Controlled Thermonuclear Fusion

Similar documents
The Path to Fusion Energy creating a star on earth. S. Prager Princeton Plasma Physics Laboratory

Magnetic Confinement Fusion and Tokamaks Chijin Xiao Department of Physics and Engineering Physics University of Saskatchewan

Introduction to Fusion Physics

Chapter IX: Nuclear fusion

Magnetic Confinement Fusion-Status and Challenges

Physics & Engineering Physics University of Saskatchewan. Supported by NSERC, CRC

Der Stellarator Ein alternatives Einschlusskonzept für ein Fusionskraftwerk

INTRODUCTION TO MAGNETIC NUCLEAR FUSION

Neutron Sources Fall, 2017 Kyoung-Jae Chung Department of Nuclear Engineering Seoul National University

A Faster Way to Fusion

General Physics (PHY 2140)

TWO FUSION TYPES NEUTRONIC ANEUTRONIC

Unpressurized steam reactor. Controlled Fission Reactors. The Moderator. Global energy production 2000

PARTICLE PHYSICS :Higher Level Long Questions

Toward the Realization of Fusion Energy

Recent Development of LHD Experiment. O.Motojima for the LHD team National Institute for Fusion Science

Stellarators. Dr Ben Dudson. 6 th February Department of Physics, University of York Heslington, York YO10 5DD, UK

Leptons and Weak interactions

The Sun Our Nearest Star The Sun is an average star in mass, lifetime, and energy output. We will look at in detail before studying stars in general

Nuclear Physics and Radioactivity

The Sun = Typical Star

The Dynomak Reactor System

Turbulence and Transport The Secrets of Magnetic Confinement

Mega-Science research infrastructure

A Technology Review of Electricity Generation from Nuclear Fusion Reaction in Future

Lecture 14, 8/9/2017. Nuclear Reactions and the Transmutation of Elements Nuclear Fission; Nuclear Reactors Nuclear Fusion

Prospects of Nuclear Fusion Energy Research in Lebanon and the Middle-East

References and Figures from: - Basdevant, Fundamentals in Nuclear Physics

MHD. Jeff Freidberg MIT

11/19/08. Gravitational equilibrium: The outward push of pressure balances the inward pull of gravity. Weight of upper layers compresses lower layers

A brief history of neutrino. From neutrinos to cosmic sources, DK&ER

Current density modelling in JET and JT-60U identity plasma experiments. Paula Sirén

Hans Albrecht Bethe (1906- Nobel Prize for Physics (1967)

Possibilities for Long Pulse Ignited Tokamak Experiments Using Resistive Magnets

Exhaust scenarios. Alberto Loarte. Plasma Operation Directorate ITER Organization. Route de Vinon sur Verdon, St Paul lez Durance, France

PHY492: Nuclear & Particle Physics. Lecture 8 Fusion Nuclear Radiation: β decay

Tokamak Fusion Basics and the MHD Equations

Reading Clicker Q 2/7/17. Topics for Today and Thur. ASTR 1040: Stars & Galaxies

β and γ decays, Radiation Therapies and Diagnostic, Fusion and Fission Final Exam Surveys New material Example of β-decay Beta decay Y + e # Y'+e +

purposes is highly encouraged.

Fast ion physics in the C-2U advanced, beam-driven FRC

AST 301 Introduction to Astronomy

Nuclear Energy; Effects and Uses of Radiation

Neutral beam plasma heating

Chapter 12. Magnetic Fusion Toroidal Machines: Principles, results, perspective

NUCLEI. Atomic mass unit

EF2200 Plasma Physics: Fusion plasma physics

M. Cobal, PIF 2006/7. Quarks

Welcome to the XXVIII (18th) NUFACT Workshop QUY NHON, Vietnam August 2016 Neutrino Physics with Accelerators

Nuclear Reactions. Fission Fusion

6-8 February 2017 Hotel do Mar Sesimbra. Hands on Neutrinos

Jim s early days: Brookhaven, Princeton, and the CP Discovery. September 30, 2016 Stewart Smithx

INTRODUCTION TO BURNING PLASMA PHYSICS

energy loss Ionization + excitation of atomic energy levels Mean energy loss rate de /dx proportional to (electric charge) 2 of incident particle

Nuclides with excess neutrons need to convert a neutron to a proton to move closer to the line of stability.

