Thermonuclear AB-Reactors for Aerospace
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The Fork in the Road to Electric Power from Fusion US Navy Compact
The Fork in the Road to Electric Power From Fusion US Navy compact fusion reactors Peter Lobner, 1 February 2021 1. Background For at least the past 40 years, the US Navy has been funding fusion power research and development in considerable secrecy. In this article, we’ll take a brief look at the following US Navy fusion programs, focusing on the two most recent programs. • LINUS - pulsed stabilized liquid liner compressor (SLC) • Low Energy Nuclear Reactions (LENR, aka cold fusion) • Polywell fusion - inertial electrostatic confinement (IEC) • NIKE & Electra krypton fluoride direct-drive laser inertial confinement fusion (ICF) • Plasma compression fusion device (2019) • Argon fluoride direct-drive laser ICF (2020) 2. LINUS - pulsed stabilized liquid liner compressor (SLC) In the 1970s, this Naval Research Laboratory (NRL)-sponsored project developed and tested several pulsed stabilized liquid liner compressor (SLC) machines: LINUS-0, SUZY-II and HELIUS. A plasma is injected into a void space in a flowing molten lead-lithium liner. The liquid liner is then imploded mechanically, using high- pressure helium-driven pistons. The imploding liner compresses and adiabatically heats the plasma to fusion conditions. While the SLC concept was abandoned by the US Navy in the 1970s, it was revived in the 2000s as the basis for the small fusion reactor designs being developed by Compact Fusion Systems (US) and General Fusion (Canada). 3. Low Energy Nuclear Reactions (LENR, aka cold fusion) From the mid 1990s to at least the mid-2000s the US Navy sponsored research into cold fusion. You’ll find a list of cold fusion papers by Navy researchers from NRL, China Lake Naval Weapons 1 The Fork in the Road to Electric Power From Fusion Laboratory, and Space and Naval Warfare Systems Center (SPAWAR) here: https://lenr-canr.org/wordpress/?page_id=952 4. -
Controlled Nuclear Fusion
Controlled Nuclear Fusion HANNAH SILVER, SPENCER LUKE, PETER TING, ADAM BARRETT, TORY TILTON, GABE KARP, TIMOTHY BERWIND Nuclear Fusion Thermonuclear fusion is the process by which nuclei of low atomic weight such as hydrogen combine to form nuclei of higher atomic weight such as helium. two isotopes of hydrogen, deuterium (composed of a hydrogen nucleus containing one neutrons and one proton) and tritium (a hydrogen nucleus containing two neutrons and one proton), provide the most energetically favorable fusion reactants. in the fusion process, some of the mass of the original nuclei is lost and transformed to energy in the form of high-energy particles. energy from fusion reactions is the most basic form of energy in the universe; our sun and all other stars produce energy through thermonuclear fusion reactions. Nuclear Fusion Overview Two nuclei fuse together to form one larger nucleus Fusion occurs in the sun, supernovae explosion, and right after the big bang Occurs in the stars Initially, research failed Nuclear weapon research renewed interest The Science of Nuclear Fusion Fusion in stars is mostly of hydrogen (H1 & H2) Electrically charged hydrogen atoms repel each other. The heat from stars speeds up hydrogen atoms Nuclei move so fast, they push through the repulsive electric force Reaction creates radiant & thermal energy Controlled Fusion uses two main elements Deuterium is found in sea water and can be extracted using sea water Tritium can be made from lithium When the thermal energy output exceeds input, the equation is self-sustaining and called a thermonuclear reaction 1929 1939 1954 1976 1988 1993 2003 Prediction Quantitativ ZETA JET Project Japanese Princeton ITER using e=mc2, e theory Tokomak Generates that energy explaining 10 from fusion is fusion. -
Can 250+ Fusions Per Muon Be Achieved?
