Cluster Radioactivity in Superheavy Nuclei 299-302120
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Spontaneous Fission of U234, Pu236, Cm240, and Cm244
Lawrence Berkeley National Laboratory Lawrence Berkeley National Laboratory Title Spontaneous Fission of U234, Pu236, Cm240, and Cm244 Permalink https://escholarship.org/uc/item/0df1j1qm Authors Ghiorso, A. Higgins, G.H. Larsh, A.E. et al. Publication Date 1952-04-21 eScholarship.org Powered by the California Digital Library University of California TWO-WEEK LOAN COPY This is a Library Circulating Copy which may be borrowed for two weeks. For a personal retention copy, call Tech. Info. Division, Ext. 5545 UCRL-1772 Unclassified-Chemistry Distribution UNIVEBSITY OF CALIFCEiNIil Radiation Laboratory Contract No, ti-7405-eng-4.8 24.4 SPONTANEOUS FISSION OF' I'Zu6, ~m~~~~ AND Gm A, Ghiorso, G. H, Higgins, A. E. Larsh, Go To Seaborg, and So G, Thompson April 21, 1752 Berkeley, California A. Ghiorso, G. H. Higgins, A. E. Larsh, G. T. Seaborg, and S. Go Thompson Radiation Laboratory and Department of Chemistry Uni versity of California, Berkeley, Californf a April 21, 1952 In a recent communication commenting on the mechanism of fission we called attention to the simple exponential dependence of spontaneous fission rate on Z~/Aand to the effect of an odd nucleon in slowing the fission process.1 Since it is of interest to test further the simple correlation of the spontaneous fission rate for even-even nuclides wfth z~/A~a further number of such rates have been determined, The spontaneous fission rates were measured by pladng the chemically purified samples on one electrode of a parallel plate ionization chamber, filled with a mixture of argon and carbon dioxide, which was connected with an amplifier f ollawed by a register and a stylus recorder. -
Decay Modes of Uranium in the Range 203 <A<299
Indian Journal of Pure & Applied Physics Vol. 58, April 2020, pp. 234-240 Decay modes of Uranium in the range 203 <A<299 H C Manjunathaa*, G R Sridharb,c, P S Damodara Guptab, K N Sridharb, M G Srinivasd & H B Ramalingame aDepartment of Physics, Government College for Women, Kolar 563 101, India bDepartment of Physics, Government First Grade College, Kolar 563 101, India cResearch and Development Centre, Bharathiar University, Coimbatore 641 046, India dDepartment of Physics, Government First Grade College, Mulbagal 563 131, India eDepartment of Physics, Government Arts College, Udumalpet 642 126, India Received 17 February 2020 In the present work, we have considered the total potential as the sum of the coulomb and proximity potential. We have used the recent proximity function to calculate the nuclear potential. The calculated logarithmic half-lives correspond to fission, cluster and alpha decay are compared with that of experiments. We also identified the most probable decay mode by studying branching ratios of these different decay modes. The competition between different decay modes such as fission, cluster radioactivity and alpha decay finds an important role in nuclear structure. Keywords: Nuclear potential, Cluster radioactivity, Alpha decay, Spontaneous fission 1 Introduction Parkhomenko et al.18 studied the alpha decay It is important to study the alpha decay properties properties for odd mass number superheavy nuclei. of superheavy nuclei. Most of the superheavy nuclei Poenaru et al.19 improved the formula for alpha decay are identified through alpha decay process only. halflives around magic numbers by using the SemFIS Many researchers in the nuclear physics field formula. -
Spontaneous Fission Half-Lives of Heavy and Superheavy Nuclei Within a Generalized Liquid Drop Model
