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What is random matrix theory?
linear algebra
matrix properties:
- eigenvalues/vectors
- singular values/vectors
- trace, determinant, etc.
M =
⎛
⎜
⎝
2.4 1 − 0.5i · · ·
1 + 0.5i 33 · · ·
...
...
...
⎞
⎟
⎠
A. Edelman, B. D. Sutton and Y. Wang. “Modern Aspects of Random Matrix Theory”.
Proceedings of Symposia in Applied Mathematics 72, (2014)
What is random matrix theory?
linear algebra
matrix properties:
- eigenvalues/vectors
- singular values/vectors
- trace, determinant, etc.
M =
⎛
⎜
⎝
2.4 1 − 0.5i · · ·
1 + 0.5i 33 · · ·
...
...
...
⎞
⎟
⎠
A. Edelman, B. D. Sutton and Y. Wang. “Modern Aspects of Random Matrix Theory”.
Proceedings of Symposia in Applied Mathematics 72, (2014)
random matrix theory
ensemble of matrices
M =
⎛
⎜
⎝
g g · · ·
g g · · ·
...
...
...
⎞
⎟
⎠
ensemble of matrix properties
Noteb
1. The semicircle law
M =
⎛
⎜
⎝
g g · · ·
g g · · ·
...
...
...
⎞
⎟
⎠
n=500
M=randn(n, n)
M=(M+M’)/√2n
hist(eigvals(M))
E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
distribution of
eigenvalues
Notebook
histogram of level spacings
2. Level spacings: nuclear transitions
M. L. Mehta, “Random Matrices” 3/e (2004), Ch. 1energy levels
level
spacings
uncorrelated eigenvalues
“randomly” correlated
eigenvalues
distribution of eigenvalue gaps
= distribution of nuclear energy levels
0 0.5 1 1.5 2 2.5 3 3.5
0
0.2
0.4
0.6
0.8
1
1.2
bus spacing
P(s)
s
Figure1. BusintervaldistributionP(s) obtainedforcitylinenumberfour. Thefullcurverepresents
the random matrix prediction (4), the markers (+) represent the bus interval data and bars display
the random matrix prediction (4) with 0.8% of the data rejected.
2. Level spacings: bus arrival times
Nextbus.com/MBTA real-time data
12/6/2012 and 12/7/2012
Picture: transitboston.com
bus intervals in Cuernavaca, Mexico
Krbálek and Šeba, J. Phys. A 33 (2000) L229
0 0.5 1 1.5 2 2.5 3 3.5
0
0.2
0.4
0.6
0.8
1
1.2
bus spacing
P(s)
s
Figure1. BusintervaldistributionP(s) obtainedforcitylinenumberfour. Thefullcurverepresents
the random matrix prediction (4), the markers (+) represent the bus interval data and bars display
the random matrix prediction (4) with 0.8% of the data rejected.
2. Level spacings: bus arrival times
bus intervals in Cuernavaca, Mexico
Krbálek and Šeba, J. Phys. A 33 (2000) L229
mean
3. Growth & the Tracy-Widom Law
−5 −4 −3 −2 −1 0 1 2
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
0.5
K A Takeuchi and M Sano J. Stat. Phys. 147 (2012) 853
C A Tracy and H Widom, Phys. Lett. B 305 (1993) 115; Commun.
Math. Phys. 159 (1994), 151; 177 (1996), 727
experimental fluctuations of phase boundary = theoretical fluctuations in Gaussian ensembles
phase interface in a liquid crystal
statistics of fluctuations:
skewness, kurtosis
distribution of largest
eigenvalue
−2.5 −2 −1.5 −1 −0.5 0 0.5 1 1.5 2 2.5
−0.1
0
0.1
0.2
0.3
0.4
M =
⎛
⎜
⎝
g g · · ·
g g · · ·
...
...
...
⎞
⎟
⎠
largest eigenvalue of a random matrix
Physical consequences of disorder
❖ Electrical resistance in metals
thermal fluctuations

