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Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

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Page 1: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 2: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Dr Ian FalconerDr Ian Falconer

School of Physics, University of SydneySchool of Physics, University of Sydney

Some of the slides shown in this presentation were provided by:

Dr Joe Khachan, University of Sydney

Professor John O’Connor, University of Newcastle

I gratefully acknowledge their permission to use these slides

Page 3: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 4: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Fusion:

our energy future?

Page 5: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

FUSION

• The energy that drives the stars

• Can it also be harnessed on earth to provide the energy our society needs?

Page 6: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

• The world has real energy problems (And fusion energy MUST be a big part of the solution)

• What is fusion?

• How do we harness fusion energy?

Why fusion?

And what IS fusion?

Page 7: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

The world is running out of (cheap) energy - i.e. fossil fuels

and CO2 from fossil fuels is a greenhouse gas

For these reasons, we URGENTLY need a energy source to replace fossil fuels

(and it must be “portable” - like petrol – so it can be used in cars and trucks)

Page 8: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 9: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

The world has real energy problems

• We are fast running out of oil (and natural gas)

• Burning of fossil fuels generates carbon dioxide (CO2) For every tonne of oil or coal used for generating energy, around THREE tonnes of CO2 are generated

• Per capita energy consumption increases as nations become wealthier Think about India and China

Page 10: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

The case for fusion energy : standard of living

Growth of Australia’s Primary energy consumption and GDP

Page 11: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

The case for fusion energy : standard of living

Page 12: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

The case for fusion energy : standard of living

Page 13: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

How long will it last?How long will it last?

Oil ~50-100 years

Natural gas ~60-100 years

Nuclear fission energy (U235 burners) 50 to ~100 years

Nuclear fission energy (breeder reactors)

Thousands of years

Solar, wind, tidal energy Renewable

Fusion energy Millenia

Page 14: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

• We have only limited oil and natural gas resources

Not only do these fuels generate CO2, but are a valuable feedstock for the chemical industry

• The combustion of coal must necessarily generate the greenhouse gas CO2

• Nuclear energy is another limited resource, and waste disposal and proliferation are problematic – at least politically

• The “renewables” are intermittent resources, which require extensive – and expensive - energy storage capacity if the are to provide energy “on tap”

Fusion energy MUST be part of the solutionFusion energy MUST be part of the solution

Page 15: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

What is fusion?

Page 16: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Fusion energy powers the SunFusion energy powers the Sun

Page 17: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Chemically these isotopes are the same, but the deuterium and tritium store considerable energy in their nuclei – this is the energy that holds the nuclei together

• The release of the energy stored in the nuclei of “heavy hydrogen” atoms - deuterium and tritium Hydrogen: nucleus consists of 1 proton Deuterium: nucleus consists of 1 proton and 1 neutron Tritium: nucleus consists of 1 proton and 2 neutrons

What is fusion? What is fusion?

Page 18: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

The Most Promising Fusion Reaction

Page 19: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

D-D Fusion Reaction

Proton

Neutron

Page 20: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Where do the fuels come from?

Deuterium is present in all “natural” hydrogen. There is 1 atom of deuterium for every 6,000 atoms of hydrogen. Water is thus an abundant source of deuterium

Tritium also occurs naturally, but in a fusion reactor will be created by bombarding a blanket of lithium surrounding the core of the reactor

Lithium is also abundant in nature: Australia has 60% of the world’s proven lithium reserves

Page 21: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

“Breeding” tritium

Lithium + neutron → Tritium + Helium + ENERGY

Liquid lithium will be used as a coolant in fusion reactors. It will absorb the energy of the neutrons, and at the same time “breed” tritium and produce more energy

Page 22: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 23: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

How do we harness fusion energy?

Page 24: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

How do we harness fusion energy?

