Nuclear Fusion
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Overview of the SPARC Tokamak
This is a repository copy of Overview of the SPARC tokamak. White Rose Research Online URL for this paper: https://eprints.whiterose.ac.uk/166980/ Version: Published Version Article: Creely, A. J., Greenwald, M. J., Ballinger, S. B. et al. (42 more authors) (2020) Overview of the SPARC tokamak. Journal of Plasma Physics. 865860502. ISSN 0022-3778 https://doi.org/10.1017/S0022377820001257 Reuse This article is distributed under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs (CC BY-NC-ND) licence. This licence only allows you to download this work and share it with others as long as you credit the authors, but you can’t change the article in any way or use it commercially. More information and the full terms of the licence here: https://creativecommons.org/licenses/ Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. [email protected] https://eprints.whiterose.ac.uk/ J. Plasma Phys. (2020), vol. 86, 865860502 © The Author(s), 2020. 1 Published by Cambridge University Press This is an Open Access article, distributed under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives licence (http://creativecommons.org/licenses/by-nc-nd/4.0/), which permits non-commercial re-use, distribution, and reproduction in any medium, provided the original work is unaltered and is properly cited. The written permission of Cambridge University Press must be obtained for commercial re-use or in order to create a derivative work. -
STATUS of FUSION ENERGY Impact & Opportunity for Alberta Volume II
STATUS OF FUSION ENERGY Impact & Opportunity for Alberta Volume II Appendices Prepared by Alberta/Canada Fusion Energy Program March 2014 ALBERTA COUNCIL OF TECHNOLOGIES Gratefully acknowledges the support of: Alberta Energy Stantec Corporation University of Alberta Alberta/Canada Fusion Energy Advisory Committee Gary Albach Nathan Armstrong Brian Baudais Will Bridge Robert Fedosejevs Peter Hackett Chris Holly Jerry Keller Brian Kryska Axel Meisen Rob Pitcairn Klaas Rodenburg John Rose Glenn Stowkowy Martin Truksa Gary Woloshyniuk Perry Kinkaide Allan Offenberger A special thank you is extended to the institutions (identified in this report) that were visited and to the many persons who so graciously hosted our site visits, provided the briefing material presented in this status report and thereby assisted our fusion assessment. Report Authors Allan Offenberger Robert Fedosejevs Klaas Rodenburg Perry Kinkaide Contact: Dr. Perry Kinkaide [email protected] 780-990-5874 Dr. Allan Offenberger [email protected] 780-483-1740 i TABLE OF CONTENTS Page List of Acronyms ………………………………………………………………………….. iii List of Figures……………………………………………………………………………… iv Appendix A: Assessment of Major Global Fusion Technologies 1.0 Context - Global Energy Demand……………………………………………………… 1 1.0.1 Foreward ……………………………………………………………………… 1 1.0.2 Energy Trends………………………………………………………………… 2 1.0.3 Energy From Fusion Reactions……………………………………………… 4 1.1 Major Approaches to Fusion Energy………………………………………………….. 7 1.1.1 Introduction……………………………………………………………………. 7 1.1.2 Fusion Reactions & the Fuel Cycle………………………………………….. 8 1.1.3 IFE Approaches to Fusion…………………………………………………… 11 1.1.3.1 Introduction………………………………………………………….. 11 1.1.3.2 Indirect Drive…………………………………………………………14 1.1.3.3 Direct Drive…………………………………………………………. 16 1.1.3.4 Fast Ignition………………………………………………………… 17 1.1.3.5 Shock Ignition………………………………………………………..19 1.1.3.6 IFE Power Reactor Systems……………………………………….20 1.1.3.7 Modeling Codes……………………………………………………. -