lattice defects

chemical impurities
❖ Spontaneous magnetization
ergodicity breaking

spontaneous symmetry breaking
❖ Dynamical localization
interference between paths suppresses
transport
Pictures: Wikipedia
ahmedmater.com
UPAA MIC Winners, Sep. 2011
Why is the semicircle law true?
E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325
Notebook
Wigner’s original proof:
Compute all moments of the eigenvalue distribution
Recall:
For a matrix M, the nth moment of its spectral density is the
expected trace of Mn. Denote this quantity as <Mn>.
Why is the semicircle law true?
E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325
The expected trace of Mn is actually a long sum of expectations
Why is the semicircle law true?
E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325
The expected trace of Mn is actually a long sum of expectations
Why is the semicircle law true?
E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325
The expected trace of Mn is actually a long sum of expectations
= N-1 paths of weight 1
+ 1 path of weight 1
on average
= N
Why is the semicircle law true?
E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325
The only distribution with these moments is the semicircle law
(using Carleman, 1923).
= N-1 paths of weight 1
+ 1 path of weight 1
on average
= N
Can we add eigenvalues?
In general, no. One must add eigenvalues vectorially.
eig(A) + eig(B) = eig(A+B) ?
1 + 1 = 2
vector 1
direction = eigenvector of A
magnitude = eigenvalue of A
vector 2
direction = eigenvector of B
magnitude = eigenvalue of Bvector sum
direction = eigenvector of A+B
magnitude = eigenvalue of A+B
Special cases of “matrix sums”
eigenvector of A
eigenvalue of A
eigenvector of B
eigenvalue of B
eigenvector of A+B
eigenvalue of A+B
Case 1. A and B commute.
A and B have the same basis, i.e. all their
corresponding eigenvectors are parallel.
Case 2. A and B are in general position.
The bases of A and B are randomly oriented
and have no preferred directions in common.
No deterministic analogue!
The eigenvalue distribution (density of states)
of A + B is the free convolution of the separate
densities of states.
=
A. Nica and R. Speicher, Lectures on the Combinatorics of Free Probability, 2006
JC and A Edelman, arXiv:1204.2257
Generalization to random matrices:
The eigenvalue distribution (density of states)
of A + B is the convolution of the separate
densities of states.
=*
Free convolutions
Case 2. A and B are in general position.
The bases of A and B are randomly oriented
and have no preferred directions in common.
The eigenvalue distribution (density of states)
of A + B is the free convolution of the separate
densities of states.
=
D. Voiculescu, Inventiones Mathematicae, 1991, 201-220.
function eigvals_free(A, B)
n = size(A, 1)
Q = qr(randn(n, n))
M = A + Q*B*Q’
eigvals(M)
end
The spectral density of M can be
given by free probability theory
Noisy electronic structure
Tight binding Anderson Hamiltonian in 1D
constant coupling
Gaussian disorder
interaction
J
+
random fluctuation of site energies
Avoiding diagonalization
In general, exact diagonalization is expensive.
Strategy: split H into pieces with known eigenvalues
then recombine using free convolution. How accurate is it?
−4 −3 −2 −1 0 1 2 3 4
0
0.05
0.1
0.15
0.2
0.25
0.3
0.35
0.4
0.45
Results of free convolution
Approximation
Exact
high noise moderate noise low noise
JC et al. Phys. Rev. Lett. 109 (2012),
036403
-10
0
10 0.1
1
10
0
0.1
0.2
ρ(x)
x
σ/J
ρ(x)
-10
0
10 0.1
1
10
0
0.1
0.2
ρ(x)
x
σ/J
ρ(x)
2D square 2D honeycomb
-10
0
10 0.1
1
10
0
0.1
0.2
ρ(x)
x
σ/J
ρ(x)
3D cube
-10
0
10 0.1
1
10
0
0.1
0.2
0.3
ρ(x)
x
σ/J
ρ(x)
1D next-nearest neighbors
-10
0
10 0.1
1
10
0
0.1
0.2
ρ(x)
x
σ*/σ
ρ(x)
1D NN with fluctuating interactions
exact
approx.
Spectral signature of localization
Spectral compressibility
0 for Wigner statistics (maximally delocalized states)
1 for Poisson statistics (localized states)
measures fine-scale fluctuations in the level density
Can tell something about eigenvectors from the eigenvalues?!
B. L. Altshuler, I. K. Zharekeshev, S. A. Kotochigova, and B. I. Shklovskii, Sov. Phys. JETP 67 (1988) 625.
Relationships between c and localization length of eigenvectors are
conjectured to hold for certain random matrix ensembles
χ(E) = lim
⟨N(E)⟩→∞
d ∆N2
(E)
d ⟨N(E)⟩
∼
∆N2
(E)
⟨N(E)⟩
Excitation energy (eV)
RMSlength(normalized)
1.6 1.8 2 2.2 2.4
0.2
0.4
0.6
0.8
Can tell something about eigenvectors from the eigenvalues?!
Spectral signature of localization
spectral compressibility
Strategy 1. Model Hamiltonians
atomic coordinates electronic structure
dynamics
observable
disordered system
ensemble-averaged
observable
sampling in
phase space
...
ensemble of
model
Hamiltonians
Outline
❖ Introduction: organic solar cells
Bulk heterojunctions

Disorder matters!

