the physics of blue lasers, solar cells, and stop lights

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The physics of blue lasers, solar cells, and stop lights Paul Kent University of Cincinnati & ORNL QuickTime™ and aTI QuickTime™ and aTIFF (Uncompressed) decompressorare needed to see this picture

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The physics of blue lasers, solar cells, and stop lights. Paul Kent. University of Cincinnati & ORNL. U.S. Department of Energy. Office of Science. Basic Energy Sciences. Division of Materials Sciences. The physics of blue lasers, solar cells, and stop lights. Paul Kent. - PowerPoint PPT Presentation

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Page 1: The physics of blue lasers,  solar cells, and stop lights

The physics of blue lasers, solar cells, and stop lights

Paul KentUniversity of Cincinnati & ORNL

QuickTime™ and aTIFF (Uncompressed) decompressorare needed to see this picture.QuickTime™ and aTIFF (Uncompressed) decompressorare needed to see this picture.

Page 2: The physics of blue lasers,  solar cells, and stop lights

The physics of blue lasers, solar cells, and stop lights

Paul KentSolid State Theory Group

National Renewable Energy Laboratory

U.S. Department of EnergyOffice of ScienceBasic Energy SciencesDivision of Materials Sciences

Thanks to: Alex Zunger & SST Group/Basic Sciences

Page 3: The physics of blue lasers,  solar cells, and stop lights

Outline

1. IntroductionNitride semiconductorsNovel phenomena. Localized states

2. How can we model these systems?Computational techniques

3. New photovoltaic materialsGaAsN (and GaPN)Band gap reduction. Localized states

4. Blue emittersInGaNLocalization at In inhomogeneities

Page 4: The physics of blue lasers,  solar cells, and stop lights

Blue laserSony 30GB DVD

High brightness LEDsTraffic signals. Solid state lighting?

High efficiency photovoltaics?

InGaNInGaN, AlGaN…

GaAsNGaAs/Ge 19% eff.

Page 5: The physics of blue lasers,  solar cells, and stop lights

Absorption in semiconductors

Conduction band

Valance band(occupied states)

Ene

rgy

Photon h

Page 6: The physics of blue lasers,  solar cells, and stop lights

High Efficiency Multijunction Solar Cells

GaAs1.4 eV

GaAs1.4 eV

GaAs1.4 eV

GaInP1.8 eV

GaInP1.8 eV

GaInP1.8 eV

Ge0.7 eV

New1.0 eV

future generationin

production

New1.0 eV

4 5 6 7 8 9

1

2 3 4

Energy (eV)

• Want 1 eV material lattice-matched to GaAs

Try GaInNAs

Calculated efficiencies (ideal)500X

AM1.5D: 36% 47% 52%one sun

AM0: 31% 38% 41%

Page 7: The physics of blue lasers,  solar cells, and stop lights

Isostructural semiconductor alloying

Properties approx. a linear combination of the components

Page 8: The physics of blue lasers,  solar cells, and stop lights

Anomaly #1: Band gap reduction in GaAsN

Band gap reduced by ~120meV per % nitrogen!

Shan et al. Phys. Rev. Lett. 82 1221 (1999)

No nitr

ogen

0.9 %

2 % Band gapsGaAs ~1.5 eVGaN ~3.5 eV

1.2 %

Page 9: The physics of blue lasers,  solar cells, and stop lights

Anomaly #2: Dilute Nitrogen in GaAs

Many sharp lines seen in emission!

Liu, Pistol and Samuelson. Appl. Phys. Lett. 56 1451 (1990) T. Makimoto et al. Appl. Phys. Lett. 70 2984 (1997)

GaAs:N

Wavelength (nm)

NN1

0 kbar

1 kbar

Page 10: The physics of blue lasers,  solar cells, and stop lights

Outline

1. IntroductionNitride semiconductorsNovel phenomena. Localized states

2. How can we model these systems?Computational techniques

3. New photovoltaic materialsGaAsN (and GaPN)Band gap reduction. Localized states

4. Blue emittersInGaNLocalization at In inhomogeneities

Page 11: The physics of blue lasers,  solar cells, and stop lights

Simplified view of a semiconductor alloy

Simulate regular latticesDistributions of atoms10^3-10^6 atoms required Atomic relaxation important

Page 12: The physics of blue lasers,  solar cells, and stop lights

Computational Modeling of Alloys

Use large supercells (10^3-10^6 atoms) containing many nitrogensStatistically average properties of many random configurationsUse Valence Force Field for structural relaxationUse Empirical Pseudopotential Method for wavefunctions

