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excitations

Ament, L.J.P.

Citation

Ament, L. J. P. (2010, November 11). Resonant inelastic x-ray scattering studies of elementary excitations. Casimir PhD Series. Retrieved from https://hdl.handle.net/1887/16138

Version: Not Applicable (or Unknown)

License: Leiden University Non-exclusive license Downloaded from: https://hdl.handle.net/1887/16138

Note: To cite this publication please use the final published version (if applicable).

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A p p e n d i x A

QED

This appendix contains some details of the derivation of the higher-order electron- photon coupling Hamiltonian.

A.1 H

Ψ

to second order

Below the components of HΨ= ΩHα−1+ i~(∂tΩ)Ω−1 are calculated. First, ΩHα−1= Hα+1

2

h ˜D2, Hα

i

= Hα+1 2

h ˜D2, −eφi

. (A.1)

where in the last step only terms up to O(m−2) are kept, and where (2mc)2h ˜D2, φi

= σiσj(DiDjφ − φDiDj) = σiσj(Di(∂jφ) + DiφDj− φDiDj)

= σiσj(∂i(∂jφ) + (∂jφ)Di+ (∂iφ)Dj) = ∂i2φ + 2(∂iφ)Di

= −ρ/0+2i

~

(∇φ) · (p + eA). (A.2)

Second,

i~∂tΩ = i~

2(2mc)2t(p + eA)2+ e~σ · B

= ie~

2(2mc)2[(∂tA) · (p + eA) + (p + eA) · (∂tA) + ~σ · (∂tB)]

= ie~

2(2mc)2[2(∂tA) · (p + eA) + ~σ · (∂tB)] (A.3)

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Putting things together, one finds HΨ= Hα−1

2 e~2ρ (2mc)20

− ie~

(2mc)2E · (p + eA) + ie~2

2(2mc)2σ · (∂tB)

= (p + eA)2

2m + e~

2mσ · B − eφ + e~

(2mc)2σ · E × (p + eA) + 1 2

e~2ρ (2mc)20

− ie~

2(2mc)2~σ · (∂tB). (A.4)

Note that the E × p term is not Hermitian for dynamic fields, because E and p do not commute in that case. The ‘imaginary term’ in HΨ solves this issue: it can be rewritten as

− ie~

2(2mc)2k(∂tBk) = ie~2

2(2mc)2ijkσk(∂iEj) = ie~2

2(2mc)2ijkσk(∂iEj− Eji)

= − e~

2(2mc)2ijkσk(−i~∂iEj+ Ei(−i~)∂j)

= − e~

2(2mc)2σ · (p × E + E × p) (A.5)

With this substitution, HΨ assumes the form of Eq. (2.22).

A.2 H

Ψ

to third order

This section contains the derivation of HΨto order O(m−3).

Starting point is Eq. (2.7):

β(x) = ˜Dα(x) + ˜D0Dα(x) + ˜˜ D02Dα(x).˜ (A.6) Substitution in Eq. (2.5) gives the equation for α(x):

0α(x) + ˜D

1 + ˜D0+ ˜D02 ˜Dα(x) = 0. (A.7) Every ˜D0 is commuted to the right:

0 =



0+ ˜D2+ ˜D 1 + ˜D0



D ˜˜D0+ ie~

(2mc)2iEi



α(x)

=



0+ ˜D2+ ˜D



D ˜˜D0+ ie~

(2mc)2iEi



+ ˜D



D ˜˜D0+ ie~

(2mc)2iEi



0+ ˜D0 ie~

(2mc)2iEi



α(x) (A.8) Using

h ˜D0, Eii

= −i~

2mc(∂0Ei), (A.9)

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A.2 HΨ to third order 193

one obtains

− ˜D0α(x) =

 D˜2

1 + ˜D0+ ˜D02

+ ˜D ie~

(2mc)2iEi

1 + 2 ˜D0



+ ˜De~2σi(∂0Ei) (2mc)3c



α(x). (A.10)

0α(x) is replaced by the second order Schr¨odinger equation, and only terms that contribute to the Schr¨odinger equation at order O(m−3) are considered:

− ˜D0α(x) =

 D˜2

1 − ˜D2

+ ˜D ie~

(2mc)2iEi+ ˜De~2σi(∂0Ei) (2mc)3c



α(x). (A.11) The normalization condition becomes

Z d3x



α(x)α(x) +n

1 + ˜D0+ ˜D20 ˜Dα(x)on

1 + ˜D0+ ˜D20 ˜Dα(x)o

= 1.

