presentation for university of chicago physics colloquium april 3, 2008 burton richter

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1 Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter Freeman Spogli Institute of International Studies Senior Fellow Paul Pigott Professor in the Physical Sciences Emeritus Stanford University and Former Director Stanford Linear Accelerator Center

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Energy in the 21st Century. Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter Freeman Spogli Institute of International Studies Senior Fellow Paul Pigott Professor in the Physical Sciences Emeritus Stanford University and Former Director - PowerPoint PPT Presentation

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Page 1: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

1

Presentation for

University of Chicago Physics ColloquiumApril 3, 2008

Burton RichterFreeman Spogli Institute of International Studies Senior Fellow

Paul Pigott Professor in the Physical Sciences EmeritusStanford University

andFormer Director

Stanford Linear Accelerator Center

Page 2: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

10.000 5,000 0 Years before 2,005

Page 3: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Average Temperature of the Earth

Turn off Greenhouse EffectAll energy radiated from surface escapes.

Average T = -4°F (-20°C).

Turn on Greenhouse EffectPart of energy radiated is blocked.

Surface T goes up so what gets through balances incoming.

Average T = 64°F (15°C).

Page 4: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

2005 was the hottest year on record; the 13 hottest all occurred since 1990, 23 out of the 24 hottest since 1980.

J. Hansen et al., PNAS 103: 14288-293 (26 Sept 2006)

Green bars show 95% confidence intervals

°C

Page 5: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

IIASA Projection of Future Energy Demand Scenario A1 (High

Growth)

Page 6: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Projected Global Average Surface Warming at the End of the 21st Century

Source IPCC 4AR WG1

Case Temperature changes(degrees F) relative to 1980-1999

Best Estimate Range

B1 3.2 2.0 – 5.2A1T 4.3 2.5 – 6.8B2 4.3 2.5 – 6.8

A1B 5.0 3.1 – 7.9

A2 6.1 3.6 – 9.7A1FI 7.2 4.3 – 11.5

Page 7: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter
Page 8: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Removal Time and Percent Contribution to Climate Forcing

AgentRough Removal

Time

Approximate Contribution in

2006Carbon Dioxide >100 years 60%

Methane 10 years 25%Tropospheric Ozone 50 days 20%

Nitrous Oxide 100 years 5%Fluorocarbons >1000 years <1%Sulfate Aerosols 10 days -25%

Black Carbon 10 days +15%

Page 9: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Reference Scenario: World Primary Energy Demand

Global demand grows by more than half over the next quarter of a century, with coal use rising most in absolute terms

Oil

Coal

Gas

BiomassNuclear

Other renewables

0

2 000

4 000

6 000

8 000

10 000

12 000

14 000

16 000

18 000

1970 1980 1990 2000 2010 2020 2030

Mto

e

From International Energy Agency “World Energy Outlook 2006”

Page 10: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Total Primary Energy Supply by Fuel

YearFuel

2005 2030

Oil 35% 33%Coal 25% 26%Gas 21% 23%

Nuclear 6% 5%Other* 12% 12%* = Includes combustibles (10% in 2005), hydro and renewables.

(Source: IEA “Key World Energy Statistics 2007”)

Page 11: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Path for 50% chance of avoiding ∆Tavg >2°C (gold) is much more demanding than path for 50% chance of avoiding >3°C (green).

BAU ( 6°C+)

(~3°C)(~2°C)

CO2 emissions paths: BAU versus stabilizing CO2 concentration to limit ∆Tavg

Page 12: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Primary Power Requirements for 2050 for Scenarios Stabilizing CO2

at 450 ppm and 550 ppm

Source2000 2050

450 ppm 550 ppm

Carbon Based 11 TW 7 TW 12 TW

Carbon Free 3 TW 20 TW 15 TW

M. Hoffert, et al., Nature, 395, p881, (Oct 20, 1998)

Page 13: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

“Science,” 305, 968 (August 13, 2004)

Page 14: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Ready for Large-Scale Deployment Now

Conservation and Efficiency.

Nuclear for Baseload Application.

Ready for Limited Deployment Now

Solar for Daytime Use.

Wind with Back up from Others.

CARBON-FREE ENERGY

Page 15: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter
Page 16: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Energy Intensity and Composite Fuel Price in North America

Page 17: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Power (TW) Required in 2050 Versus Rate of Decline in Energy

Intensity

Page 18: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Carbon Dioxide Intensity andPer Capita CO2 Emissions -- 2001

(Fossil Fuel Combustion Only)

0.00

5.00

10.00

15.00

20.00

25.00

0.00 0.10 0.20 0.30 0.40 0.50 0.60 0.70 0.80 0.90 1.00intensity (tons of CO2 per 2000 US Dollar)

Tons

of C

O2

per p

erso

n

Canada Australia

S. Korea

California

Mexico

United States

Austria

Belgium

Denmark

France

Germany

Italy

Netherlands

New Zealand

Switzerland

Japan

Page 19: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Peak Load vs. Base Load

Peak Load

Base Load

Page 20: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Solar comes in 3 Varieties• Solar Hot Water – simple, cheap, old

fashioned, effective• Solar Photovoltaic – spreading,

expensive, particularly good for small & distributed

• Solar Thermal Electric – large scale, beginning to be deployed more widely

Page 21: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Solar PhotovoltaicExpensive but costs are coming down.

