Precision Atomic Physics Techniques for Nuclear Physics with Radioactive Beams 28
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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. -
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. -
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. -
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 -
(A) Two Stable Isotopes of Lithium and Have Respective Abundances of And
NCERT Solution for Class 12 Physics :Chapter 13 Nuclei Q.13.1 (a) Two stable isotopes of lithium and have respective abundances of and . These isotopes have masses and , respectively. Find the atomic mass of lithium. Answer: Mass of the two stable isotopes and their respective abundances are and and and . m=6.940934 u Q. 13.1(b) Boron has two stable isotopes, and . Their respective masses are and , and the atomic mass of boron is 10.811 u. Find the abundances of and . Answer: The atomic mass of boron is 10.811 u Mass of the two stable isotopes are and respectively Let the two isotopes have abundances x% and (100-x)% Aakash Institute Therefore the abundance of is 19.89% and that of is 80.11% Q. 13.2 The three stable isotopes of neon: and have respective abundances of , and . The atomic masses of the three isotopes are respectively. Obtain the average atomic mass of neon. Answer: The atomic masses of the three isotopes are 19.99 u(m 1 ), 20.99 u(m 2 ) and 21.99u(m 3 ) Their respective abundances are 90.51%(p 1 ), 0.27%(p 2 ) and 9.22%(p 3 ) The average atomic mass of neon is 20.1771 u. Q. 13.3 Obtain the binding energy( in MeV ) of a nitrogen nucleus , given m Answer: m n = 1.00866 u m p = 1.00727 u Atomic mass of Nitrogen m= 14.00307 u Mass defect m=7 m n +7 m p - m m=7Aakash 1.00866+7 1.00727 - 14.00307 Institute m=0.10844 Now 1u is equivalent to 931.5 MeV E b =0.10844 931.5 E b =101.01186 MeV Therefore binding energy of a Nitrogen nucleus is 101.01186 MeV. -
Mass Fraction and the Isotopic Anomalies of Xenon and Krypton in Ordinary Chondrites
Scholars' Mine Masters Theses Student Theses and Dissertations 1971 Mass fraction and the isotopic anomalies of xenon and krypton in ordinary chondrites Edward W. Hennecke Follow this and additional works at: https://scholarsmine.mst.edu/masters_theses Part of the Chemistry Commons Department: Recommended Citation Hennecke, Edward W., "Mass fraction and the isotopic anomalies of xenon and krypton in ordinary chondrites" (1971). Masters Theses. 5453. https://scholarsmine.mst.edu/masters_theses/5453 This thesis is brought to you by Scholars' Mine, a service of the Missouri S&T Library and Learning Resources. This work is protected by U. S. Copyright Law. Unauthorized use including reproduction for redistribution requires the permission of the copyright holder. For more information, please contact [email protected]. MASS FRACTIONATION AND THE ISOTOPIC ANOMALIES OF XENON AND KRYPTON IN ORDINARY CHONDRITES BY EDWARD WILLIAM HENNECKE, 1945- A THESIS Presented to the Faculty of the Graduate School of the UNIVERSITY OF MISSOURI-ROLLA In Partial Fulfillment of the Requirements for the Degree MASTER OF SCIENCE IN CHEMISTRY 1971 T2572 51 pages by Approved ~ (!.{ 1.94250 ii ABSTRACT The abundance and isotopic composition of all noble gases are reported in the Wellman chondrite, and the abundance and isotopic composition of xenon and krypton are reported in the gases released by stepwise heating of the Tell and Scurry chondrites. Major changes in the isotopic composition of xenon result from the presence of radio genic Xel29 and from isotopic mass fractionation. The isotopic com position of trapped krypton in the different temperature fractions of the Tell and Scurry chondrites also shows the effect of isotopic fractiona tion, and there is a covariance in the isotopic composition of xenon with krypton in the manner expected from mass dependent fractiona tion. -
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. -
«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. -
Chapter 16 Nuclear Chemistry
Chapter 16 275 Chapter 16 Nuclear Chemistry Review Skills 16.1 The Nucleus and Radioactivity Nuclear Stability Types of Radioactive Emissions Nuclear Reactions and Nuclear Equations Rates of Radioactive Decay Radioactive Decay Series The Effect of Radiation on the Body 16.2 Uses of Radioactive Substances Medical Uses Carbon-14 Dating Other Uses for Radioactive Nuclides 16.3 Nuclear Energy Nuclear Fission and Electric Power Plants Nuclear Fusion and the Sun Special Topic 16.1: A New Treatment for Brain Cancer Special Topic 16.2: The Origin of the Elements Chapter Glossary Internet: Glossary Quiz Chapter Objectives Review Questions Key Ideas Chapter Problems 276 Study Guide for An Introduction to Chemistry Section Goals