CAN 250+ FUSIONS PER MUON BE ACHIEVED? CONF-870448—1 Steven E. Jones DE87 010472 Brigham Young University Dept. of Physics and Astronomy Provo, UT 84602 U.S.A. INTRODUCTION Nuclear fusion of hydrogen isotopes can be induced by negative muons (u) in reactions such as: y- + d + t + o + n -s- u- (1) t J N This reaction is analagous to the nuclear fusion reaction achieved in stars in which hydrogen isotopes (such as deuterium, d, and tritium, t) at very high temperatures first penetrate the Coulomb repulsive barrier and then fuse together to produce an alpha particle (a) and a neutron (n), releasing energy which reaches the earth as light and heat. Life in the universe depends on fusion energy. In the case of reaction (1), the muon in general reappears after inducing fusion so that the reaction can be repeated many (N) times. Thus, the muon may serve as an effective catalyst for nuclear fusion. Muon- catalyzed fusion is unique in that it proceeds rapidly in deuterium-tritium mixtures at relatively cold temperatures, e.g. room temperature. The need for plasma temperatures to initiate fusion is overcome by the presence of the nuon. In analogy to an ordinary hydrogen molecule, the nuon binds together the deuteron and triton in a very small molecule. Since the muonic mass is so large, the dtp molecule is tiny, so small that the deuteron and triton are induced to fuse together in about a picosecond - one millionth of the nuon lifetime. We could speak here of nuonlc confinement, in lieu of the gravitational confinement found in stars, or MASTER DISTRIBUTION OF THIS BBCUMENT IS UNLIMITED magnetic or inertial confinement of hot plasmas favored in earth-bound attempts at imitating stellar fusion. -
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. -
Simulation of a Device Providing Nuclear Fusion by Electrostatic Confinement, with Multiplasma
1 Simulation of a device providing nuclear fusion by electrostatic confinement, with Multiplasma Copyright © 2018 Patrick Lindecker Maisons-Alfort (France) 22th of July 2018 Revision B Revision B: replacement of the term « efficiency » by « yield » to avoid an ambiguity and the aneutronic fusion H+ <-> B11+ taken into account. 1. Goal To design your own electrostatic confinement nuclear fusion reactor. It is addressed to people interested by nuclear fusion, having a good general culture in physics (and who are patient because simulations can be long). It is set aside the fact that your project is physically achievable or not. 2. Warning This design will be just for the « fun » or from curiosity, because even if the calculations done by Multiplasma are as serious as possible, in the limit of the knowledge of the author (who is not a nuclear physicist but a generalist engineer), of course, nobody is going to build your nuclear reactor… Otherwise, none checking has been made by another person and the program development does not follow any quality assurance process (so there are probably a lot of errors). It is just a personal program made available to those interested by this subject. 3. Brief explanations of a few of the terms used: Deuterium (D or D2) / Tritium (T or T2): these are hydrogen isotopes comprising, besides one proton, either one neutron (Deuterium) or 2 neutrons (Tritium). As other elements, they are susceptible to produce fusions by collisions. The Deuterium is relatively abundant, in sea water, for example. It constitutes 0.01 % of hydrogen. The tritium is naturally present at traces 2 amounts but it is produced (as a gaseous effluent) by fission nuclear centrals, in very small quantities. -
Trivia Questions