Computing
❖ Disordered excitons ab initio
The sampling challenge

Exciton band structures
❖ Models for disordered excitons
Random matrix theory

Quantum mechanics without wavefunctions
±
+
Excitation energy (eV)
Localizationlength(normalized)
1.4 1.6 1.8 2 2.2 2.4
0
0.2
0.4
0.6
0.8
A standard protocol of
computational chemistry
crystal atomic coordinates
electronic structure
dynamics
observable
A standard protocol of
computational chemistry
crystal atomic coordinates
electronic structure
dynamics
observable
?X
disordered system
disordered system
observable
?
Modeling disorder: explicit sampling
Modeling disorder: explicit sampling
disordered system
observable
sampling in
phase space
...
atomic coordinates electronic structure
dynamics
observable
ensemble averaging
Q-Chem input
generation
Infrastructure for large-scale
quantum chemical simulations
HDF5
Database
Q-Chem output file parsing
Q-Chem
QM/MM
Grid
Engine
CHARMM
error handling
convergence failures
system failures
...
job dispatcher
queue monitor
error handling for
cluster-wide failures
post-analysis
scripts
sampling electronic structure observables
thermalizedperfect crystal
Step 1. Sample thermalized states using molecular dynamics
NVT dynamics of 8x8x8 supercell in CHARMM
Cost: ~4 CPU-hours
Step 2. Calculate absorption frequencies (energies) of each
molecule using ab initio electronic structure theory
TD-PBE0/6-31G* with electrostatic embedding in Q-Chem + 0.2 eV shift
*L Edwards and M. Gouterman, J. Mol. Spect. 33 (1970), 292
Qx
Qy
B
Step 3. Collect statistics to recover averaged spectra
100 snapshots x 128 molecules, ~6 CPU-years
Absorption spectrum (gas)
1.2 1.4 1.6 1.8 2 2.2
(condensed)
Energy (eV)
Qx
Qy
Qx Qy
tail states?
• Normalized root mean square spread

of the exciton wavefunction
• Localization determines nature of transport
Localization of states
1
N 1
l =
1
Lmax
ψ |r|
2
ψ − ⟨ψ |r| ψ⟩
2
incoherent
diffusive
coherent
ballistic
Localization of states
Excitation energy (eV)
RMSlength(normalized)
1.6 1.8 2 2.2 2.4
0.2
0.4
0.6
0.8
Localization of states
Excitation energy (eV)
RMSlength(normalized)
1.6 1.8 2 2.2 2.4
0.2
0.4
0.6
0.8
delocalized
Localization of states
Excitation energy (eV)
RMSlength(normalized)
1.6 1.8 2 2.2 2.4
0.2
0.4
0.6
0.8
0 50 100 20
40
60
60
80
100
120
140
160
180
sample 61, state 5, energy = 2.126573
- delocalized along
herringbone axis only
- antiferromagnetic order
in transition dipoles
Localization of states
Excitation energy (eV)
RMSlength(normalized)
1.6 1.8 2 2.2 2.4
0.2
0.4
0.6
0.8
- mostly delocalized along
herringbone axis
- polaron-like
- antiferromagnetic order
in transition dipoles
Localization of states
Excitation energy (eV)
RMSlength(normalized)
1.6 1.8 2 2.2 2.4
0.2
0.4
0.6
0.8
0
50
100
20
40
60
60
80
100
120
140
160
180
sample 1, state 51, energy = 1.715239
- mostly delocalized along
herringbone axis
- polaron-like
- ferromagnetic order
in transition dipoles
Excitation energy (eV)
RMSlength(normalized)
1.6 1.8 2 2.2 2.4
0.2
0.4
0.6
0.8
Asymmetry from neighbor shells
Excitation energy (eV)
RMSlength(normalized)
1.6 1.8 2 2.2 2.4
0.2
0.4
0.6
0.8
1 2 all
number of
neighbor
shells
Neighbor shells in crystal
Excitation energy (eV)
RMSlength(normalized)
1.7 1.75 1.8 1.85 1.9
0.6
0.7
0.8
0.9
1
Excitation energy (eV)
RMSlength(normalized)
1.5 1.6 1.7 1.8 1.9 2
0.8
0.85
0.9
0.95
1
Excitation energy (eV)
RMSlength(normalized)
1.5 1.6 1.7 1.8 1.9 2
0.85
0.9
0.95
1
Excitation energy (eV)
RMSlength(normalized)
1.4 1.6 1.8
0.7
0.75
0.8
0.85
0.9
0.95
1
1 2 3 all
number of
neighbor
shells
Summary
Excitons in H2Pc come in
three distinct flavors
high energy:

