Beta Decay of Neutron-Rich Isotopes of Zinc and Gallium
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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. -
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. -
Inertial Electrostatic Confinement Fusor Cody Boyd Virginia Commonwealth University
Virginia Commonwealth University VCU Scholars Compass Capstone Design Expo Posters College of Engineering 2015 Inertial Electrostatic Confinement Fusor Cody Boyd Virginia Commonwealth University Brian Hortelano Virginia Commonwealth University Yonathan Kassaye Virginia Commonwealth University See next page for additional authors Follow this and additional works at: https://scholarscompass.vcu.edu/capstone Part of the Engineering Commons © The Author(s) Downloaded from https://scholarscompass.vcu.edu/capstone/40 This Poster is brought to you for free and open access by the College of Engineering at VCU Scholars Compass. It has been accepted for inclusion in Capstone Design Expo Posters by an authorized administrator of VCU Scholars Compass. For more information, please contact [email protected]. Authors Cody Boyd, Brian Hortelano, Yonathan Kassaye, Dimitris Killinger, Adam Stanfield, Jordan Stark, Thomas Veilleux, and Nick Reuter This poster is available at VCU Scholars Compass: https://scholarscompass.vcu.edu/capstone/40 Team Members: Cody Boyd, Brian Hortelano, Yonathan Kassaye, Dimitris Killinger, Adam Stanfield, Jordan Stark, Thomas Veilleux Inertial Electrostatic Faculty Advisor: Dr. Sama Bilbao Y Leon, Mr. James G. Miller Sponsor: Confinement Fusor Dominion Virginia Power What is Fusion? Shielding Computational Modeling Because the D-D fusion reaction One of the potential uses of the fusor will be to results in the production of neutrons irradiate materials and see how they behave after and X-rays, shielding is necessary to certain levels of both fast and thermal neutron protect users from the radiation exposure. To reduce the amount of time and produced by the fusor. A Monte Carlo resources spent testing, a computational model n-Particle (MCNP) model was using XOOPIC, a particle interaction software, developed to calculate the necessary was developed to model the fusor. -
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. -
How Earth Got Its Moon Article
FEATURE How Earth Got its MOON Standard formation tale may need a rewrite By Thomas Sumner he moon’s origin story does not add up. Most “Multiple impacts just make more sense,” says planetary scientists think that the moon formed in the earli- scientist Raluca Rufu of the Weizmann Institute of Science in est days of the solar system, around 4.5 billion years Rehovot, Israel. “You don’t need this one special impactor to Tago, when a Mars-sized protoplanet called Theia form the moon.” whacked into the young Earth. The collision sent But Theia shouldn’t be left on the cutting room floor just debris from both worlds hurling into orbit, where the rubble yet. Earth and Theia were built largely from the same kind of eventually mingled and combined to form the moon. material, new research suggests, and so had similar composi- If that happened, scientists expect that Theia’s contribution tions. There is no sign of “other” material on the moon, this would give the moon a different composition from Earth’s. perspective holds, because nothing about Theia was different. Yet studies of lunar rocks show that Earth and its moon are “I’m absolutely on the fence between these two opposing compositionally identical. That fact throws a wrench into the ideas,” says UCLA cosmochemist Edward Young. Determining planet-on-planet impact narrative. which story is correct is going to take more research. But the Researchers have been exploring other scenarios. Maybe answer will offer profound insights into the evolution of the the Theia impact never happened (there’s no direct evidence early solar system, Young says. -
Radioactive Decay