TRIVIA QUESTIONS Submitted by: ANS Savannah River - A. Bryson, D. Hanson, B. Lenz, M. Mewborn 1. What was the code name used for the first U.S. test of a dry fuel hydrogen bomb? Castle Bravo 2. What was the name of world’s first artificial nuclear reactor to achieve criticality? Chicago Pile-1 (CP-1), I also seem to recall seeing/hearing them referred to as “number one,” “number two,” etc. 3. How much time elapsed between the first known sustained nuclear chain reaction at the University of Chicago and the _____ Option 1: {first use of this new technology as a weapon} or Option 2: {dropping of the atomic bomb in Hiroshima} A3) First chain reaction = December 2nd 1942, First bomb-drop = August 6th 1945 4. Some sort of question drawing info from the below tables. For example, “what were the names of the other aircraft that accompanied the Enola Gay (one point for each correct aircraft name)?” Another example, “What was the common word in the call sign of the pilots who flew the Japanese bombing missions?” A4) Screenshots of tables from the Wikipedia page “Atomic bombings of Hiroshima and Nagasaki” Savannah River Trivia / Page 1 of 18 5. True or False: Richard Feynman’s name is on the patent for a nuclear powered airplane? (True) 6. What is the Insectary of Bobo-Dioulasso doing to reduce the spread of sleeping sickness and wasting diseases that affect cattle using a nuclear technique? (Sterilizing tsetse flies; IAEA.org) 7. What was the name of the organization that studied that radiological effects on people after the atomic bombings? Atomic Bomb Casualty Commission 8. -
Article Thermonuclear Bomb 5 7 12
1 Inexpensive Mini Thermonuclear Reactor By Alexander Bolonkin [email protected] New York, April 2012 2 Article Thermonuclear Reactor 1 26 13 Inexpensive Mini Thermonuclear Reactor By Alexander Bolonkin C&R Co., [email protected] Abstract This proposed design for a mini thermonuclear reactor uses a method based upon a series of important innovations. A cumulative explosion presses a capsule with nuclear fuel up to 100 thousands of atmospheres, the explosive electric generator heats the capsule/pellet up to 100 million degrees and a special capsule and a special cover which keeps these pressure and temperature in capsule up to 0.001 sec. which is sufficient for Lawson criteria for ignition of thermonuclear fuel. Major advantages of these reactors/bombs is its very low cost, dimension, weight and easy production, which does not require a complex industry. The mini thermonuclear bomb can be delivered as a shell by conventional gun (from 155 mm), small civil aircraft, boat or even by an individual. The same method may be used for thermonuclear engine for electric energy plants, ships, aircrafts, tracks and rockets. ----------------------------------------------------------------------- Key words: Thermonuclear mini bomb, thermonuclear reactor, nuclear energy, nuclear engine, nuclear space propulsion. Introduction It is common knowledge that thermonuclear bombs are extremely powerful but very expensive and difficult to produce as it requires a conventional nuclear bomb for ignition. In stark contrast, the Mini Thermonuclear Bomb is very inexpensive. Moreover, in contrast to conventional dangerous radioactive or neutron bombs which generates enormous power, the Mini Thermonuclear Bomb does not have gamma or neutron radiation which, in effect, makes it a ―clean‖ bomb having only the flash and shock wave of a conventional explosive but much more powerful (from 1 ton of TNT and more, for example 100 tons). -
Cavitation-Induced Fusion: Proof of Concept Vol
1 Fomitchev-Zamilov: Cavitation-Induced Fusion: Proof of Concept Vol. 9 Cavitation-Induced Fusion: Proof of Concept Max I. Fomitchev-Zamilov Quantum Potential Corporation, 200 Innovation Blvd, Suite 254, State College, PA 16803 e-mail: [email protected] Cavitation-induced fusion (also known as bubble fusion or sonofusion) has been a topic of much debate and controversy and is generally (albeit incorrectly) perceived as unworkable. In this paper we present the theoretical foundations of cavitation-induced fusion and summarize the experimental results of the research conducted in the past 20 years. Based on the systematic study of all available data we conclude that the cavitation-induced fusion is