coursera 07 - future energy needs and consequences from a physical
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Future Energy Needs and Consequences From a Physical
Sciences Perspective
The sun is the largest exploitable resource:
1 hour of sun to earth = all of mankind’s yearly energy:
Basic Science: How to capture and store?
Photosynthesis
Artificial photosyntesis
Uses of Solar Fuels
Hydrogen and carbon-based feedstocks are widely used in industry.
Fertilizers
Pharmaceuticals
Plastics
Synthetic fuels
Challenges in large-scale productionof solar fuels
Efficient, so that they harness as much of the sunlight hitting them as possible to produce fuels.
Durable, so that they can convert a lot of energy in their lifetime relative to the energy required to install them.
Cost effective, so that solar fuels are commercially viable.
All working together
Integrating the different processes and materials involved, from capturing and channeling sunlight through to producing a chemical fuel;
Identifying inexpensive catalysts to drive different aspects of the process
Developing ways to avoid the system degrading quickly because of exposure to sunlight.
Supercondutivity
TemperatureR
esi
stiv
ity Kelvin (1902)
Matthiessen (1864)
Dewar (1904)
H. Kamerlingh Onnes
“Mercury has passed into a new state, which on account of its extraordinary electrical properties may be called the superconducting state”
1911: Liquid Helium (B.P.: 4.2K)
1911: Observed that electrical resistance R(T)
of mercury vanished below Tc=4.2K
Tc Superconducting critical
temperature
1913: Nobel Prize in Physics
Discovery of Superconductivity
Origin of superconductivity
Metal:
• Periodic arrangement (lattice) of positively charged ions “Gas” of mobile negatively charged changed conduction electrons.
Normal State: Scattering of electrons by:
• Thermal motion of ions
• Impurities
• Other electrons
Superconducting state:
• Electrons with opposite momentum P and spin S are paired (P ,-P )
• Electron pairs move in concert through lattice
e-
e-
Phonon
Cooper pair model
Superconducting materials: Maximum Value of Tc versus time
1920 1940 1960 1980 20000
20
40
60
80
100
120
140
Cs2RbC
60
MgB2
LHe
Liquid nitrogen
HgBa2Ca
2Cu
3O8
Tl2Sr2Ca
2Cu
3O10
Bi2Sr2Ca
2Cu
3O10
YBa2Cu
3O7
La2-xSrxCuO
4
Ba1-xKxBiO
3
BaPb1-xBixO3
NaxWO
3NbO
Nb3Ge
Nb3SnNbN
NbPbHg
TC [
K]
Year
A superconductor is a perfect diamagnet. Superconducting material expels magnetic flux from the interior.
Superconducting Aplications
The grand challenge with superconductors
Superconductor state only happens at very low temperature
The mechanism for the materials are not well-known yet
Non-superconductor Nano-vortices within superconductors (quantum vortex)
Energy considerations
IPhone uses more energy than your refrigerator
More E to stream a video than to manufacture and ship a CD
10% of E consumption is on wireless
Waste is unavoidable
No foreseeable ceiling for use of E for devices
The Problem With the Actual Technology
The actual technology already has problems with its compounds that do lose energy in its operation.
Magnetoresistence
Electrical heating
Mechanical deformations by heating
New technologies
Plasma
Optical fiber (uses photons/computers uses electrons)
Excitons
Homemade Sun
The Tokamak Reactor
Is based in the principle of magnetic confined
Inside of it we have temperatures of about 150 million of Celsius degrees Forming a hot plasma
Has superconducting coils surrounded the tokamak
The issue here is how we can confine it
The conclusion
We actually have a big amount of technologies that would be a solution for our energy necessities, but actually need more research in this fields.
Talking about synthetic photosynthesis we need more research and start to use prototypes than allows improve this technology.
About superconductors we need to understand in a better way the physics of these things.
The nanomaterial actually are very used maybe we thing another ways for use this materials for avoid our energy wastes.