North Berwick High School Department of Physics Higher Physics Unit 2 Particles and Waves Section 3 Fission and Fusion Section 3 Fission and Fusion Note Making Make a dictionary with the meanings of any new words. Einstein and nuclear energy 1. Write down Einstein’s famous equation along with units. 2. Explain the importance of this equation and its relevance to nuclear power. A basic model of the atom 1. Copy the components of the atom diagram and state the meanings of A and Z. 2. Copy the table on page 5 and state the difference between elements and isotopes. Radioactive decay 1. Explain what is meant by radioactive decay and copy the summary table for the three types of nuclear radiation. 2. Describe an alpha particle, including the reason for its short range and copy the panel showing Plutonium decay. 3. Describe a beta particle, including its range and copy the panel showing Tritium decay. 4. Describe a gamma ray, including its range. Fission: spontaneous decay and nuclear bombardment 1. Describe the differences between the two methods of decay and copy the equation on page 10. Nuclear fission and E = mc2 1. Explain what is meant by the terms ‘mass difference’ and ‘chain reaction’. 2. Copy the example showing the energy released during a fission reaction. 3. Briefly describe controlled fission in a nuclear reactor. Nuclear fusion: energy of the future? 1. Explain why nuclear fusion might be a preferred source of energy in the future. 2. Describe some of the difficulties associated with maintaining a controlled fusion reaction. -
Arxiv:1901.01410V3 [Astro-Ph.HE] 1 Feb 2021 Mental Information Is Available, and One Has to Rely Strongly on Theoretical Predictions for Nuclear Properties
Origin of the heaviest elements: The rapid neutron-capture process John J. Cowan∗ HLD Department of Physics and Astronomy, University of Oklahoma, 440 W. Brooks St., Norman, OK 73019, USA Christopher Snedeny Department of Astronomy, University of Texas, 2515 Speedway, Austin, TX 78712-1205, USA James E. Lawlerz Physics Department, University of Wisconsin-Madison, 1150 University Avenue, Madison, WI 53706-1390, USA Ani Aprahamianx and Michael Wiescher{ Department of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556, USA Karlheinz Langanke∗∗ GSI Helmholtzzentrum f¨urSchwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany and Institut f¨urKernphysik (Theoriezentrum), Fachbereich Physik, Technische Universit¨atDarmstadt, Schlossgartenstraße 2, 64298 Darmstadt, Germany Gabriel Mart´ınez-Pinedoyy GSI Helmholtzzentrum f¨urSchwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany; Institut f¨urKernphysik (Theoriezentrum), Fachbereich Physik, Technische Universit¨atDarmstadt, Schlossgartenstraße 2, 64298 Darmstadt, Germany; and Helmholtz Forschungsakademie Hessen f¨urFAIR, GSI Helmholtzzentrum f¨urSchwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany Friedrich-Karl Thielemannzz Department of Physics, University of Basel, Klingelbergstrasse 82, 4056 Basel, Switzerland and GSI Helmholtzzentrum f¨urSchwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany (Dated: February 2, 2021) The production of about half of the heavy elements found in nature is assigned to a spe- cific astrophysical nucleosynthesis process: the rapid neutron capture process (r-process). Although this idea has been postulated more than six decades ago, the full understand- ing faces two types of uncertainties/open questions: (a) The nucleosynthesis path in the nuclear chart runs close to the neutron-drip line, where presently only limited experi- arXiv:1901.01410v3 [astro-ph.HE] 1 Feb 2021 mental information is available, and one has to rely strongly on theoretical predictions for nuclear properties. -
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. -
Heavy Element Nucleosynthesis
Heavy Element Nucleosynthesis A summary of the nucleosynthesis of light elements is as follows 4He Hydrogen burning 3He Incomplete PP chain (H burning) 2H, Li, Be, B Non-thermal processes (spallation) 14N, 13C, 15N, 17O CNO processing 12C, 16O Helium burning 18O, 22Ne α captures on 14N (He burning) 20Ne, Na, Mg, Al, 28Si Partly from carbon burning Mg, Al, Si, P, S Partly from oxygen burning Ar, Ca, Ti, Cr, Fe, Ni Partly from silicon burning Isotopes heavier than iron (as well as some intermediate weight iso- topes) are made through neutron captures. Recall that the prob- ability for a non-resonant reaction contained two components: an exponential reflective of the quantum tunneling needed to overcome electrostatic repulsion, and an inverse energy dependence arising from the de Broglie wavelength of the particles. For neutron cap- tures, there is no electrostatic repulsion, and, in complex nuclei, virtually all particle encounters involve resonances. As a result, neutron capture cross-sections are large, and are very