feasible, doable, and can be used for commercial power generation. We present the results of our own research and disclose a commercial reactor prototype. threatened), to tenure and promotion issues and academic 1. Introduction misconduct (Krivit, 2011). As a result of the ensuing Nuclear fusion (which powers the sun) is the energy of the “bubblegate” scandal Taleyarkhan’s career was destroyed future: 10 microgram of deuterium is equivalent to a barrel of (Reich, 2009) and CIF research became a taboo. oil. Deuterium is cheap, plentiful and easily extracted from What was forgotten amid the outburst of emotions is that water. Unlike uranium fission in modern nuclear power plants cavitation-induced fusion is a fruitful area of research that must be deuterium fusion does not produce radioactive waste. Yet continued: no less than 7 independent peer-reviewed reports despite 40 years of research and over $20B in government exist demonstrating neutron emissions from collapsing spending (Chu, 2008) on inertial/magnetic confinement cavitation bubbles; even heavily criticized experiments by projects (ICF/MCF) the fusion power remains out of reach: to Taleyarkhan’s group have been successfully repeated (Xu & this date there are no fusion reactors capable of sustained Butt, 2005), (Forringer, Robbins, & Martin, 2006), (Bugg, 2006). -
ITER Aims and Technical Challenges
I and I I - ITER Aims and Technical Challenges Jo Lister CRPP-EPFL Centre de Recherches en Physique des Plasmas Ecole Polytechnique Fédérale de Lausanne Switzerland Outline of the first 2 talks q A previous lecture series was given by Prof. Ambrogio Fasoli q These introduced fusion and ITER but concentrated on the physics q Today and tomorrow we revisit the basic aims and design of ITER, but try to extract the technical challenges, and more importantly, where these challenges come from Jo Lister, CRPP-EPFL, "ITER Technical Challenges" CERN, May/June 2005 2 Remember why we are doing this ! q Finite oil resource thinking was launched by Hubbert in 1956 when he predicted US oil production would peak around 1970 - no-one listened q It did - he was right - US production was allowed at 100% capacity q Now domestic production is decreasing q Idem for world oil, idem for gas Provide a long term energy supply Jo Lister, CRPP-EPFL, "ITER Technical Challenges" CERN, May/June 2005 3 We don’t have a solution for demand exceeding production ! q Swenson’s Law says: “ To avoid deprivation resulting from the exhaustion of non-renewable resources, humanity must employ conservation and renewable resource substitutes sufficient to match depletion.” q One reason no-one important wants to know is that oil depletion might (?) lead to war, famine, plague…. Match supply and demand Jo Lister, CRPP-EPFL, "ITER Technical Challenges" CERN, May/June 2005 4 Fusion physics basics - Nuclear ?? q Where does fusion energy come from ? • The nucleus, B/A is the energy “stored” -
Cold Fusion Again 1 Introduction
Prespacetime Journal j February 2016 j Volume 7 j Issue 2 j pp. 379-396 379 Pitk¨anen,M., Cold Fusion Again Exploration Cold Fusion Again Matti Pitk¨anen 1 Abstract During years I have developed two models of cold fusion and in this article these models are combined together. The basic idea of TGD based model of cold is that cold fusion occurs in two steps. First dark nuclei (large heff = n × h) with much lower binding energy than ordinary nuclei are formed at magnetic flux tubes possibly carrying monopole flux. These nuclei can leak out the system along magnetic flux tubes. Under some circumstances these dark nuclei can transform to ordinary nuclei and give rise to detectable fusion products. An essential additional condition is that the dark protons can decay to neutrons rapidly enough by exchanges of dark weak bosons effectively massless below atomic length scale. Also beta decays in which dark W boson decays to dark electron and neutrino can be considered. This allows to