(A.12) Up to order O(m−3), this is

1 = Z

d3x



α(x)+ α(x)2+n ˜D0Dα(x)˜ o

D + α(x)˜ D ˜˜D0

 α(x)

= Z

d3x

"

α(x)+ α(x)2+



D ˜˜D0+ ie~

(2mc)2iEi

 α(x)



+α(x)



D ˜˜D0+ ie~

(2mc)2iEi



α(x)

= Z

d3x α(x)

"

1 + ˜D2+

 ie~

(2mc)2iEi



D + ˜˜ D ie~

(2mc)2iEi

# α(x)

= Z

d3x α(x)



1 + ˜D2+ e~

(2mc)2c

h ˜D, iσiEii

α(x), (A.13)

where the commutator h ˜D, iσiEii

= ~

2mc σiσj(∂iEj) − 2iijkσkEiDj

(A.14) is hermitian. The renormalization operator becomes

Ω(x) = 1 + 1 2



2+ e~

(2mc)2c

h ˜D, iσiEii

= Ω(x), (A.15) so that to order O(m−3)

Ω(x)−1= 1 −1 2



2+ e~

(2mc)2c

h ˜D, iσiEii

. (A.16)

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With this renormalization operator, one can obtain the Schr¨odinger equation for the normalized wave function Ψ(x). Its Hamiltonian HΨ consists of the parts

i~(∂tΩ)Ω−1= ie~

2(2mc)2{2(∂tA) · (p + eA) + ~σ · (∂tB)}

+ e 2c

 −i~

2mc

3

σiσj(∂tiEj) − 2iijkσk(∂tEiDj)

(A.17) and

ΩHα−1= 2mc2



− eφ

2mc2 + ˜D2− ˜D4+ ˜D ie~

(2mc)2iEi+ ˜De~2σi(∂0Ei) (2mc)3c



+ 1 2



2+ e~

(2mc)2c

h ˜D, iσiEii

, −eφ + 2mc22



= −eφ + (p + eA)2

2m + e~

2mσ · B − 1 2mc2

 (p + eA)2

2m + e~

2mσ · B

2

− e −i~

2mc

2

σjσiDjEi− e −i~

2mc

3

σjσiDj(∂0Ei)

− −i~

2mc

2e

2 ∂2iφ + 2(∂iφ)Di − e2~ 2(2mc)2c

hh ˜D, iσiEii , φi

, (A.18) where the commutator is

hh ˜D, iσiEii , φi

= −h

φ, ˜DiσiEii +h

φ, iσiEiD˜i

= −h φ, ˜Di

iEi− ˜Dφ, iσiEi + φ, iσiEiD + iσ˜ iEih φ, ˜Di

= −h φ, ˜Di

iEi+ iσiEih φ, ˜Di

= ~

2mc σjσi− σiσj Ei(∂jφ)

= ~

2mci2jikσkEi(∂jφ) = −i~

2mc2 σ · E × (∇φ), (A.19) so that

ΩHα−1= −eφ + (p + eA)2

2m + e~

2mσ · B − 1 2mc2

 (p + eA)2

2m + e~

2mσ · B

2

− e −i~

2mc

2

σjσiDjEi− e −i~

2mc

3

σjσiDj(∂0Ei)

− −i~

2mc

2e

2 ∂2iφ + 2(∂iφ)Di + ie2~2

(2mc)3cσ · E × (∇φ). (A.20) Putting the O(m−3) term of HΨtogether, one obtains

− 1 2mc2

 (p + eA)2

2m + e~

2mσ · B

2

− e −i~

2mc

3

σjσiDj(∂0Ei) +

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A.2 HΨ to third order 195

+ ie2~2

(2mc)3cσ · E × (∇φ) + e 2c

 −i~

2mc

3

σiσj(∂tiEj) − 2iijkσk(∂tEiDj)