localized in 2D, delocalized
along herringbone axis
• medium energy:

delocalized
• low energy:

dressed states localized
predominantly in 2D
Asymmetric density of states
is a nonlocal effect
J.C. et al., Phys. Rev. Lett. 2012
Excitation energy (eV)
Localizationlength(normalized)
1.4 1.6 1.8 2 2.2 2.4
0
0.2
0.4
0.6
0.8
Modeling disorder
disordered system
observable
sampling in
phase space
...
atomic coordinates electronic structure
dynamics
observable
ensemble averaging
Modeling disorder
disordered system
observable
sampling in
phase space
...
atomic coordinates electronic structure
dynamics
observable
ensemble averaging
4 CPU-hours
Absorption spectrum (gas)
1.2 1.4 1.6 1.8 2 2.2
(condensed)
Energy (eV)
6 CPU-years
1 “CPU-PhD”
Modeling disorder
atomic coordinates electronic structure
dynamics
observable
disordered system
ensemble-averaged
observable
sampling in
phase space
random matrix theory?
...
spatial disorder
spectral disorder
Summary
•Free probability allows us to construct accurate
approximations to analytic model Hamiltonians
•An error analysis of this phenomenon is known
•Statistics of eigenvalues may be able to tell us
information about experimental observations
J.C. et al., Phys. Rev. Lett. 2012

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Free probability, random matrices and disorder in organic semiconductors

