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Creating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute for Fusion Studies (UT), Princeton Plasma Physics Laboratory, MIT Plasma Science and Fusion Center, and General Atomics for advice and graphics. Thanks to SOHO web site for pictures of sun. Fusion research is funded by the US Department of Energy
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Page 1: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Creating a Star on the Earth

The challenge of fusion energy

Thanks to colleagues at Institute for Fusion Studies (UT), Princeton Plasma Physics Laboratory, MIT Plasma Science and Fusion Center, and General Atomics for advice and graphics.

Thanks to SOHO web site for pictures of sun.

Fusion research is funded by the US Department of Energy

Page 2: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

What are we looking at?

Why do we care?

Page 3: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

We are looking at...

1. A hot plasma,

2. Held together (“confined”) by gravity,

3. Powered by nuclear fusion.

Page 4: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

We care (because its

interesting and) because...

• Exploding global demand for electric power

• Unacceptable climate change from fossil fuels

• Potentially copious, benign energy source: an earthbound star

Page 5: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Some laboratory stars:

TFTR device at Princeton

Break-even fusion energy production,

1994.

Page 6: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

DIII-D toroidal device (tokamak) at General Atomics

Page 7: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Tokamak

General Atomics

Spherical Torus

PPPL (also EU) Superconducting

Stellarator - JA

Superconducting

Stellarator - EU

Superconducting

Tokamak - Korea

Large Tokamak

JA

Large Tokamak

EU

Tokamak

MIT

A Range of Toroidal Magnetic Configurations

is Being Studied WorldwideToroidal proliferation: samples

Page 8: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Joint project ofEU, Japan, Russia, US,

China, Korea, India

ITER (“The Way”)

Construction begins in 2008, in France

Page 9: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Outline of talk

• What is fusion, and how does it provide energy?

• What is plasma, and why does it matter?

• Why are all these devices toroidal (doughnut-shaped)?

• Why bother?

Page 10: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Fusion energy

Start with a basic principle: energy is conserved in every process. In that case...

1. How can energy be created? (Why is there an energy industry?)

2. How can energy be used up? (Why is there an energy crisis?)

Page 11: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Answers:

1. Energy is not created, but found---in the form of fuel.

2. Energy is not destroyed, but dissipated---dispersed into useless heat.

Page 12: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

A theorist’s view of fuel

EoutE in

(return)(investment)

Page 13: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Fuel must be concentrated

Part of the Eout from one reaction becomes Ein for other reactions: the “fire” is maintained.

But fire goes out if fuel is too broadly dispersed.

Page 14: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Where does fuel come from?

Fossil fuels: the sun (photosynthesis)

Fission fuels: nucleosynthesis in stars and supernovae

Fusion fuels: big-bang nucleosynthesis

Page 15: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Two basic facts about fusion fuel

1. Energy output is huge

450Eout X Ein⋲

2. Required energy input is also huge

→ releasing fusion energy isn’t easy

→ fusion energy could have global importance

Ein

Eout

Page 16: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Because Eout is large...

Page 17: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Eout is large because...

Nuclear mass

Energy stored in nucleus

Iron UraniumHydrogen

Fusion energy return

Fission energy return

Eout

Page 18: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

D-T fusion-easiest fusion reaction uses isotopes of hydrogen: deuterium (D) and tritium (T)

-D is plentiful in sea water; T can be manufactured from lithium (also plentiful)

D + T → He + n

Li + n → T + He

-He (helium) is harmless---even useful!

Page 19: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

+

+ +

+

+

+

But note that both fusing particles have positive charge...

Why is Ein large?

D + T → He + n

Page 20: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Two forces between nuclei1. Nuclear force is strongly attractive, but has very short range

2. Electric force is repulsive, with long range

Repulsion of like charges →“Coulomb barrier”

Only very fast nuclei can overcome barrier

D T

+ +

Page 21: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

To fuse, nuclei must collide at high speed: hot nuclear stew

For useful reaction rate, 100 million degrees (hotter than sun).