Concepts for a Deuterium-Deuterium Fusion Reactor
Concepts for a deuterium-deuterium fusion reactor Roberto Onofrio1, 2 1Dipartimento di Fisica e Astronomia “Galileo Galilei”, Universit`adi Padova, Via Marzolo 8, Padova 35131, Italy 2Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755, USA We revisit the assumption that reactors based on deuterium-deuterium (D-D) fusion processes have to be necessarily developed after the successful completion of experiments and demonstrations for deuterium-tritium (D-T) fusion reactors. Two possible mechanisms for enhancing the reactivity are discussed. Hard tails in the energy distribution of the nuclei, through the so-called κ-distribution, allow to boost the number of energetic nuclei available for fusion reactions. At higher temperatures − − than usually considered in D-T plasmas, vacuum polarization effects from real e+e and µ+µ pairs may provide further speed-up due to their contribution to screening of the Coulomb barrier. Furthermore, the energy collection system can benefit from the absence of the lithium blanket, both in simplicity and compactness. The usual thermal cycle can be bypassed with comparable efficiency levels using hadronic calorimetry and third-generation photovoltaic cells, possibly allowing to extend the use of fusion reactors to broader contexts, most notably maritime transport. I. INTRODUCTION high yield scintillating materials and hadronic calorime- try with third-generation photovoltaic cells. This could lead to energy conversion at an initially nearly compara- It is usually assumed that the first commercial fusion ble efficiency with respect to a thermal cycle, with un- reactors will be based on D-T mixtures, and within this known margins for improvement, and within a compact frame a well-defined path has been paved with the ongo- design. -
Reactor Potential for Magnetized Target Fusion
TR.TA-A Report ISSN 1102-2051 VETENSKAP OCH ISRN KTH/ALF/--01/2--SE 1ONST KTH-ALF--01-2 KTH Reactor Potential for Magnetized Target Fusion Jon-Erik Dahlin Research and Training programme on CONTROLLED THERMONUCLEAR FUSION AND PLASMA PHYSICS (Association EURATOM/NFR) FUSION PLASMA PHYSICS ALFV N LABORATORY ROYAL INSTITUTE OF TECHNOLOGY SE-100 44 STOCKHOLM SWEDEN PLEASE BE AWARE THAT ALL OF THE MISSING PAGES IN THIS DOCUMENT WERE ORIGINALLY BLANK TRITA-ALF-2001-02 ISRN KTH/ALF/--01/2--SE Reactor Potential for Magnetized Target Fusion J.-E. Dahlin VETENSKAP OCH KONST Stockholm, June 2001 The Alfven Laboratory Division of Fusion Plasma Physics Royal Institute of Technology SE-100 44 Stockholm, Sweden (Association EURATOM/NFR) Printed by Alfven Laboratory Fusion Plasma Physics Division Royal Institute of Technology SE-100 44 Stockholm Abstract Magnetized Target Fusion (MTF) is a possible pathway to thermonuclear fusion different from both magnetic fusion and inertial confinement fusion. An imploding cylindrical metal liner compresses a preheated and magnetized plasma configuration until thermonuclear conditions are achieved. In this report the Magnetized Target Fusion concept is evaluated and a zero-dimensional computer model of the plasma, liner and circuit as a connected system is designed. The results of running this code are that thermonuclear conditions are achieved indeed, but only during a very short time. At peak compression the pressure from the compressed plasma and mag- netic field is so large reversing the liner implosion into an explosion. The time period of liner motion reversal is termed the dwell time and is crucial to the performance of the fusion system. -
Can Deuterium Formation Be Measured?