Spontaneous fission half-lives of heavy and superheavy nuclei within a generalized liquid drop model Xiaojun Bao1, Hongfei Zhang1,∗ G. Royer2, Junqing Li1,3 June 4, 2018 1. School of Nuclear Science and Technology, Lanzhou University, Lanzhou 730000, China 2. Laboratoire Subatech, UMR: IN2P3/CNRS-Universit´e-Ecole des Mines, 4 rue A. Kastler, 44 Nantes, France 3. Institute of Modern Physics, Chinese Academy of Science, Lanzhou 730000, China Abstract We systematically calculate the spontaneous fission half-lives for heavy and superheavy arXiv:1302.7117v1 [nucl-th] 28 Feb 2013 nuclei between U and Fl isotopes. The spontaneous fission process is studied within the semi-empirical WKB approximation. The potential barrier is obtained using a generalized liquid drop model, taking into account the nuclear proximity, the mass asymmetry, the phenomenological pairing correction, and the microscopic shell cor- rection. Macroscopic inertial-mass function has been employed for the calculation of the fission half-life. The results reproduce rather well the experimental data. Rela- tively long half-lives are predicted for many unknown nuclei, sufficient to detect them if synthesized in a laboratory. Keywords: heavy and superheavy nuclei; half-lives; spontaneous fission ∗Corresponding author. Tel.: +86 931 8622306. E-mail address: [email protected] 1 1 Introduction Spontaneous fission of heavy nuclei was first predicted by Bohr and Wheeler in 1939 [1]. Their fission theory was based on the liquid drop model. Interestingly, their work also con- tained an estimate of a lifetime for fission from the ground state. Soon afterwards, Flerov and Petrzak [2] presented the first experimental evidence for spontaneous fission. -
Photofission Cross Sections of 238U and 235U from 5.0 Mev to 8.0 Mev Robert Andrew Anderl Iowa State University
Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1972 Photofission cross sections of 238U and 235U from 5.0 MeV to 8.0 MeV Robert Andrew Anderl Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Nuclear Commons, and the Oil, Gas, and Energy Commons Recommended Citation Anderl, Robert Andrew, "Photofission cross sections of 238U and 235U from 5.0 MeV to 8.0 MeV " (1972). Retrospective Theses and Dissertations. 4715. https://lib.dr.iastate.edu/rtd/4715 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. INFORMATION TO USERS This dissertation was produced from a microfilm copy of the original document. While the most advanced technological means to photograph and reproduce this document have been used, the quality is heavily dependent upon the quality of the original submitted. The following explanation of techniques is provided to help you understand markings or patterns which may appear on this reproduction, 1. The sign or "target" for pages apparently lacking from the document photographed is "Missing Page(s)". If it was possible to obtain the missing page(s) or section, they are spliced into the film along with adjacent pages. This may have necessitated cutting thru an image and duplicating adjacent pages to insure you complete continuity, 2. -
Cold Reaction Valleys in the Radioactive Decay of Superheavy 286 112, 292 114 and 296 116 Nuclei
COLD REACTION VALLEYS IN THE RADIOACTIVE DECAY OF SUPERHEAVY 286 112, 292 114 AND 296 116 NUCLEI K. P. Santhosh, S. Sabina School of Pure and Applied Physics, Kannur University, Payyanur Campus, India Cold reaction valleys in the radioactive decay of superheavy nuclei 286 112, 292 114 and 296 116 are studied taking Coulomb and Proximity Potential as the interacting barrier. It is found that in addition to alpha particle, 8Be, 14 C, 28 Mg, 34 Si, 50 Ca, etc. are optimal cases of cluster radioactivity since they lie in the cold valleys. Two other regions of deep minima centered on 208 Pb and 132 Sn are also found. Within our Coulomb and Proximity Potential Model half-life times and other characteristics such as barrier penetrability, decay constant for clusters ranging from alpha particle to 68 Ni are calculated. The computed alpha half-lives match with the values calculated using Viola--Seaborg-- Sobiczewski systematics. The clusters 8Be and 14 C are found to be most probable for 30 emission with T1/2 < 10 s. The alpha-decay chains of the three superheavy nuclei are also studied. The computed alpha decay half-lives are compared with the values predicted by Generalized Liquid Drop Model and they are found to match reasonably well. 1. INTRODUCTION Generally radioactive nuclei decay through alpha and beta decay with subsequent emission of gamma rays in many cases. Again since 1939 it is well known that many radioactive nuclei also decay through spontaneous fission. In 1980 a new type of decay known as cluster radioactivity was predicted by Sandulescu et al. -