overcome the Coulomb wall and explains why final state nuclei are stable and the decay to ordinary nuclei does not yield only protons. Thus it seems that this model combined with the TGD variant of Widom-Larsen model could explain nicely the existing data. In this chapter I will describe the steps leading to the TGD inspired model for cold fusion combining the earlier TGD variant of Widom-Larsen modelwith the model inspired by the TGD inspired model of Pollack's fourth phase of water using as input data findings from laser pulse induced cold fusion discovered by Leif Holmlid and collaborators. -
The Stellarator Program J. L, Johnson, Plasma Physics Laboratory, Princeton University, Princeton, New Jersey
The Stellarator Program J. L, Johnson, Plasma Physics Laboratory, Princeton University, Princeton, New Jersey, U.S.A. (On loan from Westlnghouse Research and Development Center) G. Grieger, Max Planck Institut fur Plasmaphyslk, Garching bel Mun<:hen, West Germany D. J. Lees, U.K.A.E.A. Culham Laboratory, Abingdon, Oxfordshire, England M. S. Rablnovich, P. N. Lebedev Physics Institute, U.S.3.R. Academy of Sciences, Moscow, U.S.S.R. J. L. Shohet, Torsatron-Stellarator Laboratory, University of Wisconsin, Madison, Wisconsin, U.S.A. and X. Uo, Plasma Physics Laboratory Kyoto University, Gokasho, Uj', Japan Abstract The woHlwide development of stellnrator research is reviewed briefly and informally. I OISCLAIWCH _— . vi'Tli^liW r.'r -?- A stellarator is a closed steady-state toroidal device for cer.flning a hot plasma In a magnetic field where the rotational transform Is produced externally, from torsion or colls outside the plasma. This concept was one of the first approaches proposed for obtaining a controlled thsrtnonuclear device. It was suggested and developed at Princeton in the 1950*s. Worldwide efforts were undertaken in the 1960's. The United States stellarator commitment became very small In the 19/0's, but recent progress, especially at Carchlng ;ind Kyoto, loeethar with «ome new insights for attacking hotii theoretics] Issues and engineering concerns have led to a renewed optimism and interest a:; we enter the lQRO's. The stellarator concept was borr In 1951. Legend has it that Lyman Spiczer, Professor of Astronomy at Princeton, read reports of a successful demonstration of controlled thermonuclear fusion by R. -
Formation of Hot, Stable, Long-Lived Field-Reversed Configuration Plasmas on the C-2W Device
IOP Nuclear Fusion International Atomic Energy Agency Nuclear Fusion Nucl. Fusion Nucl. Fusion 59 (2019) 112009 (16pp) https://doi.org/10.1088/1741-4326/ab0be9 59 Formation of hot, stable, long-lived 2019 field-reversed configuration plasmas © 2019 IAEA, Vienna on the C-2W device NUFUAU H. Gota1 , M.W. Binderbauer1 , T. Tajima1, S. Putvinski1, M. Tuszewski1, 1 1 1 1 112009 B.H. Deng , S.A. Dettrick , D.K. Gupta , S. Korepanov , R.M. Magee1 , T. Roche1 , J.A. Romero1 , A. Smirnov1, V. Sokolov1, Y. Song1, L.C. Steinhauer1 , M.C. Thompson1 , E. Trask1 , A.D. Van H. Gota et al Drie1, X. Yang1, P. Yushmanov1, K. Zhai1 , I. Allfrey1, R. Andow1, E. Barraza1, M. Beall1 , N.G. Bolte1 , E. Bomgardner1, F. Ceccherini1, A. Chirumamilla1, R. Clary1, T. DeHaas1, J.D. Douglass1, A.M. DuBois1 , A. Dunaevsky1, D. Fallah1, P. Feng1, C. Finucane1, D.P. Fulton1, L. Galeotti1, K. Galvin1, E.M. Granstedt1 , M.E. Griswold1, U. Guerrero1, S. Gupta1, Printed in the UK K. Hubbard1, I. Isakov1, J.S. Kinley1, A. Korepanov1, S. Krause1, C.K. Lau1 , H. Leinweber1, J. Leuenberger1, D. Lieurance1, M. Madrid1, NF D. Madura1, T. Matsumoto1, V. Matvienko1, M. Meekins1, R. Mendoza1, R. Michel1, Y. Mok1, M. Morehouse1, M. Nations1 , A. Necas1, 1 1 1 1 1 10.1088/1741-4326/ab0be9 M. Onofri , D. Osin , A. Ottaviano , E. Parke , T.M. Schindler , J.H. Schroeder1, L. Sevier1, D. Sheftman1 , A. Sibley1, M. Signorelli1, R.J. Smith1 , M. Slepchenkov1, G. Snitchler1, J.B. Titus1, J. Ufnal1, Paper T. Valentine1, W. Waggoner1, J.K. Walters1, C.