CAN DEUTERIUM FORMATION BE MEASURED? Robert K. Soberman∗ and Maurice Dubin† retired (Dated: November 12, 2018) The fundamental PP reaction has never been attempted in the laboratory as theory states it cannot be measured within the human life span. This forms the foundation of stellar nucleosynthesis and the standard solar model. Yet numerous observations including the Sun’s obvious variability argue the theory is flawed and the reaction occurs in times many orders of magnitude shorter than prediction. Considering the consequence to accepted models and controlled fusion, testing is warranted. PACS numbers: 95.30.Cq, 96.60.-j, 25.40.-h There is no record of an attempt to measure the transmutation probability for the fundamental reaction 1H(p, e+,ν)2H. As Bethe and Critchfield [1] predicted a reaction rate of 14(10)9 years no one has been bold enough to test this prediction. Parker and Rolfs [2] wrote “It can be estimated that with a total cross section of 10−47cm2 at Ep(lab) = 1MeV for a proton beam of 1 mA incident on a thick hydrogen target, there would be only one 1H(p, e+,ν)2H reaction in 106 yr.” A similar but numerically discrepant statement appears in Clayton’s classic stellar nucleosynthesis text [3]. As no research team has the patients, resources or longevity to wait out such a prediction it is not surprising that it has never been tested. Such a slow reaction rate was necessary for the standard stellar power model. A much shorter time would cut the lifetime of stars accordingly and a brief reaction time such as seconds would, in that model, cause stars to explode when the reaction conditions were reached. -
Cold Fusion Phenomena May 23-25, 1989 Santa Fe, New Mexico
WORKSHOP ON COLD FUSION PHENOMENA MAY 23-25, 1989 SANTA FE, NEW MEXICO AGENDA Sponsored by Los Alamos National Laboratory and the U.S. Department of Energy TABLE OF CONTENTS Program Committee V Agenda 1-6 Abstracts of Presentations Sessions A - E WORKSHOP CO-CHAIRMAN Prof. Johann Rafelski Department of Physics Dr. Norman Hackerman University of Arizona The Welch Foundation Tucson, AZ Houston, TX Dr. A. John Appleby Dr. J. Robert Schrieffer Center for Electrochemical Systems Director, Institute for and Hydrogen Research Theoretical Physics Texas A&M University University of California College Station, TX Santa Barbara, CA Dr. Anthony L. Turkevich Enrico Fermi Institute TECHNICAL PROGRAM COORDINATOR University of Chicago Chicago, IL Dr. Reed J. Jensen Los Alamos National Laboratory PROGRAM SUPPORT COORDINATOR Mr. David C. Phillips Los Alamos National Laboratory WORKSHOP PROGRAM COMMITTEE Prof. Allen Bard Department of Chemistry University of Texas Austin, TX Dr. Hans Frauenfelder Department of Physics University of Illinois at Urbana-Champaign Urbana, IL Dr. Steven E. Jones Department of Chemistry Brigham Young University Provo, UT Prof. Arthur K. Kerman Director, Laboratory for Nuclear Science MIT Cambridge, MA Prof. Steve Koonin Institute for Theoretical Physics University of California Santa Barbara, CA AGENDA WORKSHOP ON COLD FUSION PHENOMENA May 22-25, 1989 SWEENEY CENTER, SANTA FE, NM MONDAY, MAY 22 Workshop participants arrive in Santa Fe 4:00 - 8:00 Registration and badge issue at EldoradoHotel -Hospitality room available at EldoradoHotel TUESDAY, MAY 23 7:30 - 8:00 Arrival at Sweeney Center 8:00 - 8:30 Late Registration 8:30 - 9:00 Preliminary Remarks Reed J. -
Stellar Evolution
AccessScience from McGraw-Hill Education Page 1 of 19 www.accessscience.com Stellar evolution Contributed by: James B. Kaler Publication year: 2014 The large-scale, systematic, and irreversible changes over time of the structure and composition of a star. Types of stars Dozens of different types of stars populate the Milky Way Galaxy. The most common are main-sequence dwarfs like the Sun that fuse hydrogen into helium within their cores (the core of the Sun occupies about half its mass). Dwarfs run the full gamut of stellar masses, from perhaps as much as 200 solar masses (200 M,⊙) down to the minimum of 0.075 solar mass (beneath which the full proton-proton chain does not operate). They occupy the spectral sequence from class O (maximum effective temperature nearly 50,000 K or 90,000◦F, maximum luminosity 5 × 10,6 solar), through classes B, A, F, G, K, and M, to the new class L (2400 K or 3860◦F and under, typical luminosity below 10,−4 solar). Within the main sequence, they break into two broad groups, those under 1.3 solar masses (class F5), whose luminosities derive from the proton-proton chain, and higher-mass stars that are supported principally by the carbon cycle. Below the end of the main sequence (masses less than 0.075 M,⊙) lie the brown dwarfs that occupy half of class L and all of class T (the latter under 1400 K or 2060◦F). These shine both from gravitational energy and from fusion of their natural deuterium. Their low-mass limit is unknown. -