Small SupercellApproach

Large SupercellApproach

Page 13: The physics of blue lasers,  solar cells, and stop lights

Folded Spectrum Method (FSM)

valence states

conductionstates

ψψ εii

H =ˆ

1

4

23

5

N-4

N-1

N-3N-2

N

( ) ( )ψψ εεεirefirefH 22 −=−ˆ

1

4

23

5

1

4

23

5

“Fold” States

εrefBand Gap

valence states

conductionstates

Only calculate “interesting”states around band gap

Wang & Zunger J. Chem. Phys. (1994)Recently: Jacobi-Javidson Tackett PRB (2002)

1

Page 14: The physics of blue lasers,  solar cells, and stop lights

Outline

1. IntroductionNitride semiconductorsNovel phenomena. Localized states

2. How can we model these systems?Computational techniques

3. New photovoltaic materialsGaAsN (and GaPN)Band gap reduction. Localized states

4. Blue emittersInGaNLocalization at In inhomogeneities

Page 15: The physics of blue lasers,  solar cells, and stop lights

High Efficiency Multijunction Solar Cells

GaAs1.4 eV

GaAs1.4 eV

GaAs1.4 eV

GaInP1.8 eV

GaInP1.8 eV

GaInP1.8 eV

Ge0.7 eV

New1.0 eV

future generationin

production

New1.0 eV

4 5 6 7 8 9

1

2 3 4

Energy (eV)

• Want 1 eV material lattice-matched to GaAs

Try GaInNAs

Calculated efficiencies (ideal)500X

AM1.5D: 36% 47% 52%one sun

AM0: 31% 38% 41%

Page 16: The physics of blue lasers,  solar cells, and stop lights

Anomaly #1: Band gap reduction in GaAsN

Band gap reduced by ~120meV per % nitrogen!

Shan et al. Phys. Rev. Lett. 82 1221 (1999)

No nitr

ogen

0.9 %

2 % Band gapsGaAs ~1.5 eVGaN ~3.5 eV

1.2 %

Page 17: The physics of blue lasers,  solar cells, and stop lights

Anomaly #2: Dilute Nitrogen in GaAs

Many sharp lines seen in emission!

Liu, Pistol and Samuelson. Appl. Phys. Lett. 56 1451 (1990) T. Makimoto et al. Appl. Phys. Lett. 70 2984 (1997)

GaAs:N

Wavelength (nm)

NN1

0 kbar

1 kbar

Page 18: The physics of blue lasers,  solar cells, and stop lights

N in GaAs, GaP

1. Isolated Nitrogen

2. Pairs and clusters

3. Well-developed alloys

I will discuss three cases:

Page 19: The physics of blue lasers,  solar cells, and stop lights

GaP:N

Nitrogen localized a1(N)

In GaP:N (0.01%):

Level ~30 meV below CBMIntroduces character

Any concentration of nitrogen in GaP creates “direct gap” character

Page 20: The physics of blue lasers,  solar cells, and stop lights

A1 Levels of Isolated Impurity GaAs:N

44 Angstrom 44 A

ngst

rom

4096 atoms

/ L / X (%)

Nitrogen localized level ~ 150 meV inside conduction band

Localized Level in GaAs:N

Page 21: The physics of blue lasers,  solar cells, and stop lights

N in GaAs, GaP

1. Isolated Nitrogen

2. Pairs and clusters

3. Well-developed alloys

Page 22: The physics of blue lasers,  solar cells, and stop lights

N Clusters in GaAs, GaP

1. Ga(PmN4-m) Clusters

2. [1,1,0]-Oriented Nitrogen Chains

1 N 2 N 3 N 4 N

[1,1,0]

N N N N N

Page 23: The physics of blue lasers,  solar cells, and stop lights

4096 Atom Supercells

Energy levels of Ga-centred Nitrogen Clusters and (110) Chains in GaP

mNo. of Nitrogen Atoms in Cluster/Chain

1 2 3 4 5 6

Conduction Band Energy (meV)

-600

-500

-400

-300

-200

-100

0

100

CBMCBM

Ga-Centered Clusters

(110)-Oriented Chains

Energy levels of Clusters and Chains in GaP

Page 24: The physics of blue lasers,  solar cells, and stop lights

N in GaAs, GaP

1. Isolated Nitrogen

2. Pairs and clusters

3. Well-developed alloys

Page 25: The physics of blue lasers,  solar cells, and stop lights

ECBE = Delocalized Conduction Band Edge

Page 26: The physics of blue lasers,  solar cells, and stop lights
Page 27: The physics of blue lasers,  solar cells, and stop lights