Atomic physics in fusion development

Matter, Antimatter and the Strangeness of CP violation

Plasma Physics and Fusion Energy Research

Plasma & Fusion on Earth: merging age-old natural phenomena into your present and future

Neutrino vs antineutrino. Lepton number

Alpha-particle physics in the tokamak fusion test reactor DT experiment


Cosmic Rays - R. A. Mewaldt - California Institute of Technology

for the French fusion programme

Perspective on Fusion Energy

What is matter and how is it formed?

The Physics of Cosmic Rays

PHYS:1200 LECTURE 36 ATOMIC AND NUCLEAR PHYSICS (4)

Nuclear Energy 6/04/08. Lecture 22 1

Physics of fusion power. Lecture 14: Anomalous transport / ITER

Nuclear Fusion. STEREO Images of Extreme UV Radia6on at 1 Million C

M. Cobal, PIF 2006/7. Quarks

DIAGNOSTICS FOR ADVANCED TOKAMAK RESEARCH

Overview of Tokamak Rotation and Momentum Transport Phenomenology and Motivations

Compact, spheromak-based pilot plants for the demonstration of net-gain fusion power

Physics 2D Lecture Slides Jan 22. Vivek Sharma UCSD Physics

1. What does this poster contain?

Nuclear Fusion Energy Research at AUB Ghassan Antar. Physics Department American University of Beirut

Elementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016

TRANSP Simulations of ITER Plasmas

Jack Steinberger Learning About Particles 50 Privileged Years

Toroidal confinement of non-neutral plasma. Martin Droba

The Spherical Tokamak as a Compact Fusion Reactor Concept

Plasma Wall Interactions in Tokamak

Chapter 30. Nuclear Energy and Elementary Particles

The extrapolation of the experimentally measured energy confinement time in existing tokamaks towards ITER is considered to be robust because the

A Passion for Plasma Physics and Nuclear Fusion Research. K. A. Connor Plasma Dynamics Laboratory ECSE Department RPI

Relevant spatial and time scale in tokamaks. F. Bombarda ENEA-Frascati, FSN-FUSPHY-SAD

Introduction to Nuclear Fusion. Prof. Dr. Yong-Su Na

PCES 5.1. Kaiser Wilhelm Institute (Berlin) in Hahn & Strassmann the discovery of nuclear fission in Berlin (1938)

Neutrinos and the Universe

Bold Step by the World to Fusion Energy: ITER

ASTR 200 : Lecture 20. Neutron stars

Lecture 14 Cosmic Rays

PFC/JA NEUTRAL BEAM PENETRATION CONSIDERATIONS FOR CIT

Nuclear Physics and Astrophysics

OpenStax-CNX module: m Fusion * OpenStax. Abstract Dene nuclear fusion. Discuss processes to achieve practical fusion energy generation.

STUDY OF ADVANCED TOKAMAK PERFORMANCE USING THE INTERNATIONAL TOKAMAK PHYSICS ACTIVITY DATABASE

Ryan Stillwell Paper: /10/2014. Neutrino Astronomy. A hidden universe. Prepared by: Ryan Stillwell. Tutor: Patrick Bowman

Agenda for Ast 309N, Sep. 6. The Sun s Core: Site of Nuclear Fusion. Transporting Energy by Radiation. Transporting Energy by Convection

Transcription:

Controlled Thermonuclear Fusion Roscoe White Plasma Physics Laboratory, Princeton University

The promise of cheap clean energy Consistently twenty years off, for the last 60 years Research began at Princeton with project Matterhorn in 1951 In 1950 Sakharov and Tamm sketched a tokamak design. Declassified 1958, Geneva conference on Atomic Energy D + T H 4 e (3.5MeV ) + n(14.1mev) ntτ E > 3 10 21 kev s/m 3

Much progress made since 1 KeV plasma in Kurchatov T-3 1968 1994 at PPPL in Princeton and at JET in Abingdon fusion power out equalled roughly half of the heating power in. Fusion power in KW has increased more rapidly than computer speed. Princeton was in the 90 s the hottest place in the solar system, 200 million degrees, more than 20 times the interior of the sun, with a plasma volume of cubic meters. Tile wall at 1000 degrees, as on shuttle. Stable discharges have run for minutes, Heating is no problem with neutral beams, But need all three, Temperature, density, confinement time, implies large size.

