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yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

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Page 1: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

yale university

Photovoltaic Properties of a Revolutionary New Solar Cell

Drew Mazurek Advisor: Jerry Woodall

April 30, 2002

Page 2: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells in real life

• Cost-effective way to provide power to remote areas

Page 3: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells in real life

• Cost-effective way to provide power to remote areas

• Environmentally-friendly renewable energy source

Page 4: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells in real life

• Cost-effective way to provide power to remote areas

• Environmentally-friendly renewable energy source

• Power source for outer space applications

Page 5: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

how solar cells work

The simple idea: photons in, current and voltage out

Page 6: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

how solar cells work

A closer look: photons above the semiconductor’s band gap energy generate hole/electron pairs…

pn-junction

p

n

- holes

- electrons

h > Eg

Page 7: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

how solar cells work

which then diffuse across the cell’s concentration gradients

pn-junction

p

n

- holes

- electrons

Page 8: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

how solar cells work

Some holes and electrons recombine before they can reach the other side of the junction. In good cells,

however, there is very little recombination.

pn-junction

p

n

- holes

- electrons

Page 9: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

how solar cells work

Most holes and electrons make it to the other side, resulting in a net charge increase on each side. This net charge increase is

realized outside the cell as current and voltage, or power.

pn-junction

p

n

- holes

- electrons

Page 10: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells in space

To go into space, solar cells must be

• efficient – want to produce as much power as possible

• lightweight – launching satellites into space costs $5,000 per pound

Additionally, we’d like them to be

• inexpensive to manufacture – $$$

• radiation-hard – Van Allen Belt ideal place for satellites, but high radiation environment

Page 11: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

Strong electric field (~1,000-10,000 V/cm)

n++ n p

Indium Phosphide drift-based design

surface

Page 12: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

n++ n p

h > Eg

Indium Phosphide drift-based design

Strong electric field (~1,000-10,000 V/cm)

surface

Page 13: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

Strong electric field (~1,000-10,000 V/cm)

solar cells at yale

n++ n p

Indium Phosphide drift-based design

surface

Page 14: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

• motion of carriers due to electric field

• not as susceptible to material defects

• motion of carriers due to concentration gradient

• material defects shorten carrier lifetime, causing more recombination

Diffusion (theirs)

Drift (ours)

vs.

Page 15: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

Strong electric field… so what?

• holes are immediately swept into the junction, producing power

• fewer hole/electron pairs are lost due to recombination – no time to recombine!

n++ n p

Page 16: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

Strong electric field… so what?

• radiation damage decreases carrier lifetimes. Carriers swept by drift (electric) fields, however, aren’t affected as much.

n++ n p

Page 17: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

Why Indium Phosphide?

• very high ideal efficiency: ~37% at concentration of 1,000 suns

Page 18: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

Why Indium Phosphide?

• very high ideal efficiency: ~37% at concentration of 1,000 suns

• absorbs most light at small thicknesses – lightweight! 0

20

40

60

80

100

0.01 0.1 1 10 100 1000

Thickness (μm)

Abs

orbe

d P

ower

(%)

Si GaAs InP

Page 19: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

Why Indium Phosphide?

• very high quantum efficiency across all wavelengths of visible light and UV – highly efficient and it makes good use of almost the entire spectrum 0%

10%

20%

30%

40%

50%

60%

70%

80%

90%

100%

100 200 300 400 500 600 700 800 900 1000

Wavelength (nm)

Inte

rnal

Qua

ntum

Eff

icie

ncy

1 µm InP (10 Å dead region)1 µm GaAs (100 Å dead region)1 µm Si (10 Å dead region)10 µm Si (5 Å dead region)

Page 20: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

solar cells at yale

Yale’s InP solar cells are ideal for outer space applications:

• lightweight

• radiation-hard

• highly efficient

• low cost (~$1/cm2 vs. $10/cm2 for current high-efficiency solar cells)

Page 21: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

summary

• Solar cells are simply pn-junctions in which hole/electron pairs are created from photons.

• The holes/electrons diffuse into the junction, and are immediately swept to the other side.

• The net charge gain is seen outside the cell as current and voltage, or power.

Page 22: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

summary

• At Yale, we have designed and perfected the first ever drift-dominated solar cell.

• By collecting carriers with an electric field, we are able to create solar cells that are robust in the strong radiation of outer space.

• Additionally, our cells are lightweight and inexpensive.

Page 23: Yale university Photovoltaic Properties of a Revolutionary New Solar Cell Drew Mazurek Advisor: Jerry Woodall April 30, 2002

acknowledgements

Many thanks to:

Professor Jerry Woodall

Professor Janet Pan

Yanning Sun