= 1

(2mc)3



−c (p + eA)2+ e~σ · B2

+ie2~2

c σ · E × (∇φ)

−e

2c(−i~)3σjσi(∂jtEi) + (∂tEi)Dj+ Dj(∂tEi) +e(−i~)3

2c



σiσj(∂tiEj) − 2iijkσk



(∂tEi)Dj+ie

~

Ei(∂tAj)



= 1

(2mc)3



−c (p + eA)2+ e~σ · B2

+e(−i~)3

2c −2iijkσk(∂tEi)Dj

−e

2c(−i~)3σjσi(∂tEi)Dj+ Dj(∂tEi) −ie2~2

c σ · E × E



= 1

(2mc)3

h−c (p + eA)2+ e~σ · B2

−e (−i~)3

2c (∂tEi)Di+ Di(∂tEi) − iijkσk(∂tjEi)

#

, (A.21)

giving Eq. (2.23).

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A p p e n d i x B

YTiO 3

This appendix contains some of the lengthy expressions involved in calculating the RIXS spectra of YTiO3(section 5.4).

B.1 RIXS – Single site processes

The angular momentum ˆl and quadrupole operators ˆQ, ˆT in Eqs. (5.43−5.45) are defined as follows:

ˆlx= i(cb − bc) (B.1)

ˆly= i(ac − ca) (B.2)

ˆlz= i(ba − ab) (B.3)

x= ˆl2x− ˆly2= nb− na (B.4) Qˆz= 1

√3(ˆlx2+ ˆl2y− 2ˆl2z) = 1

√3(2nc− na− nb) (B.5) Tˆx= ˆlyˆlz+ ˆlzˆly= −(bc + cb) (B.6) Tˆy= ˆlxˆlz+ ˆlzˆlx= −(ca + ac) (B.7) Tˆz= ˆlxˆly+ ˆlyˆlx= −(ab + ba) (B.8)

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which are normalized by Tr ˆΓ2

= 2. The corresponding matrices Γd0d in Eq. (5.41) are

ΓQx =1 2

−1 0 0

0 1 0

0 0 0

, ΓQz = 213

−1 0 0

0 −1 0

0 0 2

,

ΓTx = −1 2

0 0 0 0 0 1 0 1 0

, ΓTy = −12

0 0 1 0 0 0 1 0 0

,

ΓTz = −1 2

0 1 0 1 0 0 0 0 0

, Γlx= 12

0 0 0

0 0 i

0 −i 0

,

Γly = 1 2

0 0 −i

0 0 0

i 0 0

, Γlz =12

0 i 0

−i 0 0

0 0 0

 (B.9)

with the indices d, d0 = (yz, zx, xy) (or for polarization dependence: α, β = (x, y, z)).

B.2 Multiplet factors

For the multiplet effect factors in Eq. (5.46), we have

MdA01gd = r2

3(hd0| ˆx |mi hm| ˆx |di + hd0| ˆy |mi hm| ˆy |di + hd0| ˆz |mi hm| ˆz |di) (B.10) MdQ0dx= (hd0| ˆy |mi hm| ˆy |di − hd0| ˆx |mi hm| ˆx |di) (B.11) MdQ0dz = 1

√3(2 hd0| ˆz |mi hm| ˆz |di − hd0| ˆx |mi hm| ˆx |di − hd0| ˆy |mi hm| ˆy |di) (B.12) MdT0xd= − (hd0| ˆy |mi hm| ˆz |di + hd0| ˆz |mi hm| ˆy |di) (B.13) MdT0yd= − (hd0| ˆz |mi hm| ˆx |di + hd0| ˆx |mi hm| ˆz |di) (B.14) MdT0zd= − (hd0| ˆx |mi hm| ˆy |di + hd0| ˆy |mi hm| ˆx |di) (B.15) Mdlx0d= −i (hd0| ˆy |mi hm| ˆz |di − hd0| ˆz |mi hm| ˆy |di) (B.16) Mdly0d= −i (hd0| ˆz |mi hm| ˆx |di − hd0| ˆx |mi hm| ˆz |di) (B.17) Mdlz0d= −i (hd0| ˆx |mi hm| ˆy |di − hd0| ˆy |mi hm| ˆx |di) (B.18) Note that the position operators act on the core electrons, not the t2g ones. Both the core and t2g electrons are implied in the states |di , |d0i.

