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Supplementary Information for manuscript titled "Spontaneous light emission from molecular junctions: Theoretical analysis of

up-conversion signal"

Hari Kumar Yadalam, Souvik Mitra, and Upendra Harbola

Department of Inorganic and Physical Chemistry, Indian Institute of Science, Bangalore, 560012 India

E-mail: [email protected] Phone: +91 (080)229 33410

The Liouville space algebraic expression for the current-induced fluorescence can be writ- ten down readily1 from the double-sided diagram shown in Fig. (1a). We get,

S(1)s) = 1

¯

h4ReX

|T|2 Z t

−∞

dτe−iωs(t−τ) Z τ

−∞

1 Z τ

−∞

2e¯hiα2−τ1)fα(α)hTˆµˆsR(t)ˆµsL(τ)ˆciL1)ˆciR2)i (1)

where the electron is created due to the interaction with αth lead. Note that the relative time-ordering in the first two operators at τ1 and τ2 is irrelevant as they act on different branches. It is straightforward to write down the corresponding Hilbert space expression.

After inserting the molecular many-body states and performing the time integrals, we obtain,

S(1)s) = γ

¯ h

X

X

a0e0

|T|2 |ha|ci|e0ihe0s|a0i|2fα(α)

[(¯hωs−Ee0a0)22][(α−¯hωs−Ea0a)2+ Γ2] (2)

1

(2)

whereΓ and γ are the life-times of the a→e0 and e0 →a0 excitations, and Ee0a0 =Ee0−Ea0 is the energy difference between the anionic excited and (lower energy) ground states, |e0i and |a0i, respectively, and the first Lorentzian with width γ in (2) is to make sure that the correct a0 and e0 states are picked up from the sum. This fact has been used above to replace Ee0a0 by¯hωs in the second Lorentzian. Sum over the lead states α can be converted to integration by introducing lead density of states ρα(α). Taking small temperature limit such that fα(α) = Θ(α−EF −eV) and performing the integral over the lead energies, α, we obtain the results given in Eq. (5).

Similarly, for the EL process depicted in Fig. (1b), we obtain the following expression in terms of the Liouville space correlation function.

S(2)s) = − 1

12¯h6ReX

ii0

X

αβ

|T|2|Ti0β|2 Z t

−∞

dτ Z τ

−∞

1 Z τ

−∞

2 Z τ2

−∞

3 Z τ1

−∞

4

es(τ−t)e¯hiα2−τ1)e¯hiβ4−τ3)fα(α)(1−fβ(β))hTˆµˆsR(t)ˆµsL(τ)ˆciR2)ˆciL1)ˆci0L4)ˆci0R(τ(3)3)i

where α 6= β. Again, it is straightforward to write down the corresponding Hilbert space expression and then inserting the molecular many-body states as depicted in the diagram and leads to

S(2)s) =− 1

12¯h5ReX

ii0

X

αβ

|T|2|Ti0β|2fα(α)(1−fβ(β))|ha|ci0|e00ihe00|ci|eihe|µs|ai|2δ(¯hωs−Eea)

Z 0

1 Z

0

2 Z

0

3 Z

0

4e¯hi(αβ−Eea)(τ1−τ2)e¯hi(β−Eae003−τ4) (4)

Straightforward integration over times and replacing sum over lead energies we obtain,

S(2)s) = γ 12¯h

X

ii0ee00

ραρβ|TTi0β|2 (¯hωs−Eea)22

Z d

Z d0

ha|ci0|e00ihe00|ci|eihe|µ|ai

(−0−hω¯ s−iΓae)(0+Ee00a−iΓe00a)

2

fα()(1−fβ(0)). (5)

In order to perform energy integrals, we assume small Γae limit and then taking small temperature limit, such that the Fermi functions become heavy-side function and µα = eV

2

(3)

and µβ = 0, we obtain the result given in Eq. (6).

Green function result

When the self-energy matrix, Γ, is not diagonal, that is, when the coherences between the molecular orbitals induced by the leads are not negligible, Green functions are not diagonal in the molecular orbital basis. For this case, GRL(ω) and GLR(ω) for a non-interacting system at steady-state and within the wide band approximation can be expressed in matrix form as,

GRL(ω) = −i X

α=L,R

[1−fα(ω)]Gr(ω)SαGa(ω) (6) GLR(ω) = i X

α=L,R

fα(ω)Gr(ω)SαGa(ω) (7)

where fα(ω) = eβ(ω−µα)+ 1−1

are the Fermi functions of the reservoirs and Sα is the self- energy matrix due to coupling to the αth lead. Gr/a(ω) are the retarded/advanced Green functions of the molecule under the influence of the leads given as,

Gr(ω) = Ga(ω)=

"

ωI −Hsys+ i 2

X

α=L,R

Sα

#−1

(8)

with Hsys

ijiδij and[Sα]ij = 2πραTT. Gr(ω)can be expressed in quasi-diagonal form using the right (|Rni) and the left (hLn|) eigenstates corresponding to the nth eigenvalue, γn, of the non-hermitian operatorHsys2i P

α=L,RSα. This gives, Gr(ω) =X

n

|RnihLn|

ω−γn . (9)

3

(4)

Substituting this in (6), we obtain,

GRL(ω) = −i X

α=L,R

X

mn

(1−fα(ω))|Rni hLn|Sα|Lmi

(ω−γn)(ω−γm)hRm| (10) GLR(ω) = i X

α=L,R

X

mn

fα(ω)|Rni hLn|Sα|Lmi

(ω−γn)(ω−γm)hRm| (11)

Using the above expressions for GLR(ω) and GRL(ω) in the equation for signal given in Eq. (11) and performing ω integral using Cauchy’s residue method2 gives,

S(ωs) = 2 π

X

α,β=L,R

nαβs)<

( X

n,m,k,l

"

hLn|Sα|LmihRm|RkihLk|Sβ|LlihRl|µ|Rni (ωsn−γk)

#

×

 Ψh

1

2 +iβ(γn−µα)i

−Ψ

1

2 +iβ(γn−µβs)

n−γm) (ωsn−γl) + Ψh

1

2 +iβ(γk−µα−ωs)i

−Ψ

1

2 +iβ(γk−µβ)

k−γl) (ωs−γkm)





 (12)

wherenαβs) = eβ(µα−µβhω)−1−1

is the Bose-Einstein distribution function, Ψ[Z] is the digamma function3 and [µ]ij = Θ[ij]Vij.

References References

(1) C. Marx, U. Harbola and S. Mukamel, Nonlinear optical spectroscopy of single, few, and many molecules: Nonequilibrium Green function QED approach, Phys. Rev. A77, 022110 (2008).

(2) J. E. Marsden and M. J. Hoffman, Basic Complex Analysis, 3rdEdition, W. H. Freeman Comp., New York (1999).

(3) Handbook of Mathematical Functions, Edited by M. Abramowitz and I. A. Stegun, Dover Publications, New York (1972).

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