GaPN

Page 28: The physics of blue lasers,  solar cells, and stop lights

GaAsN

Page 29: The physics of blue lasers,  solar cells, and stop lights

Two types of state observed

Dilute Limit: PHS in conduction band and pair/cluster CS in gap

Intermediate Range: CS do not movePHS plunge down in energy

Amalgamation Point: Lowest energy PHS just below CS

Page 30: The physics of blue lasers,  solar cells, and stop lights

Anticrossing/repulsion between band edge and

localized statesdrives band gap down

Band gap reduction

Page 31: The physics of blue lasers,  solar cells, and stop lights

GaPN Pressure dependence

–14 meV/GPa

PressureE

nerg

y

Bulk GaP

Page 32: The physics of blue lasers,  solar cells, and stop lights

Red Shift of PL vs PLE

Majority stateabsorbs

Minority stateemits

I. A. Buyanova et al. MRS IJNSR 6 2 (2001)

- Emission from localized minority states

- Absorption to majority states

Page 33: The physics of blue lasers,  solar cells, and stop lights

Summary: GaAsN & GaPN

2. Cluster states are fixed in energy

3. Host states move down, overtaking the cluster levels, one-by-one

Host states repelled from nitrogen resonant levels

4. Both localized and delocalized states existat the band edge

1. Small nitrogen aggregates create near-gap levels Some “cluster state” levels are deep, even for small aggregates

Kent & Zunger Phys. Rev. Lett. 86 2613 (2001)

Kent & Zunger Phys. Rev. B 64 5208 (2001)Kent & Zunger Appl. Phys. Lett. 79 2339( 2001)

Page 34: The physics of blue lasers,  solar cells, and stop lights

Outline

1. IntroductionNitride semiconductorsNovel phenomena. Localized states

2. How can we model these systems?Computational techniques

3. New photovoltaic materialsGaAsN (and GaPN)Band gap reduction. Localized states

4. Blue emittersInGaNLocalization at In inhomogeneities

Page 35: The physics of blue lasers,  solar cells, and stop lights

Zinc-Blende InGaN Alloys

Despite large defect density InGaN alloys emit

• Time resolved PL – many length (time) scales• Theory: Bulk InGaN alloys emit weakly

Q. What is the role of In inhomogeneity?

Why is emission so efficient?

Page 36: The physics of blue lasers,  solar cells, and stop lights

InGaN band offsets

Page 37: The physics of blue lasers,  solar cells, and stop lights

Experimental Observations

15% In

20% In

25% In

HRTEM InGaN MQW Lin et al. APL 77 2988 (2000)

Lemos et al. PRL 84 3666 (2000)

~300 meV+ lowering in emissionenergy in 33% c-InGaN samples

10nm

Page 38: The physics of blue lasers,  solar cells, and stop lights

InGaN Intrinsic Dot Calculations

Spherical dot in 141000 atom supercell

Dot: High In composition 80%+

Alloy supercell: Lower In composition 33%

ElectronsQuantum confined on dot

HolesLocalized in/near dot

(strain, alloy fluctuations)

Page 39: The physics of blue lasers,  solar cells, and stop lights

Calculations of Intrinsic Dots

Small In-rich regions give large “band gap” reduction

Page 40: The physics of blue lasers,  solar cells, and stop lights

Hole Localization in Random Alloys

Holes localize near (statistically occurring)(1,1,0)-oriented Indium chains!

1000 atom supercell20% In

Page 41: The physics of blue lasers,  solar cells, and stop lights

Indium fluctuations are key

Localized states occur near VBM, CBM

} “Quantum dot” states due to inhomogeneity

Page 42: The physics of blue lasers,  solar cells, and stop lights

Summary: InGaN

Indium fluctuations are key - localization easily results=> Can specify quality of growth required for opto devices

Kent & Zunger Appl. Phys. Lett. 79 1977 (2001)

• Small (~30 A) In-rich (80%+) regions cause low energy PL• Localized hole states exist even in random alloy

Page 43: The physics of blue lasers,  solar cells, and stop lights

Conclusion

[email protected]

1. Nitride alloys display “new physics” due to formation of localized states

2. Large-scale computational modelingcan help explain nitride properties

http://www.physics.uc.edu/~pkent

Page 44: The physics of blue lasers,  solar cells, and stop lights