Roi Baer - Home | Institute for Mathematics and its … 1.6 1.5 1.34 1.8 1.41 1.38 Ne 3.1 2.9 2.4...
Transcript of Roi Baer - Home | Institute for Mathematics and its … 1.6 1.5 1.34 1.8 1.41 1.38 Ne 3.1 2.9 2.4...
Roi BaerInstitute of Chemistry,
The Fritz Haber Center for Molecular Dynamics
The Hebrew University of Jerusalem,
Jerusalem, Israel
• Ms. Ester Livshits (PhD student, Jerusalem)• Dr. Helen Eisenberg (Postdoc, Jerusalem)• Tamar Gershon (PhD student Jerusalem)Collaborators • Tamar Gershon (PhD student, Jerusalem)• Professor Leeor Kronik (Weizmann)• Professor Daniel Neuhauser (UCLA)• Professor Anna Krylov (USC)
Collaborators and Students
• Professor Anna Krylov (USC)
• Israel Science Foundation (ISF)• US-Israel Binational Science Foundation
(BSF)Funding (BSF)• FAME network of excellence
Funding
• An electron is repelled not only by other electrons, but also by itselfSelf
• Good at the short range (emulates correlation)
• But much too much at long range
Self repulsion
• Static polarizability• Stability of anions• Charge quantization in decoupled systems
Unphysical b h i
g q p y• Charge transfer excitations• Rydberg excitations
behavior
1 1 2 2Take a charge at and bring another charge from infinity to . q qr r
1 22 12 1 2
12
The energy for this i .s: q q
E rr
= = −r r
1 3 2 3Next bring another charge from infinity to :q q q q
q E = +r3 3 313 23
Next, bring another charge from infinity to :q Er r
= +r
1The total energy is a sum over pairs:
2i j
i j ij
q qE
r≠
= ∑2 i j ijr≠
( ) ( )( )3 31
For continuous charge dist: ( density of charge)2
n nE d rd r n
′′=
′−∫r r
rr r
But this includes self interaction - analogous to the termsi j=
( ) ( ) ( ) ( ) ( )In Hartree-Fock theory we have: , ; ,occN
i inρ φ φ ρ′ ′= =∑r r r r r r r( ) ( ) ( ) ( ) ( )
( ) ( ) ( )1
2
3 3 3 3r,r1 1
The 2-electron repulsion is: d rd r2 2 r-r
i
ee
n nE d rd r
ρ=
′′′ ′= −
′ ′−∫ ∫r r
r rDirect or Hatree Exchange
So in HF theory self-repulsion is automatically removed.
.5
V(x) .3
.4
High and widebarrier
V0 0
.1
.2
x-2.0 -1.5 -1.0 -.5 0.0 .5 1.0 1.5 2.0
0.0
Self repulsionNo self repulsion
.3
.4
.5
High and widebarrier
p
.3
.4
.5
High and widebarrier
V(x)
.1
.2
.3 ba e
V(x)
.1
.2
x-2.0 -1.5 -1.0 -.5 0.0 .5 1.0 1.5 2.0
0.0
x-2.0 -1.5 -1.0 -.5 0.0 .5 1.0 1.5 2.0
0.0
• LSDA/GGA: no barrier• Scheffler et al:
– Electron to O2 too early – O - is strongly attracted– O2 is strongly attracted– Introduced “spin rules”– Lowering the spin on the
triplet O2 was forbidden – This is a strange ad hoc
mechanism
J. Behler, B. Delley, S. Lorenz, K. Reuter, and M. Scheffler,, Phys. Rev. Lett. 94 (3), 036104 (2005).
E.