Primordial Nucleosynthesis in the Precision Cosmology Era the Annual Review of Nuclear and Particle Science Gary Steigman (2007)
Primordial Nucleosynthesis in the Precision Cosmology Era The Annual Review of Nuclear and Particle Science Gary Steigman (2007) Galactic Archeology Seminar Manuel Kramer Universit¨atHeidelberg December 1, 2017 Contents 1 Introduction 2 Fusion of the first nuclides 3 Observations of the relic nuclides 4 Theory vs data 5 Summary Source: CERN Introduction Fusion of the first nuclides Observations of the relic nuclides Theory vs data Summary Fusion of the first nuclides Initial neutron to proton ratio Neutron & Proton equilibrium Once stable hadrons can form from the quark gluon plasma in the very early universe, neutrons and protons are in thermal equilibrium by the weak interactions: − p + e $ n + νe (1) + n + e $ p +ν ¯e Mass of protons is slightly lower than that of the neutrons ni =pi = 1=7 (2) Introduction Fusion of the first nuclides Observations of the relic nuclides Theory vs data Summary Deuterium evolution Deuterium is formed by fusion of a proton and a neutron n + p $ d + γ (3) Significant amounts can only built up when kT . 80 keV −10 The higher the baryon density η10 = 10 (nB=nγ), the higher the interaction rate Introduction Fusion of the first nuclides Observations of the relic nuclides Theory vs data Summary Helium-4 evolution Nucelar fusion processes The starting point for all subsequent fusions is Deuterium Deuterium fusion is a slow reaction Deuterium is immediately converted to 3He and tritium no stable mass-5 nuclides ! bottleneck at 4He Source: https://en.wikipedia.org/ wiki/Big Bang nucleosynthesis Introduction Fusion of -
Tokamak Energy April 2019
Faster Fusion through Innovations M Gryaznevich and Tokamak Energy Ltd. Team FusionCAT Webinar 14 September 2020 © 2020 Tokamak Energy Tokamak 20202020 © Energy Tokamak Fusion Research – Public Tokamaks JET GLOBUS-M Oxford, UK StPetersburg, RF COMPASS KTM Prague, CZ (1) Kurchatov, KZ (3) T15-M Alcator C-Mod Moscow STOR-M Cambridge, MA MAST Saskatoon, SK Oxford, UK ASDEX KSTAR ITER(1)(2) / WEST Garching, DE Daejeon, KR LTX / NSTX Cadarache, FR FTU HL-2 (1) Pegasus Princeton, NJ Frascati, IT JT-60SA DIII-D Madison, WI TCV Chengdu, CN QUEST Naka, JP San Diego, CA ISTTOK Lausanne, CH Kasuga, JP Lisbon, PT SST-1 / ADITY EAST Gandhinagar, IN Hefei, CN Conventional Tokamak • Fusion research is advancing Spherical Tokamak • However, progress towards Fusion Power is constrained Note: Tokamaks are operating unless indicated otherwise. (1) Under construction. (2) The International Thermonuclear Experimental Reactor (“ITER”) megaproject is supported by China, the European Union, India, Japan, Korea, Russia and the United States. © 2020© Energy Tokamak (3) No longer in use. 2 Fusion Development – Private Funding Cambridge, MA Langfang, PRC Vancouver, BC Los Angeles, CA Orange County, CA • Common goal of privately and publicly Oxford, UK Oxford, UK funded Fusion research is to develop technologies and Fusion Industry • At TE, we have identified the key technology Conventional Tokamak Spherical Tokamak gaps needed to create a commercial fusion Non-Tokamak Technology reactor and then used Technology Roadmapping as an approach chart our path. © 2020© -
Modern Physics, the Nature of the Interaction Between Particles Is Carried a Step Further