nearly inde- pendent of energy. To appreciate how heavy elements can be built up, we must first consider the lifetime of an isotope against neutron capture. If the cross-section for neutron capture is independent of energy, then the lifetime of the species will be ( )1=2 1 1 1 µn τn = ≈ = Nnhσvi NnhσivT Nnhσi 2kT For a typical neutron cross-section of hσi ∼ 10−25 cm2 and a tem- 8 9 perature of 5 × 10 K, τn ∼ 10 =Nn years. Next consider the stability of a neutron rich isotope. If the ratio of of neutrons to protons in an atomic nucleus becomes too large, the nucleus becomes unstable to beta-decay, and a neutron is changed into a proton via − (Z; A+1) −! (Z+1;A+1) + e +ν ¯e (27:1) The timescale for this decay is typically on the order of hours, or ∼ 10−3 years (with a factor of ∼ 103 scatter). -
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 -
Optimization Studies of the CERN-ISOLDE Neutron Converter and Fission Target System
Optimization Studies of the CERN-ISOLDE neutron converter and fission target system Raul Luís1, José G. Marques, Thierry Stora, Pedro Vaz, Luca Zanini 1ITN – Estrada Nacional 10, 2686-953, Sacavém, Portugal 2CERN – CH-1211, Genève 23, Switzerland 3PSI – 5232 Villigen, Switzerland E-mail: [email protected] Abstract. The ISOLDE facility at CERN has been one of the leading isotope separator on-line (ISOL) facilities worldwide since it became operative in 1967. More than 1000 isotopes are available at ISOLDE, produced after the bombardment of various primary targets with a pulsed proton beam of energy 1.4 GeV and an average intensity of 2 μA. A tungsten solid neutron converter has been used for ten years to produce neutron-rich fission fragments in UCx targets. In this work, the Monte Carlo code FLUKA and the cross section codes TALYS and ABRABLA were used to study the current layout of the neutron converter and fission target system of the ISOLDE facility. An optimized target system layout is proposed, which maximizes the production of neutron-rich isotopes and reduces the contamination by undesired proton-rich isobars. The studies here reported can already be applied to ISOLDE and will be of special relevance for the future facilities HIE-ISOLDE and EURISOL. 1. Introduction One of the most efficient ways to study nuclei far from stability is the Isotope Separation On-Line (ISOL) method, in which a beam of high-energy hadrons hits a thick target, producing a great variety of radioactive products through different processes like fission, spallation and fragmentation [1]. The resulting nuclides can be studied after they are extracted from the target, ionized and mass separated. -
Concurrent Reduction and Distillation; an Improved Technique for the Recovery and Chemical Refinement of the Isotopes of Cadmium and Zinc*
If I CONCURRENT REDUCTION AND DISTILLATION; AN IMPROVED TECHNIQUE FOR THE RECOVERY AND CHEMICAL REFINEMENT OF THE ISOTOPES OF CADMIUM AND ZINC* H. H. Cardill L. E. McBride LOHF-821046—2 E. W. McDaniel DE83 001931 Operations Division Oak Ridge National Laboratory Oak Ridge, Tennessee 3 7830 .DISCLAIMER • s prepared es an accouni oi WOTk sconsQ'ed by an agency of itie United Slates Cover r "iiit?3 Stilt 65 Gov(?fnft»gn ^ ri(jt ^nv aQcncy Tllf GO* ^or rlny O^ tt^^ir ^rnployut^. TigV MASTER lostifl. ion, apod'aiuj pioiJut;. <y vned nghtv Reference hcein xc any v>t^-'T*t. ^ Dv ^.r^de narno, tf^Oernafk^ mir'ij'iJClureT. or otrierw «d <Jo*^ •nenaalion. or liivONng bv 'Vhe United _^_ . vs and opinions of authors enp'«i«] herein do noi IOM t' irip UnitK* Stales Govefnrneni c a^v agency For presentation at the 11th World Conference of the International Nuclear Target Development Society, October 6-8, 1982, Seattle, Washington. By acceptance of this article, the publisher or recipient acknowledge* the U.S. Govarnment's right to retain a nonaxclusiva, royalty-frtta license in and to any copyright covering tha article. NOTICE P0T09_0£-Jfns,J^SPQRT_JfgE_Il,LESIBLE. I has been reproauce.1 from the best available aopy to pensit the broadest possible avail- ability* *Research sponsored by the Office of Basic Energy Science, U.S. Department of Energy under contract W-7405-eng-26 with the Union Carbide Co rpcration,, DISTRIBUTION OF THIS DOCUMEHT 18 UNLIMITED ' CONCURRENT REDUCTION AND DISTILLATION - AY. IMPROVED TECHNIQUE FOR THE RECOVERY AND CHEMICAL REFINEMENT OF THE ISOTOPES OF CADMIUM AND ZINC H.