Two-Proton Radioactivity 2
Two-proton radioactivity Bertram Blank ‡ and Marek P loszajczak † ‡ Centre d’Etudes Nucl´eaires de Bordeaux-Gradignan - Universit´eBordeaux I - CNRS/IN2P3, Chemin du Solarium, B.P. 120, 33175 Gradignan Cedex, France † Grand Acc´el´erateur National d’Ions Lourds (GANIL), CEA/DSM-CNRS/IN2P3, BP 55027, 14076 Caen Cedex 05, France Abstract. In the first part of this review, experimental results which lead to the discovery of two-proton radioactivity are examined. Beyond two-proton emission from nuclear ground states, we also discuss experimental studies of two-proton emission from excited states populated either by nuclear β decay or by inelastic reactions. In the second part, we review the modern theory of two-proton radioactivity. An outlook to future experimental studies and theoretical developments will conclude this review. PACS numbers: 23.50.+z, 21.10.Tg, 21.60.-n, 24.10.-i Submitted to: Rep. Prog. Phys. Version: 17 December 2013 arXiv:0709.3797v2 [nucl-ex] 23 Apr 2008 Two-proton radioactivity 2 1. Introduction Atomic nuclei are made of two distinct particles, the protons and the neutrons. These nucleons constitute more than 99.95% of the mass of an atom. In order to form a stable atomic nucleus, a subtle equilibrium between the number of protons and neutrons has to be respected. This condition is fulfilled for 259 different combinations of protons and neutrons. These nuclei can be found on Earth. In addition, 26 nuclei form a quasi stable configuration, i.e. they decay with a half-life comparable or longer than the age of the Earth and are therefore still present on Earth. -
Alpha-Decay Chains of Z=122 Superheavy Nuclei Using Cubic Plus Proximity Potential with Improved Transfer Matrix Method
Indian Journal of Pure & Applied Physics Vol. 58, May 2020, pp. 397-403 Alpha-decay chains of Z=122 superheavy nuclei using cubic plus proximity potential with improved transfer matrix method G Naveyaa, S Santhosh Kumarb, S I A Philominrajc & A Stephena* aDepartment of Nuclear Physics, University of Madras, Guindy Campus, Chennai 600 025, India bDepartment of Physics, Kanchi Mamunivar Centre for Post Graduate Studies, Lawspet, Puducherry 605 008, India cDepartment of Physics, Madras Christian College, Chennai 600 059, India Received 4 May 2020 The alpha decay chain properties of Z = 122 isotope in the mass range 298 A 350, even-even nuclei, are studied using a fission-like model with an effective combination of the cubic plus proximity potential in the pre and post-scission regions, wherein the decay rates are calculated using improved transfer matrix method, and the results are in good agreement with other phenomenological formulae such as Universal decay law, Viola-Seaborg, Royer, etc. The nuclear ground-state masses are taken from WS4 mass model. The next minimum in the half-life curves of the decay chain obtained at N=186,178 & 164 suggest the shell closure at N=184, 176 & 162 which coincides well with the predictions of two-centre shell model approach. This study also unveils that the isotopes 298-300, 302, 304-306, 308-310, 312,314122 show 7, 5, 4, 3, 2 and 1 decay chain, respectively. All the other isotopes from A = 316 to 350 may undergo spontaneous fission since the obtained SF half -lives are comparatively less. The predictions in the present study may have an impact in the experimental synthesis and detection of the new isotopes in near future. -
Spontaneous Fission