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B.3 The operators ˆΓ in terms of orbitons 199

B.3 The operators ˆ Γ in terms of orbitons

In terms of the orbiton operators, we obtain the one-orbiton creation part of Γˆq=P

ieiq·riΓˆi to be

ˆl(1)x,q−q

1 =i |c0| 2

rN 3

hn(1 −√

3)uq+ (1 +√ 3)vqo

(sh θ1,q+ ch θ1,q1,−q +n

(−1 −√

3)uq+ (1 −√ 3)vqo

(sh θ2,q+ ch θ2,q2,−qi

(B.19) ˆly,q−q(1) 2 =i |c0|

2 rN

3 hn

(1 +√

3)uq+ (1 −√ 3)vqo

(sh θ1,q+ ch θ1,q1,−q +n

(−1 +√

3)uq+ (1 +√ 3)vqo

(sh θ2,q+ ch θ2,q2,−qi

(B.20) ˆl(1)z,q−q3 = −i |c0|

rN 3 h

(uq+ vq)(sh θ1,q+ ch θ1,q1,−q + (vq− uq)(sh θ2,q+ ch θ2,q2,−qi

(B.21) Tˆx,q−q(1) 1 =|c0|

6

√ Nhn

(1 +√

3)uq+ (−1 +√ 3)vqo

(ch θ1,q− sh θ1,q1,−q +n

(1 −√

3)uq+ (1 +√ 3)vqo

(ch θ2,q− sh θ2,q2,−q i

(B.22) Tˆy,q−q(1)

2 =|c0| 6

√ Nhn

(1 −√

3)uq+ (−1 −√ 3)vqo

(ch θ1,q− sh θ1,q1,−q +n

(1 +√

3)uq+ (1 −√ 3)vqo

(ch θ2,q− sh θ2,q2,−q i

(B.23) Tˆz,q−q(1) 3 = −|c0|

3

√ Nh

(uq− vq)(ch θ1,q− sh θ1,q1,−q + (uq+ vq)(ch θ2,q− sh θ2,q2,−qi

(B.24) Qˆ(1)x,q = |c0|

rN 3

h−(uq+ vq)(ch θ1,q− sh θ1,q1,−q + (uq− vq)(ch θ2,q− sh θ2,q2,−qi

(B.25) Qˆ(1)z,q= − |c0|

rN 3

h

(uq− vq)(ch θ1,q− sh θ1,q1,−q + (uq+ vq)(ch θ2,q− sh θ2,q2,−qi

(B.26) with q1 = (π, 0, π), q2 = (π, π, 0), q3 = (0, π, π). The expressions for the two-orbiton creation part of ˆΓq=P

ieiq·riΓˆi are ˆl(2)x,q= i

√3 X

k

h

(vu0− uv0)ch θ1sh θ01α1,kα1,−k−q

1−q +

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+ (vu0− uv0)ch θ2sh θ02α2,kα2,−k−q

1−q

+ (uu0+ vv0)(ch θ1sh θ20 − sh θ1ch θ201,k α2,−k−q

1−q

i

(B.27) with u, v, θ1, θ2= uk, vk, θ1,k, θ2,k and primed quantities u0, v0, θ10, θ02= uk+q1+q, vk+q1+q, θ1,k+q1+q, θ2,k+q1+q. Further, ˆl(2)y,qand ˆl(2)z,qhave the same form as ˆlx,q(2)