Also has a storage problem (day-night, clouds, etc.).

Some places solar can be important.

In U.S. solar is negligible (less than 10% of wind, mostly in CA).

Page 22: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Solar Thermal Electric• Barstow Solar 2 Power Tower (photo courtesy of NREL)

Page 23: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

WindCommercially viable now (with 1.9¢/kw-hr

subsidy).Nationally about 11,000 Megawatts of installed

capacity (2500 in CA).But, the wind does not blow all the time and

average energy delivered is about 20% of capacity.

Wind cannot be “baseload” power until an energy storage mechanism is found.

Page 24: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter
Page 25: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

EON-NETZ (GERMANY) WIND POWER VARIABILITY

AVERAGE IS 20% OF INSTALLED WIND CAPACITY

Page 26: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Other RenewablesBig Hydroelectric: About 50% developed

world wide.

Geothermal: California, Philippines, and New Zealand are the largest (CA ≈ 1.5 Gigawatts).

Bio Fuel: A very complicated story, and verdict not yet in.

Page 27: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

CoalLargest Fossil Fuel Resource.US & China each have about 25% of world

resources.IF CO2 emitted can be captured and safely

stored underground, problem of reducing Greenhouse Gas emissions is much easier.

Page 28: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

CO2 Sequestration Most study has been on CO2 injection into underground reservoirs. Capacity not well known.

OptionGigaton

CO2

Fraction of Integrated Emissions to 2050

Depleted Gas Fields 690 34%

Depleted Oil Fields 120 6%

Deep Saline Aquifers 400 - 10,000 20% - 500%

Unmineable Coal 40 2%

Page 29: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

FutureGen

$1 Billion Industry-Government Partnership to Generate Electricity & Sequester the CO2.

Page 30: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Area GDP (ppp)(Billions of U.S. Dollars)

CO2/GDPKg/$(ppp)

World 42,400 0.56

France 1,390 0.28

CO2 Intensity(IEA, Key World Energy Statistics 2003)

Page 31: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

World Nuclear Expansion(as of December 2007)

Under construction 34Approved and to be

started 94

Under discussion 222

Total 350

Page 32: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

The Nuclear Critics

It can’t compete in the market place. It is too dangerous.We don’t know what to do with spent

fuel.Proliferation risk is too big to

accept.

Page 33: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

CostsNuclear 1800 €≈$2500/KW (Areva)

Coal $1500 – 2000/KW (EIA)

Wind $1600/KW (peak) (NYT 5/1/07)

$8000/KW (avg.) (20% duty factor)

Solar $5000/KW (peak) (CA Energy Commision)

$25,000/KW (avg.)

Page 34: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Radiation Exposures

SourceRadiation Dose

Millirem/year

Natural Radioactivity 240

Natural in Body (75kg)* 40

Medical (average) 60

Nuclear Plant (1GW electric) 0.004

Coal Plant (1GW electric) 0.003

*Included in the Natural Total

Page 35: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Nuclear AccidentsChernobyl (1986) – World’s Worst

Reactor type not used outside of old Soviet bloc(can become unstable)

Operators moved into unstable region and disabled all safety systems.

Three Mile Island (1979) – A Partial Core MeltdownLWRs are not vulnerable to instabilitiesAll LWRs have containment buildingRadiation in region near TMI about 10 mr.

New LWRs have even more safety systems.

Page 36: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Components of Spent Reactor Fuel

ComponentFission

Fragments UraniumLong-LivedComponent

Per Cent of Total 4 95 1

Radioactivity Intense Negligible Medium

Untreated required isolation time (years) 200 0 300,000

Page 37: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Yucca Mountain Repository Layout

Page 38: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Internationalize the Fuel Cycle

Supplier States: Enrich Uranium

Take back spent fuel

Reprocess to separate Actinides

Burn Actinides in “Fast Spectrum” reactors

User States: Pay for reactors

Pay for enriched fuel

Pay for treatment of spent fuel (?)

Page 39: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Conclusion

Global Warming is real and human activity is the driver.

Not clear how bad it will be with no action, but I have told my kids to move to Canada.

We can do something to limit the effects.

The sooner we start the easier it will be.

Page 40: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Conclusion

Best incentives for action are those that allow industry to make more money by doing the right thing.

Carrots and sticks in combination are required.

The economy as a whole will benefit, but some powerful interests will not.