44.1 Some Properties of Nuclei 1385 are the same, apart from the additional repulsive Coulomb force for the proton– U(r ) (MeV) proton interaction. 40 Evidence for the limited range of nuclear forces comes from scattering experi- n–p system ments and from studies of nuclear binding energies. The short range of the nuclear 20 force is shown in the neutron–proton (n–p) potential energy plot of Figure 44.3a 0 r (fm) obtained by scattering neutrons from a target containing hydrogen. The depth of 1 567432 8 the n–p potential energy well is 40 to 50 MeV, and there is a strong repulsive com- Ϫ20 ponent that prevents the nucleons from approaching much closer than 0.4 fm. Ϫ40 The nuclear force does not affect electrons, enabling energetic electrons to serve as point-like probes of nuclei. The charge independence of the nuclear force also Ϫ60 means that the main difference between the n–p and p–p interactions is that the a p–p potential energy consists of a superposition of nuclear and Coulomb interactions as shown in Figure 44.3b. At distances less than 2 fm, both p–p and n–p potential The difference in the two curves energies are nearly identical, but for distances of 2 fm or greater, the p–p potential is due to the large Coulomb has a positive energy barrier with a maximum at 4 fm. repulsion in the case of the proton–proton interaction. The existence of the nuclear force results in approximately 270 stable nuclei; hundreds of other nuclei have been observed, but they are unstable. -
Faster Fusion
AN INTRODUCTION TO Faster fusion What is fusion? That is, the tokamak is a toroidal – or ring- PROGRESS IN FUSION HAS SLOWED Can we achieve fusion faster? Additionally, high temperature Fusion is the energy of the stars. Small atomic nuclei join together to make larger ones, doughnut-shaped – vessel with magnetic We believe so. In the last few decades new superconductors can support a much which releases energy. All the heavier elements in the universe were made this way. coils that make a trap for the plasma. The Moore’s Law technologies have emerged. Building on all higher current density than conventional plasma is heated using microwaves or (computers) the work that has gone into JET and ITER, it superconductors (meaning they can achieve Fusion only happens at very high temperatures because it is forcing together particles that powerful particle injectors and it has to be Fusion energy gain now seems feasible that by using a slightly higher magnetic fields for the same thickness would usually be far apart. Nuclei are all positively charged particles, so they keep away stabilised by carefully controlling the shape of differently shaped (spherical) tokamak of superconductor), so they will work with the from each other just like magnets of the same polarity repel. Nuclei don’t want to come the magnetic fields. Progress combined with the latest generation of high squashed-up shape of the spherical tokamak. toward fusion together, so the only way for fusion to occur is to heat things up a lot, like in the stars. temperature superconductors for magnets, we HTS magnets will be a game-changer for When will we be using fusion power? could make smaller, cheaper machines and so fusion, but scaling up requires new systems That is the hardest question to answer. -
Discussion Paper DIS-16-04 Small Modular Reactors: Regulatory
Discussion Paper DIS-16-04 Small Modular Reactors: Regulatory Strategy, Approaches and Challenges Section 3. Fusion Technologies CNSC would like to know: 1. What are the types and magnitudes of risks and hazards that would be posed by different fusion technologies (conventional and radiation hazards)? 2. With this in mind, how would the risks posed by activities involving fusion reactors differ from current nuclear fission reactors? 3. Should fusion reactors be regulated differently than fission reactors? 1. Risks and hazards posed by different fusion technologies Summary Response Fusion facilities, both research and development stage, and future commercial power producing systems, will have radiation hazards driven by three factors: • Inventory of volatile radioactive substances, primarily tritium • Prompt exposure to neutron or high energy photon flux from a fusion reaction • Radioactivity from decay of materials activated by fusion neutron flux The magnitudes of these radiation hazards will depend on the specific fusion technology and the nature of the system. Large volume magnetic fusion systems, for example, may have higher tritium inventories than pulsed approaches. Similarly, neutron and photon energy flux will depend on the design of blanket and shielding systems that may be technology specific. While total tritium inventory at any one time is unlikely to create a high accidental release risk to the public, total annual tritium throughput in a fusion power plant will be relatively high (a 500 MWt fusion plant will need to produce and consume ~30 kg of tritium per year). The management and containment of tritium flows during regular operation is therefore likely to be the most important area of interest for regulators.