PBE
Livshits, R
B3LYP
R. Baer andB3LYP d R. Koslof
BNL
ff, work in BNL progress ((2009)
1 1 121 1ˆ2
ˆ2
1j
j j j jj
Ur
T′≠ ′
∇ == − ∑ ∑
( )Unique gs WF of electrons having gs density nψ = r( )q g g g y gs
ψ
( )0Unique gs WF of non-int Fermions having gs density nψ = r
ˆ ˆˆgs gs
E T V Uψ ψ= + +
0 0ˆ ˆˆ
CT V U E nψ ψ ⎡ ⎤= + + + ⎢ ⎥⎣ ⎦
( ) ( ) 30 0
ˆ ˆgs gsV v n d r Vψ ψ ψ ψ= =∫ r r
ˆ ˆˆ ˆ⎡ ⎤0 0C gs gs
E n T U T Uψ ψ ψ ψ⎡ ⎤ = + − +⎢ ⎥⎣ ⎦
0 0ˆ ˆ
C gs gsT n T Tψ ψ ψ ψ⎡ ⎤ = −⎢ ⎥⎣ ⎦
⎡ ⎤ ⎡ ⎤0 0C CE n T n⎡ ⎤ ⎡ ⎤< >⎢ ⎥ ⎢ ⎥⎣ ⎦ ⎣ ⎦
•Theorem: A physical quantity cannot have self-repulsion•Corollary: Expectation values of physical operators are self-repulsion free•Corollary: Ec and Tc are self repulsion-free
U E n E nψ ψ ⎡ ⎤ ⎡ ⎤= +⎢ ⎥ ⎢ ⎥⎣ ⎦ ⎣ ⎦( )
0 0
Self-repulsion freeH X
U E n E nψ ψ +⎢ ⎥ ⎢ ⎥⎣ ⎦ ⎣ ⎦
( ) ( ) 3 31 n nE n d rd r
′⎡ ⎤ ′=⎢ ⎥⎣ ⎦ ∫∫
r r
( )2
Has self-repulsion
HE n d rd r=⎢ ⎥⎣ ⎦ ′−∫∫ r r
( )2
′
( )Has self-repulsion
( )3 3
,12X
E n d rd rρ ′
⎡ ⎤ ′= −⎢ ⎥⎣ ⎦ ′−∫∫r r
r r
( )Has self-attraction
0 0ˆ ˆˆ ˆ
C gs gsE n T U T Uψ ψ ψ ψ⎡ ⎤ = + − +⎢ ⎥⎣ ⎦( )self repulsion-free
( ) ( )( )⎡ ⎤ ∫ ( ) ( )( )( )
3
ˆˆ ˆ
,SLC XC X
T U T E
E n f n d r En
ψ ψ ψ ψ+ +
⎡ ⎤ = −⎢ ⎥⎣ ⎦ ∇∫ r r
( )0 0gs gs HT U T Eψ ψ ψ ψ+ − +
Long range self repulsion
0 0ˆ ˆˆ ˆ
C gs gsE n T U T Uψ ψ ψ ψ⎡ ⎤ = + − +⎢ ⎥⎣ ⎦ 0 0C gs gs
ψ ψ ψ ψ⎢ ⎥⎣ ⎦
( )0 0
1ˆ ˆ ˆC j jE n Y Y Y yψ ψ ψ ψ⎡ ⎤ = − = −⎢ ⎥⎣ ⎦ ∑ r r( )0 0 2C gs gs j j
jj
yγ γ γψ ψ ψ ψ′≠
⎢ ⎥⎣ ⎦ ∑
re γ− ( )erfc rγ1 1
0.25
0.30
ey
rγ =( )erfc r
yrγ
γ=
1 11
yrγ γ
=+
( ) ( )1
0 10
0.15
0.20
ˆ ˆ0 Y Y E T Eψ ψ ψ ψ
( ) ( )0
10y r y r
r ∞= =
2 3 4 5 6 7 8
0.05
0.10
0 00 :
gs gs C C CY Y E T Eγ γγ ψ ψ ψ ψ= − = − <
ˆ ˆ: 0Y Y Eγ ψ ψ ψ ψ= ∞ = >
Conclusion: There exists a for which there is equality γ0 0
: 0gs gs CY Y Eγ γγ ψ ψ ψ ψ= ∞ − = >
0 0ˆ ˆ
C gs gsE n Y Yγ γψ ψ ψ ψ⎡ ⎤ = −⎢ ⎥⎣ ⎦ 0 0
ˆC gs gs
y y
gs gs H XY E Eγ γ
γ γ
γψ ψ⎢ ⎥⎣ ⎦
⎡ ⎤= − −⎢ ⎥⎣ ⎦Fix γ and findGood approx for f(n,dn):
↓
( ) ( )( ) 3 yH b
↓
∫
•Becke (B3LYP)•…•Savin•Hirao( ) ( )( ) 3,
y
XC XHybC
f n nE d r E γγ ∇= −∫ r r
( ) ( )1∫∫
Hirao•Handy•Baer+Neuhauser•Yang
( )
( ) ( ) 3 31,
2y
XE y d rd rγ
γρ ′ ′ ′= − −∫∫ r r r r •Tozer•Truhlar•Head-Gordon•Gerber-Angyan
( )erfc1 1, ,
1
rr ey
r r r
γ
γ
γ
γ
−
=+
Gerber Angyan•Perdew-Scuseria•…
1 r r rγ+“B3LYP” typeLong-range self-repulsion
“RSH” typeNo long-range self-repulsion
1 Cε
11
C
C Ctγ ε
=+ −
1.0g
1 3
1sr
n∝
0 6
0.8
0.4
0.6
0.2
0 5 10 15 20rs
γ HOMOε− HOMOε−SCFΔγ 10a−wγ 10a−w
100
10
Unpolarized Polarized
1g
0.1
0.010 01 0 1 1 100.01 0.1 1 10
rs
E. Livshits and R. Baer, PCCP 9, 2932(2007)
Pair correlation function taken from:P. Gori-Giorgi and J. P. Perdew, Phys. Rev. B 66, 165118 (2002).