and Introductions Section 16.1 The Nucleus and Radioactivity Goals To introduce the new terms nucleon, nucleon number, and nuclide. To show the symbolism used to represent nuclides. To explain why some nuclei are stable and others not. To provide you with a way of predicting nuclear stability. To describe the different types of radioactive decay. To show how nuclear reactions are different from chemical reactions. To show how nuclear equations are different from chemical equations. To show how the rates of radioactive decay can be described with half-life. To explain why short-lived radioactive atoms are in nature. To describe how radiation affects our bodies.. This section provides the basic information that you need to understand radioactive decay. It will also help you understand the many uses of radioactive atoms, including how they are used in medicine and in electricity generation. Section 16.2 Uses of Radioactive Substances Goal: To describe many of the uses of radioactive atoms, including medical uses, archaeological dating, smoke detectors, and food irradiation. -
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. -
All About Elements: Neon
All About Elements: Neon 1 Ward’s All About Elements Series Building Real-World Connections to the Building Blocks of Chemistry PERIODIC TABLE OF THE ELEMENTS GROUP 1/IA 18/VIIIA 1 2 H KEY He Atomic Number 1.01 2/IIA 35 13/IIIA 14/IVA 15/VA 16/VIA 17/VIIA 4.00 3 4 5 6 7 8 9 10 Li Be Symbol Br B C N O F Ne 6.94 9.01 79.90 Atomic Weight 10.81 12.01 14.01 16.00 19.00 20.18 11 12 13 14 15 16 17 18 Na Mg Al Si P S Cl Ar 8 9 10 22.99 24.31 3/IIIB 4/IVB 5/VB 6/VIB 7/VIIB VIIIBVIII 11/IB 12/IIB 26.98 28.09 30.97 32.07 35.45 39.95 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr 39.10 40.08 44.96 47.87 50.94 52.00 54.94 55.85 58.93 58.69 63.55 65.41 69.72 72.64 74.92 78.9678.96 79.90 83.80 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 Rb Sr Y Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe 85.47 87.62 88.91 91.22 92.91 95.94 (97.91)(98) 101.07 102.91 106.42 107.87 112.41 114.82 118.71 121.76 127.60 126.90 131.29 55 56 57–71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 Cs Ba La-Lu Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn ´ 132.91 137.33 178.49 180.95 183.84 186.21 190.23 192.22 195.08 196.97 200.59 204.38 207.20207.2 208.98 (208.98)(209) (209.99)(210) (222.02)(222) 87 88 89–103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 Fr Ra AcAc-Lr - Lr Rf Db Sg Bh Hs Mt Ds Rg Uub Uut Uuq Uup Uuh Uus Uuo ´´ (223.02)(223) (226.03)(226) (261.11)(261) (262.11)(262) (266.12)(266) (264.12)(264) (277.00)(277) (268.14)(268) (247.07)(269) (280.00)(272) (285.00)(285) (284.00)(284) (289.00)(289) (288.00)(288) (293.00)(289) (294.00) (294.00)(294) ´ 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu 138.91 140.12 140.91 144.24 (144.91)(145) 150.36 151.97151.96 157.25 158.93 162.50 164.93 167.26 168.93 173.04 174.97 US: www.wardsci.com Canada: www.wardsci.ca ´´ 800-962-2660 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 © 2010 Rev. -
NUCLEI LEARNING SHEET – 1 SOLUTIONS ANSWER KEY READ & EXPLAIN 1. Why Is the Atomic Mass of Chlorine Not an Integral Multi
NUCLEI LEARNING SHEET – 1 SOLUTIONS ANSWER KEY READ & EXPLAIN 1. Why is the atomic mass of chlorine not an integral multiple of hydrogen? A. Chlorine has two isotopes having masses 34.98u and 36.98u. These are nearly the integral multiples of the atomic mass of a hydrogen atom. Also, the relative abundance of these two isotopes is 75.4 % and 24.6% respectively. So, the average mass of chlorine is calculated by finding the weighted average of the masses of these two isotopes; which is, 35.47u. 2. 1 amu = ______ kg. A. 1.66 x 10-24 kg 3. What is the difference between isobars and isotones? A. Isobars are atoms that have the same mass number, i.e. the total number of protons and neutrons. Isotones have the same number of neutrons but different numbers of protons. 4. How many isotopes does Gold have? 197 195 A. Gold (79Au) has one stable isotope, Au, and 36 radioisotopes, with Au being the most stable with a half-life of 186 days. 5. Heavy stable nuclei have more neutrons than protons. This is because of the fact that (a) neutrons are heavier than protons. (b) electrostatic force between protons are repulsive. (c) neutrons decay into protons through beta decay. (d) nuclear forces between neutrons are weaker than that between protons. A. (b) electrostatic force between protons are repulsive. 6. The radius of a spherical nucleus as measured by electron scattering is 3.6 fm. What is the mass number of the nucleus? A. Given, r=3.6fm, r0=1.2fm 1/3 We know that the radius of spherical nucleus , r=r0A 푟 A=( )3 푟0 3.6 A=( )3 1.2 A=27 The correct answer is A.