At even much lower temperatures, atomic electrons and break free from their nuclei: gas becomes plasma---a gas of charged particles

Plasma is “4th state of matter”: stars, lightning, fluorescent lights...

Page 22: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Plasma physics

• Most of the universe is plasma: stars, nebulae, magnetosphere, interstellar space...

• Untamed matter: fierce interaction with electromagnetic fields

• Although basic forces understood, predicting plasma behavior is hard--a long-standing scientific challenge

Page 23: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Plasma physics applies to...

• Structure of stars, planetary atmospheres, most of astrophysics

• Creation of magnetic fields in earth and sun, sunspots, Van Allen belts...

• Various industrial processes, including computer chip manufacture

• New technologies for light, Plasma TV’s...

• Novel space-craft propulsion systems

• ...and fusion research!

Page 24: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

A hot plasma, confined by gravity: long lifetime.

A cooler plasma, not confined: very short lifetime.

Unconfined plasmas disperse and quench.

Two plasmas:

Page 25: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Plasma confinement

Cool plasma is easy to confine

But fusion plasma cannot survive contact with any wall: heat loss quenches plasma (only minor damage to wall).

Page 26: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Gravitational force, directed toward center

Solar plasma confinement:

Gravity holds plasma together, allowing fusion

But gravitational force is proportional to mass:

Solar confinement works because sun is large and massive

Page 27: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Solar corona: a different sort of confinement

Filaments and loops reveal charged particles trapped on magnetic field lines

Magnetic force is independent of mass: acts equally on large and small scales

Page 28: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Magnetic force links plasma (charged particles) to “field lines”

Motion across field lines is tightly constrained; but motion along field lines is not affected. (“2-D confinement.”)

Page 29: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Key to magnetic confinement

Suppose magnetic field lines lie on a surface, rather than wandering through some 3D volume.

A surface covered by magnetic field lines is called a magnetic surface.

A closed magnetic surface will confine plasma.

Page 30: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Magnetic bottle?An arbitrary surface cannot be covered with smooth field lines

Either singular point, or null point, somewhere on surface

?

?

?

Page 31: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Closed magnetic surface must be toroidal

TokamakKrispy Kreme

No ends to cap: field lines cover surface

Page 32: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Summarize: confinement and topology

Gravity→sphere

Magnetism→torus

Page 33: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Tokamak interior

Page 34: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Recall D-T reaction

D + T → He + n

The neutron (n), being neutral, escapes reactor and heats confining vessel. This heat produces steam and then electricity, as in other power plants.

The helium nucleus (He), being charged, remains confined. Its energy helps to keep plasma hot (providing Ein), sustaining reaction.

Page 35: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Not quite so simple...

• Confinement is the main thing, not the only thing

• Tokamaks are the main approach to confinement, not the only approach

• Tokamak confinement is not perfect...only good enough

Page 36: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Confinement is the main thing, not the only thing...

Equilibrium must be stable-historically, the hardest puzzle

Plasma must be heated (energy investment)-induction heating, plus microwave heating

Fuel must be supplied-breeding tritium is an engineering challenge

Etc.

Page 37: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Tokamaks are not the only approach...

Toroids that are not tokamaks: not symmetric about central axis (e.g., stellarator)

Non-toroidal configurations: attempts to stopper the bottle (magnetic mirror)

“Inertial confinement:” laser-compressed fusion firecrackers (NIF)

Page 38: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Magnetic confinement is not perfect

• Collisions between particles cause occasional jumps between neighboring field lines

→ gradual loss of particle and heat

• Magnetic curvature (inter alia) causes slow drifts of particles off field lines

→ enhanced losses

• Residual instabilities cause fluctuating electric fields

→ more serious turbulent heat loss

Page 39: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Yet tokamaks work:

PLTPDXJET

DIII & DIII-D

Princeton Large TokamakPrinceton Divertor ExperimentJoint European TorusGeneral Atomics Tokamak Experiments

TFTRALCATOR C

ITERJT–60U

Princeton Plasma Physics LaboratoryMassachusetts Institute of TechnologyInternational Thermonuclear Experimental ReactorJapanese Tokamak Experiment

TFTR

FUSION POWER

1970 1980 1990 2000 2010

ALCATOR C

PLT

DIII

TFTR JET / TFTR

ITER

Achieved (DD)

Achieved (DT)

Projected (DT)

1,000

100

10

1000

100

10

1000

100

10

1

PDXDIII-D

MWth

kWth

Wth

JET

JT–60U

LIGHT BULB

HOUSE

POWER

PLANT

65

What Progress Has Been MadeWhat Progress Has Been Madein Magnetic Fusion?in Magnetic Fusion?

Page 40: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Recall outline:

• ✔What is fusion?

• ✔What is plasma, and why does it matter?

• ✔Why are all these devices toroidal?

• Why bother?

Page 41: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Fossil fuelsCoal, oil and natural gas now supply 80% of global energy needs

Two problems:

1. depletion of oil and gas

-only coal, the dirtiest fuel of all, will be available in long term

2. climate change

-from dirt and greenhouse gas: global filth and global warming

Page 42: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

A true crisis

• World energy use will double by 2045

• Continued reliance on fossil fuel is certain to cause unacceptable climate change

• Serious R&D program needed to find alternative sources. Present research investment is pitifully small ($3 trillion world energy market)

Page 43: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Alternatives to coal

The usual suspects: improved efficiency, renewables, wind, solar, fission....

All should be pursued, but

• list is too short, given magnitude of problem

• not all items on list seem capable of meeting large fraction of predicted demand

Page 44: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Fusion power• worldwide availability of low-cost fuel,

billion-year supply

• no greenhouse-gas production, no smog, no acid rain

• no possibility of runaway reaction or meltdown

• no proliferation threat: not a credible bomb factory

• only short-lived radioactive wastes (from neutron bombardment of vessel material)

Page 45: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Radioactivity from fusion power plant

Page 46: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

What’s wrong with fusion power?

• large power plant

- might power a city, never a car

• expensive

- costly development path: no table-top stars (plant cost appears comparable to coal-burning plant with same output)

• complicated

- high maintenance?

• there aren’t any fusion power plants!

Page 47: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Why are tokamaks so large?

• Device size determined by required fusion temperature, and by rate of heat loss (surface to volume ratio)

• Heat loss rate determined by plasma turbulence

• Turbulence driven by temperature gradient (“residual instabilities”)

Page 48: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Turbulent heat loss:

Hot plasma bubbles up from interior

No surprise...

Page 49: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Smaller tokamaks?

A focus of present US research: “advanced tokamak”

For example, differential plasma rotation can break turbulent eddies, reducing heat loss. This effect is striking in experiments and reasonably well understood.

A more speculative approach: flat temperature profile (with density fall-off to avoid heat loss to wall) would remove drive for turbulence:

Temperature (flat)

Density (steep)Vessel wall

Page 50: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Summary: logic of an earth-bound star

Everything wants to be iron → nuclear energy source, fission or fusion

Fusion requires close encounters, despite electric repulsion

→ need for hot nuclei→ plasma state

Plasmas are prevalent and interesting

Page 51: Creating a Star on the Earth - Department of Physicsweb2.ph.utexas.edu/spw/hazeltine_091114.pdfCreating a Star on the Earth The challenge of fusion energy Thanks to colleagues at Institute

Summary concluded

• Earthbound scale requires magnetic confinement, which requires

toroidal magnetic surfaces.

• Major challenges remain in the realization fusion power, but

• Fusion’s potential advantages place it

among a small, critically important group

of alternative energy sources.


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