• In B3LYP – OK• In RSH – NOT OK• Must be: γ system dependent
30
25
HOMO B3LYP
Exp. Vertical Theorem:Theorem:
Th i i tiTh i i ti
15
20
(eV)
Basis: cc-pVTZThe ionization The ionization
potential of the potential of the
t i tlt i tl
10
IP system is exactly system is exactly
equal to the HOMO equal to the HOMO
5
energyenergy
0
• M. Levy and J. P. Perdew, in Density Functional Methods in Physics, edited by R. Dreizler and J. Perovidencia (Plenum, New York, 1985), pp. 11.
• C.‐O. Almbladh and U. von‐Barth, Phys. Rev. B 31, 3231 (1985).
γ HOMOε− HOMOε−SCFΔγ 10a−wγ 10a−w
Molecule
γ(a0
-1)
IP exp
IPw=0
IPw=0.1
IPB3LYP
( );HOMO Nε γ
Li2 0.3 5.1 -0.1 0.0 -0.2N2 0.6 15.6 -1.0 -0.6 0.0O2 0.7 12.1 -1.2 -0.9 -0.7F 0 7 15 7 -0 8 -0 4 0 1
( )( ) ( ); 1;E N E Nγ γ= − −
F2 0.7 15.7 -0.8 -0.4 0.1Na2 0.4 4.9 -0.2 -0.1 -0.3P2 0.8 10.6 -0.4 -0.3 0.0S2 0.5 9.4 -0.4 -0.2 -0.2Cl2 0.5 11.5 -0.3 0.0 0.1BeH 0.6 8.2 -0.2 -0.1 -0.2CO 0.6 14.0 -0.3 -0.1 0.0HF 0 7 16 0 -0 4 0 0 0 0HF 0.7 16.0 -0.4 0.0 0.0HCl 0.5 12.8 0.0 0.3 0.2NH3 0.5 10.2 -0.6 -0.4 -0.5PH3 0.4 9.9 -0.6 -0.4 -0.6
E. Livshits and R. Baer, PCCP 9, 2932 (2007)
Mean -0.5 -0.2 -0.2
RMS 0.6 0.4 0.3
‐0.48
‐0.52
‐0.50
HF
H2+
QCHEM 3.1
0 56
‐0.54
E(E h)
B3LYP
BLYP
cc-pVTZ
Same
‐0.58
‐0.56 Same problems appear in:
‐0.62
‐0.60 He2+, Ne2
+
etc0 1 2 3 4 5 6 7 8 9
H‐H distance (A)
R Merkle A Savin and H Preuss J Chem Phys 97 9216 (1992)R. Merkle, A. Savin, and H. Preuss, J. Chem. Phys. 97, 9216 (1992).Y. Zhang and W. Yang, J. Chem. Phys. 109, 2604 (1998).A. Ruzsinszky, J. P. Perdew, G. I. Csonka, O. A. Vydrov, and G. E. Scuseria, J. Chem. Phys. 126, 104102 (2007).
LR R+
r → ∞
L
( )( ) ( ) ( )
1
2R R
GS L R
E r E E +
= ±
→ +
RR+
( ) ( ) ( )
4
R R
...2
correctE r E E
r
α
→ +
− +R
0 5 0 5( )1
Density Picture:
n n n+R0.5 R0.5( )
( ) ( )0.5
214
2
L Rn n n
E r E Rr
= +
= +
‐0.50
‐0.48
By using RSH we get id f l i
0 54
‐0.52 HF
B3LYP
BLYP
rid of repulsion
But this is not enough
h l l‐0.56
‐0.54
E(E h) BLYP
γ=0.5There is also large error at r = r0Wrong as mptotic
‐0.60
‐0.58 Wrong asymptotic curve (≠ -α/2r4)
‐0.62
0 1 2 3 4 5 6 7 8 9
H‐H distance (A)