but with q1 replaced by q2and q3 respectively. Next, Tˆx,q(2) =X

k



−(uu0+ vv0) +uu0− vv0

√3 +uv0+ vu0 3



ch θ1sh θ01α1,kα1,−k−q

1−q

+



−(uu0+ vv0) −uu0− vv0

√3 −uv0+ vu0 3



ch θ2sh θ02α2,kα2,−k−q

1−q

+



−(uv0− vu0) −uv0+ vu0

√3 −uu0− vv0 3



(ch θ1sh θ20 + sh θ1ch θ20

α1,k α2,−k−q

1−q

i

(B.28) Tˆy,q(2)=X

k



−(uu0+ vv0) −uu0− vv0

√3 +uv0+ vu0 3



ch θ1sh θ01α1,kα1,−k−q

2−q

+



−(uu0+ vv0) +uu0− vv0

√3 −uv0+ vu0 3



ch θ2sh θ02α2,kα2,−k−q

2−q

+



−(uv0− vu0) +uv0+ vu0

√3 −uu0− vv0 3



(ch θ1sh θ20 + sh θ1ch θ20

α1,k α2,−k−q

2−q

i (B.29)

where in the expression for ˆTy,q(2) we replaced q1 by q2: u0, v0, θ10, θ02 = uk+q2+q, vk+q2+q, θ1,k+q2+q, θ2,k+q2+q.

z,q(2)=X

k



−2

3(uv0+ vu0) − (uu0+ vv0)



ch θ1sh θ10 α1,kα1,−k−q

3−q

+ 2

3(uv0+ vu0) − (uu0+ vv0)



ch θ2sh θ20 α2,kα2,−k−q

3−q

+ 2

3(uu0− vv0) − (uv0− vu0)



(ch θ1sh θ02+ sh θ1ch θ021,kα2,−k−q

3−q

 (B.30) where we replaced q1 by q3: u0, v0, θ10, θ20 = uk+q3+q, vk+q3+q, θ1,k+q3+q, θ2,k+q3+q. Finally,

(2)x,q= − 1

√3 X

k

h−(uu0− vv0)ch θ1sh θ10 α1,kα1,−k−q

+ (uu0− vv0)ch θ2sh θ02α2,kα2,−k−q+

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B.4 RIXS – two-site processes with superexchange model 201

+ (uv0+ vu0)(ch θ1sh θ20 + sh θ1ch θ201,kα2,−k−qi

(B.31) Qˆ(2)z,q= 1

√3 X

k

h

(uv0+ vu0)ch θ1sh θ01α1,kα1,−k−q

− (uv0+ vu0)ch θ2sh θ02α2,kα2,−k−q

− (uu0− vv0)(ch θ1sh θ20 + sh θ1ch θ201,kα2,−k−qi

(B.32) where in both equations we replaced q1by 0: u0, v0, θ10, θ20 = uk+q, vk+q, θ1,k+q, θ2,k+q.

B.4 RIXS – two-site processes with superex- change model

Functions f11, f22and f12in Eqs. (5.79−5.80) are:

f11(k, q) = [−γ3,q(uv0+ u0v) − γ2,q(uu0− vv0) − (1 + γ1,q)(uu0+ vv0)] × (ch θ1sh θ01+ sh θ1ch θ01)

+ 2 [γ10(uu0+ vv0) + γ20(uu0− vv0) + γ30(uv0+ u0v)] ×

(sh θ1sh θ10 + ch θ1ch θ01) (B.33) f22(k, q) = [γ3,q(uv0+ u0v) + γ2,q(uu0− vv0) − (1 + γ1,q)(uu0+ vv0)] ×

(ch θ2sh θ02+ sh θ2ch θ02)

+ 2 [γ10(uu0+ vv0) − γ20(uu0− vv0) − γ30(uv0+ u0v)] ×

(sh θ2sh θ20 + ch θ2ch θ02) (B.34) f12(k, q) = 2 [γ3,q(uu0− vv0) + γ2,q(uv0+ u0v) − (1 + γ1,q)(uv0− u0v)] ×

(ch θ1sh θ02+ sh θ1ch θ02)

+ 4 [γ10(uv0− u0v) + γ20(uv0+ u0v) − γ30(uu0− vv0)] ×

(sh θ1sh θ20 + ch θ1ch θ02) (B.35) where we shortened notation by writing θ1/2 = θ1/2,k, θ01/2 = θ1/2,k+q, u(0) = uk(+q), v(0) = vk(+q)and γi0= γi,k+q.

