Presentation is loading. Please wait.

Presentation is loading. Please wait.

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

Similar presentations


Presentation on theme: "Physics 362 – week 9 Modern Physics Seminars. The energy challenge."— Presentation transcript:

1 Physics 362 – week 9 Modern Physics Seminars

2 The energy challenge

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

4 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

5 Energy sources Oil, Natural Gas, and Coal Nuclear Renewable energy source Solar Cells Water Power plants Windmills Biomass Hydrogen

6 Energy sources

7 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

8 Carbon reduction

9 Carbon Reduction

10 World and U.S. reserves

11 Nuclear Energy Production E = m c 2 ?

12 Chronology 1905 E=mc 2 – Einstein 1939 First nuclear fission – Hahn and Strassmann 1942 First nuclear reactor – Fermi 1951 First reactor to generate electricity

13 Nuclear Forces  The nucleus is stable if the nuclear attraction dominates over the EM repulsion EM repulsion between protons Nuclear attraction

14 Binding Energy BE > 0 Higher Binding energy means more stable nuclei ~ 8 MeV/nucleon BE/A ~ constant for A>20

15 Energy production If BE/A initial < BE/A final  E initial =  M j c 2 =  (Z j m p +N j m n )c 2 -BE j /A j ·A j ] E final =  M i c 2 =  (Z i m p +N i m n )c 2 -BE i /A i ·A i ]  E final - E initial =  BE i /A i ·A i -  BE j /A j ·A j > 0

16 Energy production fissionfusion

17 Uranium Isotopes IsotopePercentHalf-life (years) 238 U99.2844.46 billions 235 U0.711704 millions 234 U0.0055245,000 239 Pu93/5724,110

18 Nuclear Fission Heavy nucleus is bombarded with neutrons  It decays into two smaller nuclei + neutrons

19 Uranium Fission

20

21 Chain reaction

22 Self sustained chain reaction K = 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

23 Energy Production K ~ 1 Neutron leakage  area/volume ratio Neutron Energy Neutron capture by non-fission elements Control of power level Safety

24 Nuclear Reactor

25 Nuclear Power Plants

26 Generation I reactors Fuel: 235 U 238 U/ 239 Pu 232 Th/ 233 U Oxides Carbides Metal alloys

27 Generation I reactors Fuel: 235 U 238 U/ 239 Pu 232 Th/ 233 U Oxides Carbides Metal alloys Coolants: Light water Gases Heavy water Organic liquid Liquid metal Molten salts System configuration: Pressurized water Boiling water

28 Pressurized Water Reactor

29 Next Generation

30 Solar cells

31

32 Satellites

33 Solar Cells

34 Water Power plants

35 Windmills Up to 72 m in rotor diameter Estimated 3-22 Q of energy

36 Biomass Wood burning Fermentation and distillation to produce ethanol Steam-powered generators

37 Hydrogen fuel cells Gemini and Apollo spacecrafts 2H 2 +O 2  2H 2 O+electricity+heat


Download ppt "Physics 362 – week 9 Modern Physics Seminars. The energy challenge."

Similar presentations


Ads by Google