Cd 128Te, 130Te, 136Xe, 150Nd J.F.
    [Show full text]
  • A Measurement of the 2 Neutrino Double Beta Decay Rate of 130Te in the CUORICINO Experiment by Laura Katherine Kogler
    A measurement of the 2 neutrino double beta decay rate of 130Te in the CUORICINO experiment by Laura Katherine Kogler A dissertation submitted in partial satisfaction of the requirements for the degree of Doctor of Philosophy in Physics in the Graduate Division of the University of California, Berkeley Committee in charge: Professor Stuart J. Freedman, Chair Professor Yury G. Kolomensky Professor Eric B. Norman Fall 2011 A measurement of the 2 neutrino double beta decay rate of 130Te in the CUORICINO experiment Copyright 2011 by Laura Katherine Kogler 1 Abstract A measurement of the 2 neutrino double beta decay rate of 130Te in the CUORICINO experiment by Laura Katherine Kogler Doctor of Philosophy in Physics University of California, Berkeley Professor Stuart J. Freedman, Chair CUORICINO was a cryogenic bolometer experiment designed to search for neutrinoless double beta decay and other rare processes, including double beta decay with two neutrinos (2νββ). The experiment was located at Laboratori Nazionali del Gran Sasso and ran for a period of about 5 years, from 2003 to 2008. The detector consisted of an array of 62 TeO2 crystals arranged in a tower and operated at a temperature of ∼10 mK. Events depositing energy in the detectors, such as radioactive decays or impinging particles, produced thermal pulses in the crystals which were read out using sensitive thermistors. The experiment included 4 enriched crystals, 2 enriched with 130Te and 2 with 128Te, in order to aid in the measurement of the 2νββ rate. The enriched crystals contained a total of ∼350 g 130Te. The 128-enriched (130-depleted) crystals were used as background monitors, so that the shared backgrounds could be subtracted from the energy spectrum of the 130- enriched crystals.
    [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]
  • Lecture 22 Alpha Decay 1 Introduction 2 Fission and Fusion
    Nuclear and Particle Physics - Lecture 22 Alpha decay 1 Introduction We have looked at gamma decays (due to the EM force) and beta decays (due to the weak force) and now will look at alpha decays, which are due to the strong/nuclear force. In contrast to the previous decays which do not change A, alpha decays happen by emission of some of the 4 nucleons from the nucleus. Specifically, for alpha decay, an alpha particle, 2He, is ejected so generically A A−4 4 X − Y + He Z !Z 2 2 for some X and Y . Y clearly has a different number of nucleons to X. Compare how alpha and beta decays move the nuclei around in Z,N plane N β+ β- α Z Note that gamma decays cannot change Z, N or A. 2 Fission and fusion Alpha decay is in fact only one specific case of a whole range of processes which involve emission of nucleons. These range from single proton or neutron emission up to splitting the nucleus into two roughly equal parts. Particularly in the latter case, these are called fission decays. Which nuclei would we expect to fission? The binding energy per nucleon curve shows that 56 the maximum occurs around 26Fe and drops off to either side. Hence, both small A and large A nuclei are less strongly bound per nucleon than medium A. This means there will be some energy release if two small nuclei are combined into a larger one, a process called fusion which will be discussed later in the course.
    [Show full text]