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A p p e n d i x C

Phonon RIXS

This appendix contains the lengthy derivations involved in calculating the Ein- stein phonon RIXS spectra of chapter 7. In the following, we evaluate the scat- tering amplitude (7.8). We use (see Mahan [62], section 4.3.2)

hn|eω0M(b−b)

n0 = e−g/2hn| eω0Mbeω0Mb n0

= e−g/2

n

X

k=0 n0

X

l=0

hn−k|(M/ω0)k k!

 n!

(n − k)!

12 (−M/ω0)l l!

 n0! (n0− l)!

12

n0−l

= e−g/2

n

X

k=0 n0

X

l=0

(M/ω0)k k!

 n!n0! (n − k)!(n0− l)!

12 (−M/ω0)l

l! δn0−l,n−k

=





e−g/2Pn0 l=0

(M/ω0)l−n0 +n (l−n0+n)!

h n!n0! (n−(l−n0+n))!(n0−l)!

i12 (−M/ω

0)l

l! for n > n0 e−g/2Pn

k=0

(M/ω0)k k!

h n!n0! (n−k)!(n0−(n0−n+k))!

i12 (−M/ω

0)n0 −n+k

(n0−n+k)! for n ≤ n0

=

e−g/2Pn0 l=0

(−1)l(M/ω0)2l−n0 +n l!(l−n0+n)!

n!n0!

(n0−l)! for n > n0 e−g/2Pn

l=0

(−1)l+n0 −n(M/ω0)2l+n0 −n l!(l+n0−n)!

n!n0!

(n−l)! for n ≤ n0

(C.1)

with g = m220. For simplicity, we assume the system is initially in its ground state: n0= 0. In that case, the above expression simplifies to

hn| eω0M(b−b)|0i = e−g/2(M/ω0)n

√n! . (C.2)

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These expressions are inserted in the Kramers-Heisenberg equation (7.12):

Ff g= Tel(0, )X

i

eiq·RiFi (C.3)

with

Fi= e−g

n0i

X

n=0 n

X

l=0

(−1)l+n0i−n(M/ω0)2l+n0i l!(l + n0i− n)!

pn0i! (n − l)!

1 z + (g − n)ω0

+ e−g

X

n=n0i+1 n0i

X

l=0

(−1)l(M/ω0)2l−n0i+2n l!(l − n0i+ n)!

pn0i! (n0i− l)!

1 z + (g − n)ω0

. (C.4)

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A p p e n d i x D

Magnetic spectral weight at the Γ point in 2D cuprates

This appendix contains the calculational details from Sec. 4.5.5, where the leading magnetic contribution to the q = 0 RIXS spectra at the Cu L edge is established.

D.1 H ¯

eff(4)

to fourth order in t/U

In this section we evaluate Eq. (4.74) in the presence of a core hole.

The first term of Eq. (4.74) changes the Hamiltonian to H¯eff(4)= H0−4t2

U X

i

pipiX

δ

Si· Si+δ+ . . . (D.1)

where pi creates a core electron, δ points to nearest neighbors, and the dots indicate the corrections to H0 due to the four hop terms.

To handle the four hop terms systematically, we categorize all terms according to the ‘connections’ between sites. With a ‘connection’ is meant that one or more hops occur between the sites in question. For example, only the sites i and j, and j and k are connected if we select the following four hoppings from the V ’s:

tijX

σ

(cc+ cc) × ... × tjkX

σ0

(c0c0+ c 0c0) × ... × tij(...) × ... × tjk(...), (D.2)

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but also processes with a different hopping order like tijtijtjktjkand tjktijtijtjk, etc., have the same connections and are thus categorized together. We will there- fore represent the category comprising all these processes by t2ijt2jk. The order of the t’s is not important, only the number of times a certain hop occurs is important for indicating the category.