Nuclear Physics- came to US with Oppenheimer, Bethe, Wheeler, Fermi Chicago PhDs of Enrico Fermi, 1941-1950 s Owen Chamberlain - A-bomb - Berkeley - Nobel Prize for anti-protons Goeffery Chew - Scattering Matrix, Berkeley Mildred Dresselhaus - Carbon nanotubes, MIT Jerome Friedman - MIT - Nobel Prize for discovery of quarks Marvin Goldberger - π meson decay, Princeton University Tsung Dao Lee - Columbia - Nobel Prize for parity violation James Rainwater - A-bomb, Columbia - Nobel Prize asymm. nuclei Marshall Rosenbluth - H-bomb, Thermonuclear fusion- Princeton IAS Arthur Rosenfeld - Berkeley, development of bubble chamber Jack Steinberger - Columbia - Nobel Prize for muon neutrino Sam Treiman - cosmic rays, weak interactions, Princeton University Paul and I are grandsons of Enrico Fermi

Why has it taken so long? The initial expectation was that fusion could be solved in 20 years The first 20 years were experiments with small systems, incapable of obtaining good confinement or high temperatures. Once the tokamak was discovered (1968) and temperatures increased, confinement improved. Stable equilibrium was obtained and understood, Grad-Shafranov The magnetic field containing the plasma, when the plasma density and temperature are significant, begins to thrash and kink. With good confinement and high densities, losses, instabilities were discovered, analyzed theoretically (occasionally first!), and defeated. A long list - Kink mode, Sawtooth, Fishbone, Ripple, Tearing, TAE A course in fusion theory proceeds from equilibrium analysis through the list of instabilities and finally to transport in the stable system.

The 20 billion dollar international reactor size next step - ITER Tokamak under construction outside Aix en Provence, in Cadarache, where France makes its nuclear submarine engines. Should produce net energy, maybe a factor of 10 over input. BUT Too costly, does not extrapolate to an economic reactor. Fuel cost is negligible, the cost of power hinges entirely on the cost and lifetime of the reactor.

Stellarators offer a steady state plasma but are more complex Tokamaks are axially symmetric, but the poloidal field is produced by transformer induced plasma current, pulsed, not steady state. First high energy plasmas were achieved with tokamaks in USSR. Initial attempts at Princeton were with stellarators and leaked, only low temperatures. But with new computer simulation capabilities designs can overcome the leakage. Wendelstein 7X - construction in Greifswald, Germany, PLASMA 2015.

A new idea that might work, leading to smaller, better, cheaper Zi Plasma 80 kev T << 16 kev turbulent thermo conduction D D + Recycling Plasma 16 kev Li PFC 80 kev NBI D + diffusive energy and particle losses Plasma column heated by 80 KeV Neutral beam injection. High recycling as in present devices, T small at edge, large gradient. A pumping wall, utilizing liquid lithium and making the wall invisible to the plasma, giving small temperature gradient, low turbulence. Some experiments in Princeton, Intensly pursued in China. Success woud dramatically reduce size and cost of a reactor.

The Future The US program is slow, with small participation in ITER Unfortunately the long time scale of the research does not help Time scale for progress is longer than congressional election periods. Costs of ITER threaten to destroy the domestic program Intense effort under way in China, Korea, Japan and now India with plans to build a demonstration reactor A small ignition device IGNITOR is a proposed collaboration between Italy and Russia, but problems in Ukraine give it an uncertain future. Princeton admits about 7 grad students per year, but only some of them work on fusion, we are barely keeping up an educated cadre of professionals who know fusion theory. It is essential to reduce the size and cost of a reactor