  • 1. What is random matrix theory? linear algebra matrix properties: - eigenvalues/vectors - singular values/vectors - trace, determinant, etc. M = ⎛ ⎜ ⎝ 2.4 1 − 0.5i · · · 1 + 0.5i 33 · · · ... ... ... ⎞ ⎟ ⎠ A. Edelman, B. D. Sutton and Y. Wang. “Modern Aspects of Random Matrix Theory”. Proceedings of Symposia in Applied Mathematics 72, (2014)
  • 2. What is random matrix theory? linear algebra matrix properties: - eigenvalues/vectors - singular values/vectors - trace, determinant, etc. M = ⎛ ⎜ ⎝ 2.4 1 − 0.5i · · · 1 + 0.5i 33 · · · ... ... ... ⎞ ⎟ ⎠ A. Edelman, B. D. Sutton and Y. Wang. “Modern Aspects of Random Matrix Theory”. Proceedings of Symposia in Applied Mathematics 72, (2014) random matrix theory ensemble of matrices M = ⎛ ⎜ ⎝ g g · · · g g · · · ... ... ... ⎞ ⎟ ⎠ ensemble of matrix properties Noteb
  • 3. 1. The semicircle law M = ⎛ ⎜ ⎝ g g · · · g g · · · ... ... ... ⎞ ⎟ ⎠ n=500 M=randn(n, n) M=(M+M’)/√2n hist(eigvals(M)) E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 distribution of eigenvalues Notebook
  • 4. histogram of level spacings 2. Level spacings: nuclear transitions M. L. Mehta, “Random Matrices” 3/e (2004), Ch. 1energy levels level spacings uncorrelated eigenvalues “randomly” correlated eigenvalues distribution of eigenvalue gaps = distribution of nuclear energy levels
  • 5. 0 0.5 1 1.5 2 2.5 3 3.5 0 0.2 0.4 0.6 0.8 1 1.2 bus spacing P(s) s Figure1. BusintervaldistributionP(s) obtainedforcitylinenumberfour. Thefullcurverepresents the random matrix prediction (4), the markers (+) represent the bus interval data and bars display the random matrix prediction (4) with 0.8% of the data rejected. 2. Level spacings: bus arrival times Nextbus.com/MBTA real-time data 12/6/2012 and 12/7/2012 Picture: transitboston.com bus intervals in Cuernavaca, Mexico Krbálek and Šeba, J. Phys. A 33 (2000) L229
  • 6. 0 0.5 1 1.5 2 2.5 3 3.5 0 0.2 0.4 0.6 0.8 1 1.2 bus spacing P(s) s Figure1. BusintervaldistributionP(s) obtainedforcitylinenumberfour. Thefullcurverepresents the random matrix prediction (4), the markers (+) represent the bus interval data and bars display the random matrix prediction (4) with 0.8% of the data rejected. 2. Level spacings: bus arrival times bus intervals in Cuernavaca, Mexico Krbálek and Šeba, J. Phys. A 33 (2000) L229 mean
  • 7. 3. Growth & the Tracy-Widom Law −5 −4 −3 −2 −1 0 1 2 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5 K A Takeuchi and M Sano J. Stat. Phys. 147 (2012) 853 C A Tracy and H Widom, Phys. Lett. B 305 (1993) 115; Commun. Math. Phys. 159 (1994), 151; 177 (1996), 727 experimental fluctuations of phase boundary = theoretical fluctuations in Gaussian ensembles phase interface in a liquid crystal statistics of fluctuations: skewness, kurtosis distribution of largest eigenvalue −2.5 −2 −1.5 −1 −0.5 0 0.5 1 1.5 2 2.5 −0.1 0 0.1 0.2 0.3 0.4 M = ⎛ ⎜ ⎝ g g · · · g g · · · ... ... ... ⎞ ⎟ ⎠ largest eigenvalue of a random matrix
  • 8. Physical consequences of disorder ❖ Electrical resistance in metals thermal fluctuations
 lattice defects
 chemical impurities ❖ Spontaneous magnetization ergodicity breaking
 spontaneous symmetry breaking ❖ Dynamical localization interference between paths suppresses transport Pictures: Wikipedia ahmedmater.com UPAA MIC Winners, Sep. 2011
  • 9. Why is the semicircle law true? E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325 Notebook Wigner’s original proof: Compute all moments of the eigenvalue distribution Recall: For a matrix M, the nth moment of its spectral density is the expected trace of Mn. Denote this quantity as <Mn>.
  • 10. Why is the semicircle law true? E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325 The expected trace of Mn is actually a long sum of expectations
  • 11. Why is the semicircle law true? E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325 The expected trace of Mn is actually a long sum of expectations
  • 12. Why is the semicircle law true? E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325 The expected trace of Mn is actually a long sum of expectations = N-1 paths of weight 1 + 1 path of weight 1 on average = N
  • 13. Why is the semicircle law true? E P Wigner, Ann. Math. 62 (1955), 548; 67 (1958), 325 The only distribution with these moments is the semicircle law (using Carleman, 1923). = N-1 paths of weight 1 + 1 path of weight 1 on average = N