We now establish the different categories. The most general string of t’s is tijtkltmntpq. A lot of these processes change the occupancy of one of the sites.

These terms vanish because of the P0’s at the beginning and end of every four hop term. This imposes a restriction on the indices i, j, k, l, m, n, p, q: if an index appears an odd number of times, the occupancy is changed and the process does not contribute to Heff(4). We are left with the following categories: (a) t4ij, (b) t2ijt2kl(i, j 6= k, l), (c) t2ijt2jk(i 6= k), and (d) tijtjktkltli (i, j, k, l form a square). If there is no core hole present at any of the sites involved, we can just copy-paste the results from Ref. [82]. Below we analyze the processes where there is a core hole present.

Processes in category (a) do not flip any spins. The doublon (the doubly occupied site) hops 4 times between site i and j, where i is the core hole site.

We obtain the (a) contribution:

Heff(4) = · · · + pipi t4 Uc3P0X

σ

ccccP0ccccP0, (D.3)

where the dots indicate other fourth order terms. At the core hole site, cc= 1, and we use the projected spins as defined in Eq. (2.14) of Ref. [82] to get

Heff(4)= · · · + pipi t4 Uc3

 {1

2(1 − σjz)}2+ {1

2(1 + σzj)}2



= · · · + pipi t4

Uc311. (D.4) The corresponding part of H0 is

H0= · · · −16t4

U3 Si· Sj (D.5)

which should be replaced by Eq. (D.4). Dropping the constant term, this gives H¯eff(4)= H0+X

i

pipiX

δ

16t4

U3 Si· Si+δ+ . . . (D.6) Processes in category (b) do not appear in the fourth order expansion of the half-filled Hubbard model. If we add one doubly occupied site (namely, the core hole site i), there still is no contribution to ¯Heff(4). The only matrix elements for which this is not a priori clear, involve configurations pictured in Fig. D.1.

If the spins at k and l are parallel, the corresponding matrix element is obvi- ously zero. Working out the other matrix elements (12 pathways for interchanging anti-parallel k and l, and 12 pathways for leaving anti-parallel k and l invariant),

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D.1 ¯Heff(4) to fourth order in t/U 207

i j

k l

Figure D.1: The processes of category (b) involve t2ijt2kl, connecting i to j and k to l.

i j k j i k

Figure D.2: The processes of category (c) are subdivided into two cases: the core hole site is connected to one other site (left), or the core hole site is connected to two other sites (right).

it turns out that all pathways interfere to give 0, just as in the half-filled case.

Therefore, H0is not modified by category (b) processes.

Processes in category (c) connect three sites i, j and k. They can be sub- divided into two cases: in the first one, the core hole site i is connected to one other site, and the second one, the core hole site i is connected to two other sites.

Starting with the first case, we have for the following matrix elements:

jk→↑jk and ↓jk→↓jk: H¯eff(4)= · · · − pipi t4 Uc3

 1

211 + 2SjzSkz



, (D.7)

jk→↑jk and ↓jk→↓jk: H¯eff(4)= · · · − pipi t4 Uc3

 1

211 − 2SjzSkz



, (D.8)

jk→↓jk and ↓jk→↑jk: H¯eff(4)= · · · + 0. (D.9) Adding these contributions and dropping the constants yields

eff(4)= · · · + 0. (D.10) The second case gives

jk→↑jk and ↓jk→↓jk: H¯eff(4)= · · · + pipi2t4 Uc3

 1

211 + 2SjzSkz



, (D.11)

jk→↑jk and ↓jk→↓jk: H¯eff(4)= · · · − pipi

 2t4

U Uc2 + 4t4 Uc2(2Uc+ U )

−2t4 Uc3

  1

211 − 2SjzSkz



, (D.12)

jk→↓jk and ↓jk→↑jk: H¯eff(4)= · · · + pipi

 2t4

U Uc2 + 4t4 Uc2(2Uc+ U )



× Sj+Sk+ SjSk+ . (D.13) Adding the contributions and dropping the constants yields

eff(4)= · · · + pipi

 4t4

U Uc2 + 8t4 Uc2(2Uc+ U )



Sj· Sk. (D.14)

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The corresponding part of H0(including the second neighbor terms from category (d))1is

H0= · · · +X

j6=k

4t2ijt2ik

U3 Sj· Sk (D.15)

and it is replaced by H¯eff(4)= H0+X

i

pipiX

j6=k

 4t4

U Uc2+ 8t4

Uc2(2Uc+ U )−4t4 U3



Sj· Sk+ . . . (D.16)

where the sum over j 6= k is over all pairs of neighbors j, k of i.