13) Nuclear fission (1) Remind! Nuclear binding energy Nuclear binding energy per nucleon V - Sum of the masses of nucleons is bigger than the e M / nucleus of an atom n o e l - Difference: nuclear binding energy c u n r e p - Energy can be gained by fusion of light elements y g r e or fission of heavy elements n e g n i d n i B Mass number 157 13) Nuclear fission (2) Spontaneous fission - heavy nuclei are instable for spontaneous fission - according to calculations this should be valid for all nuclei with A > 46 (Pd !!!!) - practically, a high energy barrier prevents the lighter elements from fission - spontaneous fission is observed for elements heavier than actinium - partial half-lifes for 238U: 4,47 x 109 a (α-decay) 9 x 1015 a (spontaneous fission) - Sponatenous fission of uranium is practically the only natural source for technetium - contribution increases with very heavy elements (99% with 254Cf) 158 1 13) Nuclear fission (3) Potential energy of a nucleus as function of the deformation (A, B = energy barriers which represent fission barriers Saddle point - transition state of a nucleus is determined by its deformation - almost no deformation in the ground state - fission barrier is higher by 6 MeV Ground state Point of - tunneling of the barrier at spontaneous fission fission y g r e n e l a i t n e t o P 159 13) Nuclear fission (4) Artificially initiated fission - initiated by the bombardment with slow (thermal neutrons) - as chain reaction discovered in 1938 by Hahn, Meitner and Strassmann - intermediate is a strongly deformed -
Production and Properties Towards the Island of Stability
This is an electronic reprint of the original article. This reprint may differ from the original in pagination and typographic detail. Author(s): Leino, Matti Title: Production and properties towards the island of stability Year: 2016 Version: Please cite the original version: Leino, M. (2016). Production and properties towards the island of stability. In D. Rudolph (Ed.), Nobel Symposium NS 160 - Chemistry and Physics of Heavy and Superheavy Elements (Article 01002). EDP Sciences. EPJ Web of Conferences, 131. https://doi.org/10.1051/epjconf/201613101002 All material supplied via JYX is protected by copyright and other intellectual property rights, and duplication or sale of all or part of any of the repository collections is not permitted, except that material may be duplicated by you for your research use or educational purposes in electronic or print form. You must obtain permission for any other use. Electronic or print copies may not be offered, whether for sale or otherwise to anyone who is not an authorised user. EPJ Web of Conferences 131, 01002 (2016) DOI: 10.1051/epjconf/201613101002 Nobel Symposium NS160 – Chemistry and Physics of Heavy and Superheavy Elements Production and properties towards the island of stability Matti Leino Department of Physics, University of Jyväskylä, PO Box 35, 40014 University of Jyväskylä, Finland Abstract. The structure of the nuclei of the heaviest elements is discussed with emphasis on single-particle properties as determined by decay and in- beam spectroscopy. The basic features of production of these nuclei using fusion evaporation reactions will also be discussed. 1. Introduction In this short review, some examples of nuclear structure physics and experimental methods relevant for the study of the heaviest elements will be presented. -
Alpha Decay and Spontaneous Fission Laboratory Exercise in Nuclear Physics
Alpha Decay and Spontaneous Fission Laboratory Exercise in Nuclear Physics Note: Before attending the laboratory exercise, make sure you read the radiation safety information! This laboratory exercise consists of three parts: • Spectroscopy of an unknown alpha source. • A measurement of the fragment energies from spontaneous fission of 252Cf. • A measurement of the energy loss of alpha particles in air as a function of air pressure. Preparation: Read K.S. Krane, chapter 8 (alpha decay), chapter 13 (fis- sion), and paragraphs 7.1 (Interactions of radiation with matter, the section about heavy charged particles) and 7.4 (semiconductor detectors). In the lab- oration a triple α-source containing the radioactive isotopes 244Cm, 241Am and 239Pu will be used for energy calibration of the instrumentation. Calcu- late the Q−values of the alpha decays for these isotopes using e.g. the table of nuclear properties found at the Brookhaven National Laboratory web- site: http://www2.bnl.gov/ton/. Deduce the kinetic energies of the emitted α-particles from the Q−values. Alpha Decay Alpha decay involves the spontaneous emission of an alpha particle from an atomic nucleus. The alpha particle consists of two protons and two neutrons 1 and is the same species as the nucleus of a helium (4He) atom. These four nucleons have their origin in the nucleus X before the decay (the mother nucleus) and the nucleus is therefore transformed into a nucleus X0 (the daughter nucleus) of another basic element according to the relation: A A−4 0 Z XN !Z−2 XN−2 + α; (1) where α is the alpha particle, N is the number of neutrons, Z is the number of protons, and A = N + Z is the mass number. -