  • 14. Can we add eigenvalues? In general, no. One must add eigenvalues vectorially. eig(A) + eig(B) = eig(A+B) ? 1 + 1 = 2 vector 1 direction = eigenvector of A magnitude = eigenvalue of A vector 2 direction = eigenvector of B magnitude = eigenvalue of Bvector sum direction = eigenvector of A+B magnitude = eigenvalue of A+B
  • 15. Special cases of “matrix sums” eigenvector of A eigenvalue of A eigenvector of B eigenvalue of B eigenvector of A+B eigenvalue of A+B Case 1. A and B commute. A and B have the same basis, i.e. all their corresponding eigenvectors are parallel. Case 2. A and B are in general position. The bases of A and B are randomly oriented and have no preferred directions in common. No deterministic analogue! The eigenvalue distribution (density of states) of A + B is the free convolution of the separate densities of states. = A. Nica and R. Speicher, Lectures on the Combinatorics of Free Probability, 2006 JC and A Edelman, arXiv:1204.2257 Generalization to random matrices: The eigenvalue distribution (density of states) of A + B is the convolution of the separate densities of states. =*
  • 16. Free convolutions Case 2. A and B are in general position. The bases of A and B are randomly oriented and have no preferred directions in common. The eigenvalue distribution (density of states) of A + B is the free convolution of the separate densities of states. = D. Voiculescu, Inventiones Mathematicae, 1991, 201-220. function eigvals_free(A, B) n = size(A, 1) Q = qr(randn(n, n)) M = A + Q*B*Q’ eigvals(M) end The spectral density of M can be given by free probability theory
  • 17. Noisy electronic structure Tight binding Anderson Hamiltonian in 1D constant coupling Gaussian disorder interaction J + random fluctuation of site energies
  • 18. Avoiding diagonalization In general, exact diagonalization is expensive. Strategy: split H into pieces with known eigenvalues then recombine using free convolution. How accurate is it? −4 −3 −2 −1 0 1 2 3 4 0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45
  • 19. Results of free convolution Approximation Exact high noise moderate noise low noise JC et al. Phys. Rev. Lett. 109 (2012), 036403
  • 20. -10 0 10 0.1 1 10 0 0.1 0.2 ρ(x) x σ/J ρ(x) -10 0 10 0.1 1 10 0 0.1 0.2 ρ(x) x σ/J ρ(x) 2D square 2D honeycomb -10 0 10 0.1 1 10 0 0.1 0.2 ρ(x) x σ/J ρ(x) 3D cube -10 0 10 0.1 1 10 0 0.1 0.2 0.3 ρ(x) x σ/J ρ(x) 1D next-nearest neighbors -10 0 10 0.1 1 10 0 0.1 0.2 ρ(x) x σ*/σ ρ(x) 1D NN with fluctuating interactions exact approx.
  • 21. Spectral signature of localization Spectral compressibility 0 for Wigner statistics (maximally delocalized states) 1 for Poisson statistics (localized states) measures fine-scale fluctuations in the level density Can tell something about eigenvectors from the eigenvalues?! B. L. Altshuler, I. K. Zharekeshev, S. A. Kotochigova, and B. I. Shklovskii, Sov. Phys. JETP 67 (1988) 625. Relationships between c and localization length of eigenvectors are conjectured to hold for certain random matrix ensembles χ(E) = lim ⟨N(E)⟩→∞ d ∆N2 (E) d ⟨N(E)⟩ ∼ ∆N2 (E) ⟨N(E)⟩
  • 22. Excitation energy (eV) RMSlength(normalized) 1.6 1.8 2 2.2 2.4 0.2 0.4 0.6 0.8 Can tell something about eigenvectors from the eigenvalues?! Spectral signature of localization spectral compressibility
  • 23.
  • 24. Strategy 1. Model Hamiltonians atomic coordinates electronic structure dynamics observable disordered system ensemble-averaged observable sampling in phase space ... ensemble of model Hamiltonians
  • 25. Outline ❖ Introduction: organic solar cells Bulk heterojunctions
 Disorder matters!
 Computing ❖ Disordered excitons ab initio The sampling challenge
 Exciton band structures ❖ Models for disordered excitons Random matrix theory
 Quantum mechanics without wavefunctions ± + Excitation energy (eV) Localizationlength(normalized) 1.4 1.6 1.8 2 2.2 2.4 0 0.2 0.4 0.6 0.8
  • 26. A standard protocol of computational chemistry crystal atomic coordinates electronic structure dynamics observable
  • 27. A standard protocol of computational chemistry crystal atomic coordinates electronic structure dynamics observable ?X disordered system