E. Livshits and R. Baer, J. Phys. Chem A 112, 12789 (2008).
( ) 0 1 0.5 0.5E E Eγ γγ − −Δ = −
1 4
1.6
Ne2+
( ) γ γ
E HF γ→ ∞
0 8
1.0
1.2
1.4
)
Ne2+
He2+
H2+ ΔE
ΔE
0 2
0.4
0.6
0.8
ΔE (eV)
LDA γ → 0
ΔE
0 4
‐0.2
0.0
0.2
( )Åeqr
‐0.4
0.4 0.6 0.8 1.0 1.2 1.4 1.6 1.8 2.0
γ (1/a0)
( )eq
2ωR+R+ R++RR0.5++R0.5+
E. Livshits and R. Baer, J. Phys. Chem A 112, 12789 (2008).
E. Livs
• Have γ so: localized-delocalized degenerate• Have γ so: localized-delocalized degenerate
hits and R.
• Energies in kcal/mole• Energies in kcal/moleProperty R BLYP B3LYP HF LC LC* Exp
Baer, J. P
h
Property R BLYP B3LYP HF BNL BNL* Exp.
Enthalpy by atomization
H 66 65 60.9 60.9 60.9 61He 82 75 43 74 59 55N 75 60 2 59 34 32
hys. Chem
ANe 75 60 2 59 34 32
Enthalpy by asymptote
H NA NA 60.9 50 60.9 61He NA NA 43 42 59 55Ne NA NA 2 27 34 32H 1 1 1 1 1 06 1 2 1 06 1 05
A 112, 1278
H 1.1 1.1 1.06 1.2 1.06 1.05He 1.2 1.1 1.075 1.2 1.078 1.080Ne 1.9 1.9 1.7 1.760 1.72 1.765H 2.7 2.9 3.3 2.9 3.3 3.32H 1 7 2 0 2 5 2 1 2 5 2 42
( )eqr Å
2ω
89 (2008).
2ω
He 1.7 2.0 2.5 2.1 2.5 2.42Ne 0.5 0.6 0.9 0.726 0.8 0.729H NA NA 1 0.6 1 1He NA NA 0.98 NA 0.98 1N NA NA 1 01 NA 1 02 1
2ω
R effα α ( ) 51
2effE r rα ′=
R refα α
Ne NA NA 1.01 NA 1.02 1H 5.3 5.6 4.51 5.8 4.51 4.50He 1.6 1.5 1.34 1.8 1.41 1.38Ne 3.1 2.9 2.4 3.2 2.70 2.66
ff
( )30
daugRa a
( )2ff
By using γ* several y g γproblems are solvedp
Repulsion instead of
i
No degeneracy
b kiProper well depth at r=r0
Fine bond lengths
“Good vibrations”
Leading term in asymptotic
form of i l
Excellent atomic l i biliattraction breaking depth at r r0 lengths vibrations potential -
correctpolarizability
E. Livshits and R. Baer, J .Phys. Chem, A 112, 12789 (2008).
Energies (kcal/mol) of (H2O)2+ relative to
Method Vertical neutral
Hemi-bonded
2 2the proton‐transferred geometry
neutral bonded
BLYP 6.7 ‐8.3B3LYP -1.6
E. Livshits, A. I. Krylov and R. Baer, work in progress
BNL*(0.56) 23.3 8.2EOM-IP-CCSD 20.0 5.3EOM-IP-CC(2.3) 21.8 7.4
p g(2009).
Neutral dimer Hemi‐bonded
Proton‐transferred
• We looked into the Anthracene-TCNE charge transfer complex in solution (CH2Cl2)