Finally, the processes of category (d) are

j di

kl

→ ↑j di

kl

+ flipped : H¯eff(4)= · · · − pipi2t4

Uc3

 1

411 + SjzSzk+ SkzSlz+ SjzSlz



, (D.17)

j di

kl

→ ↑j di

kl

+ flipped : H¯eff(4)= · · · + pipi 2t4

U Uc2

 1

411 − SjzSkz− SkzSlz+ SjzSzl



, (D.18)

j di

kl

→ ↓j di

kl

+ flip + j ↔ l : H¯eff(4)= · · · + pipi 2t4

U Uc2

 1

211 − 2SjzSlz



, (D.19)

j di

kl

→ ↑j di

kl

+ flip + j ↔ l : H¯eff(4)= · · · − pipi t4

Uc3 + t4 U Uc2



Sj+Sk+ SjSk+

+Sk+Sl+ SkSl+ , (D.20)

j di

kl → ↑j di

kl + flip + j ↔ l : H¯eff(4)= · · · − pipi t4

Uc3 + t4 U Uc2



Sj+Sl+ SjSl+ . (D.21)

where we have labeled the sites as shown in Fig. D.3, with dithe doubly occupied core hole site.

1We do this because, first, it simplifies notation: the second and third neighbor terms in the sum get the same prefactor. Second, Coldea also does this, and following him makes it easy to compare to his mean field result for the ring exchange terms.

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D.1 ¯Heff(4) to fourth order in t/U 209

i j

k l

Figure D.3: The processes of cat- egory (d) (tijtjktkltli) describe ring exchange.

Dropping constants, the final result for processes of category (d) is Heff(4)= · · · − X

i,squares at i

pipi

 2t4 U Uc2 +2t4

Uc3



(Sj· Sk+ Sk· Sl+ Sj· Sl) . (D.22)

The corresponding terms in H0 (minus the second neighbor terms, which were absorbed in the correction to H0due to category (c)) are

H0= · · · −8t4 U3

X

hi,ji

Si· Sj+80t4 U3

X

squares

[(Si· Sj)(Sk· Sl) + (Si· Sl)(Sj· Sk)

−(Si· Sk)(Sj· Sl)] . (D.23) The mean field result is easily obtained [82, 83]:

H0= · · · −48t4 U3

X

hi,ji

Si· Sj−20t4 U3

X

i,k

Si· Sk, (D.24)

where the sum over i, k is over all pairs of next nearest neighbors. Then, at the mean field, the intermediate state Hamiltonian for processes of category (d) becomes

eff(4) = H0+X

i

pipi X

squares at i

 24t4

U3 (Si· Sj+ Sj· Sk+ Sk· Sl+ Sl· Si) +20t4

U3 (Si· Sk+ Sj· Sl)

 2t4 U Uc2 +2t4

Uc3



(Sj· Sk+ Sk· Sl+ Sj· Sl)



+ . . . (D.25) Adding all contributions from all categories, we obtain

eff(4) = H0+X

i

pipi

 X

j

 16t4 U3 −4t2

U



Si· Sj+X

j6=k

4t4

U Uc2 + 8t4 Uc2(2Uc + U )

−4t4 U3



Sj· Sk+ X

squares

 24t4

U3 (Si· Sj+ Sj· Sk+ Sk· Sl+ Sl· Si) +20t4

U3 (Si· Sk+ Sj· Sl) −

 2t4 U Uc2 +2t4

Uc3



(Sj· Sk+ Sk· Sl +Sj· Sl)



. (D.26)

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