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Physics 362 – week 9 Modern Physics Seminars

Physics 362 – week 9 Modern Physics Seminars. The energy challenge

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Page 1: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Physics 362 – week 9

Modern Physics Seminars

Page 2: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

The energy challenge

Page 3: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

The energy challenge

HDI: longevity (life expectancy), educational attainment, and standard of living (gross domestic product per capita)

Page 4: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

How to produce electricity?

• Conversion of mechanical energy into electricity (dynamo)

• Conversion of chemical energy into electricity

• Conversion of nuclear energy into electricity

• Conversion of photon energy into electricity

Page 5: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Energy sources• Oil, Natural Gas, and Coal

• Nuclear

• Renewable energy source

•Solar Cells

•Water Power plants

•Windmills

•Biomass

• Hydrogen

Page 6: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Energy sources

Page 7: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Cost of energy production

Photovoltaic cells: $0.2-0.3 per kW h

Wind turbines: $0.04-0.05 per kW h

Gas: ~ $0.02 per kW h

Page 8: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Carbon reduction

Page 9: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Carbon Reduction

Page 10: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

World and U.S. reserves

Page 11: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Nuclear Energy Production

E = m c2

?

Page 12: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Chronology

1905 E=mc2 – Einstein

1939 First nuclear fission – Hahn and Strassmann

1942 First nuclear reactor – Fermi

1951 First reactor to generate electricity

Page 13: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Nuclear Forces

The nucleus is stable if the nuclear attraction dominates over the EM

repulsion

• EM repulsion between protons

• Nuclear attraction

Page 14: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Binding Energy2

np22

i c)MNmZm(MccmBE

• BE > 0

• Higher Binding energy means more stable nuclei

• <BE/A> ~ 8 MeV/nucleon

• BE/A ~ constant for A>20

Page 15: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Energy production

If BE/A initial < BE/A final

Einitial = Mjc2 = (Zjmp+Njmn)c2-BEj/Aj·Aj]

Efinal = Mic2 = (Zimp+Nimn)c2-BEi/Ai·Ai]

Efinal - Einitial = BEi/Ai·Ai - BEj/Aj·Aj > 0

Page 16: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Energy productionfissionfusion

Page 17: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Uranium Isotopes

Isotope Percent Half-life (years)238U 99.284 4.46 billions

235U 0.711 704 millions

234U 0.0055 245,000

239Pu 93/57 24,110

Page 18: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Nuclear FissionHeavy nucleus is bombarded with neutrons It decays into two smaller nuclei + neutrons

n3KrBaUn 9236

14156

23592

Page 19: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Uranium Fission

n3KrBa*UUn 9236

14156

23692

23592

Page 20: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Uranium Fission

n3KrBa*UUn 9236

14156

23692

23592

Page 21: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Chain reaction

Page 22: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Self sustained chain reactionK = Reproduction Constant

K < 1 The reactor is sub-critical it dies out

K = 1 The reactor is critical self sustained chain

K>>1 The reactor becomes unstable

Page 23: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Energy Production

K ~ 1

• Neutron leakage area/volume ratio

• Neutron Energy

• Neutron capture by non-fission elements

• Control of power level

• Safety

Page 24: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Nuclear Reactor

Page 25: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Nuclear Power Plants

Page 26: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Generation I reactors

Fuel:

235U238U/239Pu232Th/233U

OxidesCarbides

Metal alloys

n3KrBa*UUn 9236

14156

23692

23592

Page 27: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Generation I reactors

Fuel:

235U238U/239Pu232Th/233U

OxidesCarbides

Metal alloys

Coolants:

Light waterGases

Heavy waterOrganic liquidLiquid metalMolten salts

System configuration:

Pressurized waterBoiling water

Page 28: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Pressurized Water Reactor

Page 29: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Next Generation

Page 30: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Solar cells

Page 31: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Solar cells

Page 32: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Satellites

Page 33: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Solar Cells

Page 34: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Water Power plants

Page 35: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Windmills

Up to 72 m in rotor diameter

Estimated 3-22 Q of energy

Page 36: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

BiomassWood burningFermentation and distillation to produce ethanolSteam-powered generators

Page 37: Physics 362 – week 9 Modern Physics Seminars. The energy challenge

Hydrogen fuel cells

Gemini and Apollo spacecrafts

2H2+O22H2O+electricity+heat