  • 29. Modeling disorder: explicit sampling disordered system observable sampling in phase space ... atomic coordinates electronic structure dynamics observable ensemble averaging
  • 30. Q-Chem input generation Infrastructure for large-scale quantum chemical simulations HDF5 Database Q-Chem output file parsing Q-Chem QM/MM Grid Engine CHARMM error handling convergence failures system failures ... job dispatcher queue monitor error handling for cluster-wide failures post-analysis scripts sampling electronic structure observables
  • 31. thermalizedperfect crystal Step 1. Sample thermalized states using molecular dynamics NVT dynamics of 8x8x8 supercell in CHARMM
  • 32.
  • 33. Cost: ~4 CPU-hours Step 2. Calculate absorption frequencies (energies) of each molecule using ab initio electronic structure theory TD-PBE0/6-31G* with electrostatic embedding in Q-Chem + 0.2 eV shift *L Edwards and M. Gouterman, J. Mol. Spect. 33 (1970), 292 Qx Qy B
  • 34. Step 3. Collect statistics to recover averaged spectra 100 snapshots x 128 molecules, ~6 CPU-years Absorption spectrum (gas) 1.2 1.4 1.6 1.8 2 2.2 (condensed) Energy (eV) Qx Qy Qx Qy tail states?
  • 35. • Normalized root mean square spread
 of the exciton wavefunction • Localization determines nature of transport Localization of states 1 N 1 l = 1 Lmax ψ |r| 2 ψ − ⟨ψ |r| ψ⟩ 2 incoherent diffusive coherent ballistic
  • 36. Localization of states Excitation energy (eV) RMSlength(normalized) 1.6 1.8 2 2.2 2.4 0.2 0.4 0.6 0.8
  • 37. Localization of states Excitation energy (eV) RMSlength(normalized) 1.6 1.8 2 2.2 2.4 0.2 0.4 0.6 0.8 delocalized
  • 38. Localization of states Excitation energy (eV) RMSlength(normalized) 1.6 1.8 2 2.2 2.4 0.2 0.4 0.6 0.8 0 50 100 20 40 60 60 80 100 120 140 160 180 sample 61, state 5, energy = 2.126573 - delocalized along herringbone axis only - antiferromagnetic order in transition dipoles
  • 39. Localization of states Excitation energy (eV) RMSlength(normalized) 1.6 1.8 2 2.2 2.4 0.2 0.4 0.6 0.8 - mostly delocalized along herringbone axis - polaron-like - antiferromagnetic order in transition dipoles
  • 40. Localization of states Excitation energy (eV) RMSlength(normalized) 1.6 1.8 2 2.2 2.4 0.2 0.4 0.6 0.8 0 50 100 20 40 60 60 80 100 120 140 160 180 sample 1, state 51, energy = 1.715239 - mostly delocalized along herringbone axis - polaron-like - ferromagnetic order in transition dipoles
  • 41. Excitation energy (eV) RMSlength(normalized) 1.6 1.8 2 2.2 2.4 0.2 0.4 0.6 0.8 Asymmetry from neighbor shells Excitation energy (eV) RMSlength(normalized) 1.6 1.8 2 2.2 2.4 0.2 0.4 0.6 0.8 1 2 all number of neighbor shells
  • 42. Neighbor shells in crystal Excitation energy (eV) RMSlength(normalized) 1.7 1.75 1.8 1.85 1.9 0.6 0.7 0.8 0.9 1 Excitation energy (eV) RMSlength(normalized) 1.5 1.6 1.7 1.8 1.9 2 0.8 0.85 0.9 0.95 1 Excitation energy (eV) RMSlength(normalized) 1.5 1.6 1.7 1.8 1.9 2 0.85 0.9 0.95 1 Excitation energy (eV) RMSlength(normalized) 1.4 1.6 1.8 0.7 0.75 0.8 0.85 0.9 0.95 1 1 2 3 all number of neighbor shells
  • 43. Summary Excitons in H2Pc come in three distinct flavors high energy:
 localized in 2D, delocalized along herringbone axis • medium energy:
 delocalized • low energy:
 dressed states localized predominantly in 2D Asymmetric density of states is a nonlocal effect J.C. et al., Phys. Rev. Lett. 2012 Excitation energy (eV) Localizationlength(normalized) 1.4 1.6 1.8 2 2.2 2.4 0 0.2 0.4 0.6 0.8
  • 44. Modeling disorder disordered system observable sampling in phase space ... atomic coordinates electronic structure dynamics observable ensemble averaging
  • 45. Modeling disorder disordered system observable sampling in phase space ... atomic coordinates electronic structure dynamics observable ensemble averaging 4 CPU-hours Absorption spectrum (gas) 1.2 1.4 1.6 1.8 2 2.2 (condensed) Energy (eV) 6 CPU-years 1 “CPU-PhD”
  • 46. Modeling disorder atomic coordinates electronic structure dynamics observable disordered system ensemble-averaged observable sampling in phase space random matrix theory? ... spatial disorder spectral disorder
  • 47. Summary •Free probability allows us to construct accurate approximations to analytic model Hamiltonians •An error analysis of this phenomenon is known •Statistics of eigenvalues may be able to tell us information about experimental observations J.C. et al., Phys. Rev. Lett. 2012