• Bang a deuterium nucleus and a tritium nucleus HARD together so they “fuse”

• A mixture of deuterium and tritium gases must be heated to a very high temperature if the nuclei are to “fuse” – about 100 million degrees! Under these conditions all the atoms are ionized and form a PLASMA

• These high temperatures can only be achieved if the gases are contained in a “bottle” constructed from a really strong magnetic field

• And a high density of colliding nuclei is required if we are to get more fusion energy from the reactor than we put into it

Page 25: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Magnetic Confinement

Page 26: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Toroidal field produces greater confinement

Page 27: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Tokamak confinement

Page 28: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Inside a TOKAMAK

Page 29: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Tokamak Operating

Page 30: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Q = Pout /Pin ~1

• “Breakeven” regime :

Eg. Joint European Tokamak : 1983 -

• “Ignition” regime, fully self-sustained : Power Plant.

• “Burning” regime : plasma dominantly self-heated by fusion born alpha’s

1997 : Q=0.7, 16.1MW fusion

Progress in magnetically confined fusion

ITER

Page 31: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

ITER – “the way”International Thermonuclear Experimental Reactor

An international project to produce a prototype fusion reactor

ITER partners

• European Union

• Japan

• China

• Russian Federation

• USA

• Korea

• India

• (and possibly Brazil – and Canada, Mexico and Kazakhstan)

Page 32: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

The ITER project

• Fusion power = 500MW• Power Gain > 10• Temperature ~ 80 million C

Construction cost $10 billion, 10 year operation $6 billionFiscally, world’s largest science experiment

Cadarache, France

•Consortium of 7 nations

Page 33: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

ITER

Person

ITER – the next generation tokamakDesign completed – construction has just commenced

Page 34: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Aims of the ITER project• Produce and study inductively-driven, burning plasma at

Q =Pout/Pin 10 (400-500 MW) for an “extended” time, ~ 400 s

• Produce and study burning plasma with non-inductive drive Q 5

• Integrate essential fusion reactor technologies: superconducting magnets, high heat flux components, remote handling

• Test reactor components: eg tritium breeding module concepts (neutron power load > 0.5 MW m-2, fluence > 0.3 MW year m-2).

Page 35: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Fusion is part of our Energy Future

But ….. When?

2016 First plasma

2020 First DT “burn”

2021 Q = 10

2024 Construction of DEMO to commence

2033 Operation of DEMO to commence

2045 Construction of power plant to commence

2055? Power plants operates!!!

Page 36: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

NOW ASSEMBLY STARTS FIRST PLASMA

Page 37: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Source: Accelerated development of fusion power. I. Cook et al. 2005

2005 20502020

ITER

today’s experiments

materials testing facility (IFMIF)

demonstration power-plant (DEMO)

commercial power-plants

R &D on alternative concepts and advanced materials

2010 2015 2025 2030 2035 2040 2045

Beyond ITER…

Page 38: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Comparison to CPU transistors

Page 39: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

The pros and cons of fusion energyThe pros and cons of fusion energy

PRO

• “Unlimited” fuel supply

• Little waste produced

CON

• Relatively expensive (High construction and maintenance costs)

• Structure highly radioactive – for a short time

Page 40: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

0.0

01 $

/ kW

hr

internal costs: costs of constructing, fuelling, operating, and disposing of power stations

external costs: “estimated” impact costs to the environment, public and worker health,

Prospects for fusion electricity, I. Cook et al. Fus. Eng. & Des. 63-34, pp25-33, 2002

The case for fusion energy : fusion economics

Page 41: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Fusion: a safe, relatively inexpensive source of energy for which we have an inexhaustible supply of fuel

ITER is – undoubtedly – “the way”

Page 42: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

Why isn’t Australia – pioneers in the field of fusion physics -

involved in the ITER project??

Page 43: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

THE END

Page 44: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of

LHC: the Large Hadron Collider

7 TeV = 7,000,000,000,000 eV

Page 45: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 46: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 47: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 48: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 49: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 50: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of
Page 51: Dr Ian Falconer School of Physics, University of Sydney Some of the slides shown in this presentation were provided by: Dr Joe Khachan, University of