Table De Radionucl´Eides 90 Th 138
228 LNE { LNHB/CEA { Table de Radionucl´eides 90 Th 138 228 90 Th 138 1 Decay Scheme Th-228 decays 100 % by alpha-particle emission to various excited levels and the ground state of Ra-224, and by a small O-20 cluster-decay branch of 1.13 (22) 10−11 %. Le thorium 228 se d´esint`egre par ´emissionalpha principalement vers le niveau fondamental et le niveau excit´ede 84,4 keV du radium 224. 2 Nuclear Data 228 T1=2( Th ) : 1,9126 (9) a 224 T1=2( Ra ) : 3,631 (2) d Qα(228Th ) : 5520,08 (22) keV 2.1 α Transitions Energy Probability F keV × 100 α0;8 4527,43 (23) 0,0000045 (7) 7,2 α0;7 4603,74 (23) 0,000017 (3) 7 α0;6 5040,9 (3) 0,000024 (5) 4600 α0;5 5087,01 (24) 0,000010 (2) 21400 α0;4 5229,72 (22) 0,036 (6) 44 α0;3 5269,30 (22) 0,218 (4) 12,5 α0;2 5304,10 (22) 0,408 (7) 10,7 α0;1 5435,71 (22) 26,0 (5) 0,958 α0;0 5520,08 (22) 73,4 (5) 1 Surrey Univ. /A.L. Nichols 1 01=08=2001 − 15=1=2013 228 LNE { LNHB/CEA { Table de Radionucl´eides 90 Th 138 2.2 Gamma Transitions and Internal Conversion Coefficients Energy Pγ+ce Multipolarity αK αL αM αT keV × 100 γ4;2(Ra) 74,38 (4) 0,015 (5) [E2] 28,3 (4) 7,71 (11) 38,6 (6) γ1;0(Ra) 84,373 (3) 26,4 (7) E2 15,57 (22) 4,24 (6) 21,2 (3) γ2;1(Ra) 131,612 (5) 0,158 (3) E1 0,194 (3) 0,0406 (6) 0,00977 (14) 0,247 (4) γ5;4(Ra) 142,71 (11) 0,0000041 (13) [E2] 0,279 (4) 1,368 (20) 0,372 (6) 2,14 (3) γ3;1(Ra) 166,410 (4) 0,217 (4) E2 0,225 (4) 0,691 (10) 0,187 (3) 1,164 (17) γ5;3(Ra) 182,29 (10) 0,0000057 (20) [E1] 0,0894 (13) 0,01757 (25) 0,00421 (6) 0,1126 (16) γ4;1(Ra) 205,99 (4) 0,0204 (5) [E1] 0,0671 (10) 0,01292 -
Binding Energy of the Mother Nucleus Is Lower Than That of the Daughter Nucleus
Chapter 1 Learning Objectives • Historical Recap • Understand the different length scales of nuclear physics • Know the nomenclature for isotopes and nuclear reactions • Know the different types of neutron nuclear collisions and their relationship to each other • Basic principles of nuclear reactor Learning Objectives • Neutron Sources • Basic Principles of Nuclear Reactor • Bindinggg energyy curve • Liquid drop model • Fission Reaction • ODE Review • Radioactive Decay • Decay Chains • Chart of Nuclides Historical Recap • Driscoll handout • New programs – GNEP/AFCI – Gen-IV – Nuclear Power 2010 Why nuclear? • Power density – 1000 MW electric • 10 000 tons o f coal per DAY!! • 20 tons of uranium per YEAR (of which only 1 ton is U -235) A typical pellet of uranium weighs about 7 grams (0.24ounces). It can generate as much energy as…… 3.5 barrels of oil or…… 17,000 cubic feet of natural gas, or….. 1,780 pounds of coal. Why nuclear? • Why still use coal – Capital cost – Politics – Public perception of nuclear, nuclear waster issue What do you think is the biggest barrier to constructing the next U.S. nuclear power plant? 50% 40% 30% 20% 44% 10% 16% 15% 14% 0% 10% - 2008 survey of Political Nuclear Waste Cost of Fear of Other Resistance to Disposal Nuclear Nuclear energy professionals Nuclear Energy Issues Power Plant Accident Construction Image by MIT OpenCourseWare. “Eighty-two percent of Americans living in close proximity to nuclear power plants favor nuclear energy, and 71 percent are willing to see a new reactor built near them, according to a new public opinion survey of more than 1,100 adults nationwide.”– NEI, September 2007 Basic Principles ofof Nuclear Reactor • Simple device – Fissioning fuel releases energy in the “core” – Heat isis transported away by a coolant which couples the heat source to a Rankine steam cycle – Very similar to a coal plant, with the exception of the combustion process – Main complication arises from the spent fuel, a mix of over 300 fission products Public domain image from wikipedia.