1• In ideal CT excitation: 1CT ArH A
h IP EAR
νε
= − −
J. M. Masnovi, E. A. Seddon, and J. K. Kochi, Can. J. of Chem . 62 (11), 2552 (1984).
• First stage is to find the appropriate γ• This requires finding a γ that gives proper q g γ g p p
HOMO energies for IP(ArH) and EA(TCNE)γ IP (ANT) (eV) IP (TCNE-) = EA (eV) Σrγ IP (ANT) (eV) IP (TCNE ) = EA (eV) Σr
ΔESCF ‐εHOMO r ΔESCF ‐εHOMO r0.01 6.09 4.03 0.34 0.59 -0.90 2.53 2.870 02 6 09 4 22 0 31 1 69 0 73 1 43 1 740.02 6.09 4.22 0.31 1.69 -0.73 1.43 1.74
0.033 6.14 4.44 0.28 1.72 -0.52 1.30 1.580.05 6.18 4.71 0.24 1.77 -0.24 1.14 1.38
0 3 6 91 7 02 0 02 2 44 2 34 0 04 0 060.3 6.91 7.02 -0.02 2.44 2.34 0.04 0.060.4 7.04 7.35 -0.04 2.69 2.88 -0.07 0.120.5 7.08 7.56 -0.07 2.89 3.27 -0.13 0.20
• One obtains an optimal value of 0.3
• Checking the Mulliken law in gas phase3.8
3 6
3.7TDDFT g=0.3
Mulliken
3.5
3.6
E (eV)
3 3
3.4
3.2
3.3
0 02 0 025 0 03 0 035 0 04 0 045 0 050.02 0.025 0.03 0.035 0.04 0.045 0.05
1/R(a0)1CT ArH A
h I EAR
ν = − −
• We took a B3LYP optimized geometry for the complex and performed TDDFT calculation
Ar B3LYP BNLγ=0.5
BNL γ* ExpΕ f γ* Ε f Ε f2 1 0 03 4 4 0 33 3 8 0 03 3 59 0 02Benzene 2.1 0.03 4.4 0.33 3.8 0.03 3.59 0.02
Toluene 1.8 0.04 4.0 0.32 3.4 0.03 3.36 0.03o‐Xylene 1.5 ~0 3.7 0.31 3.0 0.01 3.15 0.05Naphthalene 0.9 ~0 3.3 0.32 2.7 ~0 2.60 0.01
T. Stein, L. Kronik and R. Baer, JACS to be published (2008).
Substituent PBE B3‐LYP
BNL Exp26Ε(γ=0.5) γ∗ Ε(γ=0.3)
None 0.9 1.0 2.3 0.31 1.82 1.739‐cyano Fail 0.5 2.6 0.30 2.03 2.019‐chloro 0.9 1.0 2.3 0.31 1.82 1.749‐carbo‐ 0 8 0 9 2 4 0 30 1.84 1.849 carbomethoxy
0.8 0.9 2.4 0.30 1.84 1.84
9‐methyl 1.0 1.1 2.1 0.30 1.71 1.559‐nitro 0 6 0 9 2 8 0 30 2 12 2 039‐nitro 0.6 0.9 2.8 0.30 2.12 2.039.10‐dimethyl
1.3 1.4 2.1 0.30 1.77 1.44
9 formyl 0 8 1 0 2 5 0 30 1 95 1 909‐formyl 0.8 1.0 2.5 0.30 1.95 1.909‐formyl 10‐chloro
0.8 0.9 2.5 0.30 1.96 1.96
T. Stein, L. Kronik and R. Baer, JACS to be published (2008).
• Kohn-Sham bad gaps (50-70% too small)• Because missing “derivative discontinuity”g y• Hartree-Fock theory terrible: 500% too large.
LDAE E
γ−
g g
Hartree Fock LDA
g g
E E
E E−
−
0.2
0.16
0.18 NaCl* C
Aγ
ε=
0 1
0.12
0.14
∗ MgO
optAε −
0.22C =
0 06
0.08
0.1γ∗
AlPC
0.8A=
0.02
0.04
0.06 AlP
AlN
SiC AlA
GaP
Si
0
0 2 4 6 8 10 12 14
SiC AlAsAlSb
εOpt
3.0
2.5
2.0
ap (e
V)
ExpGaP AlP
1.0
1.5
Ban
d G
a ExpgHSELSDA
AlSbSiC
0.5
1.0 LSDAAlSb
0.01 0 1 5 2 0 2 5
Si
1.0 1.5 2.0 2.5Experimental Band gap (eV)
H. Eisenberg, R. Baer, work in progress (2008).
8.0
7.0
)
6.0
Ban
d G
ap (e
V)
Exp
γ
HSEMgO
4.0
5.0
B HSE
LSDA
AlN
MgO
NaCl
3.0
4.0
4 0 5 0 6 0 7 0 8 0
CNaCl
AlN
4.0 5.0 6.0 7.0 8.0
Experimental Band gap (eV)
H. Eisenberg, R. Baer, work in progress (2008).
Dogmatic spirit Pragmatic spirit spirit
Hybrid (B3LYP/RSH) theory
γ system depende
nt
Ab initio ways to
determine γ
“Systems too difficult for DFT”
In B3LYP: In RSH: γγ
insensitive to density (factor 3)
γvery
sensitive (factor ~100)
Symmetric cation
radicals
Charge-transfer
excitationsBand gaps