It is not hard to know what to do, but very hard to get it done.

Page 41: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

The Most Difficult World Problem

What should be the criteria for action?Total emissions? Per capita emissions? Greenhouse gas per unit GDP?

The poorest countries contribute negligibly – Leave them out.

The rapidly developing countries have to be brought in somehow.

The rich countries have to lead the action agenda.

Page 42: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

IEA World Statistics 2005

64

1300

270

6400

Population(Millions)

1.4

2.1

11

36

GDP1

($Trillions)

1.4

8.1

11

55

GDP (PPP)2

($Trillions)

France

China

U.S.

World

0.236.2

0.633.9

0.5319.6

0.504.2

CO2/GDP3

(Kg/$)

CO2per Capita(Tonnes)

(Source: IEA “Key World Energy Statistics 2007”)

1. Nominal exchange rate in constant 2000 dollars.2. Purchasing Power Parity in constant 2000 dollars.3. GDP in PPP terms.

Page 43: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

BACK-UP SLIDES

Page 44: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Quantitative Greenhouse Effect

Page 45: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Source: "Life-Cycle Assessment of Electricity Generation Systems and Applications for Climate Change Policy Analysis," Paul J. Meier, University of Wisconsin-Madison, August, 2002.

Comparison of Life-Cycle Emissions

Page 46: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

World Population GrowthFigure 7. World Population Growth.

Page 47: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Final Energy by Sector(IIASA Scenario B)

2000 2050 2100

Residential and Commercial 38% 31% 26%

Industry 37% 42% 51%

Transportation 25% 27% 23%

Total (TW-yr) 9.8 19.0 27.4

Page 48: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Energy Intensity(Watt-year per dollar)

(IIASA Scenario B)

Watt-year per dollar 2000

2050 2100

Industrialized 0.30 0.18 0.11Reforming 2.26 0.78 0.29Developing 1.08 0.59 0.30World 0.52 0.36 0.23

Page 49: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Some Comparative Electricity Generating Cost Projections for Year 2010 on

Nuclear Coal GasFinland 2.76 3.64 -France 2.54 3.33 3.92Germany 2.86 3.52 4.90Switzerland 2.88 - 4.36Netherlands 3.58 - 6.04Czech Republic 2.30 2.94 4.97Slovakia 3.13 4.78 5.59Romania 3.06 4.55 -Japan 4.80 4.95 5.21Korea 2.34 2.16 4.65USA 3.01 2.71 4.67Canada 2.60 3.11 4.00

US 2003 cents/kWh, Discount rate 5%, 40 year lifetime, 85% load factor.Source: OECD/IEA NEA 2005.

Page 50: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Public Health Impacts per TWh*  Coal Lignite Oil Gas Nuclear PV Wind

Years of life lost: Nonradiological effects

Radiological effects: Normal operation Accidents

138 167 359 42 9.1

160.015

58 2.7

Respiratory hospitaladmissions

0.69 0.72 1.8 0.21 0.05 0.29 0.01

Cerebrovascular hospital admissions

1.7 1.8 4.4 0.51 0.11 0.70 0.03

Congestive heart failure 0.80 0.84 2.1 0.24 0.05 0.33 0.02Restricted activity days 4751 4976 1224

81446 314 1977 90

Days with bronchodilator usage

1303 1365 3361 397 86 543 25

Cough days in asthmatics 1492 1562 3846 454 98 621 28Respiratory symptoms in

asthmatics693 726 1786 211 45 288 13

Chronic bronchitis in children 115 135 333 39 11 54 2.4Chronic cough in children 148 174 428 51 14 69 3.2Nonfatal cancer         2.4    

*Krewitt et al., “Risk Analysis” Vol. 18, No. 4 (1998).

Page 51: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Repository Requirements in the United States by the Year 2100*

NuclearFutures Legal Limit

Extended License for

Current Reactors

Continued Constant Energy

Generation

Constant MarketShare

Growing MarketShare

Total Discharged Fuel by 2100, MTHM

63,000 120,000 240,000 600,000 1,300,000

Repositories needed with current approach

1 2 4 9 21

Repository with expanded capacity

1 2 5 11

With thermal recycle only

1 2 5

With thermal and fast

1

Page 52: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

52

Page 53: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter
Page 54: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter
Page 55: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter
Page 56: Presentation for University of Chicago Physics Colloquium April 3, 2008 Burton Richter

Per Capita Electricity Sales (not including self-generation)(kWh/person) (2005 to 2008 are forecast data)

0

2,000

4,000

6,000

8,000

10,000

12,000

14,00019

60

1962

1964

1966

1968

1970

1972

1974

1976

1978

1980

1982

1984

1986

1988

1990

1992

1994

1996

1998

2000

2002

2004

2006

2008

CaliforniaUnited States

?= 4,000kWh/yr

= $400/capita