1 Nanoparticles as Nanoscale Resonators I
Consider a quantum emitter in proximity to a gold metal nanoparticle of radius 40 nm with dielectric constant N P =−5.9311 +i2.0970 surrounded by air (1 = 1). The wavelength of the emitted photons is 550 nm.
• Calculate the modification of the spontaneous emission rate for the quantum emitter as a function of distance from the nanoparticle and of the dipole orientation in the quasistatic approximation.
Parameters: a= 40 nm,m =N P,b = 1,λ= 550 nm The Purcell factor is given by the equation:
Γ
Γ0 =F (1)
Γ
Γ0 =ηa 9
16π4 ×(1−L)2
Vph2 (2)
Where, L = 1/3 (for a sphere), andVph = 4π3 aλ33 is the volume of the sphere in units of the cubic wavelength. The antenna efficiencyηa is given by
ηa= 1 1 +ωγ
p
3 4π2
√bL Vph
, (3)
where,b= 1 and m can be written as
m= 1− ωp2
ω(ω+iγ). (4)
Then
m−1 =− ω2p
ω(ω+iγ) =−ωp2(ω−iγ)
ω(ω2+γ2), (5) Re{m−1}=−ωp2
ω
ω
(ω2+γ2). (6)
Hence we can write that
Im{m−1}=− γ ωp2
ω(ω2+γ2). (7)
Thus we get
Im{m−1}
Re{m−1} =−γ
ω. (8)
Consider thatω is close to the resonance of the nano particle. Thus we have ω' ωp
√1 + 2b
= ωp
√3, (9)
Im{m−1}
Re{m−1} =−√ 3 γ
ωp
. (10)
Thus
γ
ω '=− 1
√3
Im{m−1}
Re{m−1} = 2.1
√3×6.93 '0.175. (11) Thus the Purcell factor can be written as
Γ Γ0
= 1
1 + 0.175(λa)3× √1
3
× 9 16π4
4 9
9 16π2
λ a
6
, (12)
Γ Γ0
' 1
1 + 0.175(λa)3 9 64π6
λ a
6
, (13)
where
1
1 + 0.175(λa)3 =ηa, (14) and λa = 550/40 '13.8. Thus we can write λa6
'6.9×106. Hence we can write the Purcell factor for a dipole in the field orientation:
Γ
Γ0 = 1
2.6×102 1.4×10−4×6.9×106'3.7 (15) If the dipole is not aligned along the field, there will be no field enhancement. In this case ΓΓ
0 <1.
• When a photon is emitted, estimate the probability that the photon is radiated to the far field (external quantum efficiency) as a function of distance from the nanoparticle and of the dipole orientation.
The longitudinal fieldE≈1/(kd)3 Γ
Γ0 ' |E|2, (16)
hence
Γ Γ0
' 1
(kd)6. (17)
At distances, where the effect drops by a factor of 10 we can write:
1
(ka)6 = 10 1
k6(a+d)6, (18)
wheredis the distance from the surface of the nano particle.
1
(a)6 = 10
(a+d)6 =⇒ 1 a =
√6
10
a+d (19)
√6
10 =a+d =⇒ d=a(6
√
10−1) =⇒ d'0.47×a= 18nm. (20) The antenna efficiency can be written as
ηa= Prad
(Prad+Pabs) = Prad Ptot = Γr
Γ , (21)
ηa= 1 1 +ωγ
p
√9
bLAR2 2(ka)3
. (22)
ηa' 1
1 + 0.1(λa)3 = 1
1 + 1.4 '40%. (23)
If you increase the distance, ηa increases and it reaches 100% at about kd = 1, where d≈ 2πλ '90 nm.
2 Nanoparticles as Nanoscale Resonators II
Figure 1: Interaction between Nanoparticle and an Emitter
(a) In the figure shown above, we have a nanoparticle located in the vicinity of a quantum emitter. That emitter’s dipole could be oriented horizontally or vertically.
The spontaneous emission rate of the emitter without the nanoparticleΓoand using the Purcell factor we can then calculate the modification of the spontaneous emission rate ΓΓ
o. As the dipole emits radiation in free space, it is associated with the electric field of the radiated emitted, and the relationship is as follows:
Γo ∼ωIm n
~ p·E~∗
o , whereE~∗ is the electric field of the dipole itself.
The field of the dipole in the presence of a nanoparticle would be otherwise if the nanoparticle does not exist. Such that the radiation emitted by the dipole propagates to the nanoparticle, a portion of it will be absorbed by the nanoparticle, but the other portion will be reflected back to the emitter (dipole).
Γ
Γo = 1 +6πo
k Im n
~ p·S·~p
o ,
where S represents the field emitted by the dipole, which goes to the nanoparticle and gets emitted back by the nanoparticle to the dipole.
The dipole field in presence of the nanoparticle, it corresponds to the Green’s tensor times the dipole.
G(0,0;ω) =Go(0,0, ω) +Go(0, d, ω)oα(ω)Go(d,0;ω),
whered is the distance separating the emitter apart of the nanoparticle, α(ω) is the polariz- ability of the nanoparticle, andGo(0,0, ω) is the free-space Green’s tensor.
S=GooαGo Go(R;ω) =
"
(1−RˆR) +ˆ i
kR(1−3 ˆRR) +ˆ 1
k2R2(1−3 ˆRR)ˆ
# eikR 4πRo
k ,
whereR=|r−r0 |is the difference between the distance vectors from the origin point to the source and the origin to the point of the field.
1=
1 0 0 0 1 0 0 0 1
and
RˆRˆ =
Rx
Ry Rz
Rx Ry Rz .
To calculate this as a function of the dipole orientation, let’s consider the orientation clarified below:
Figure 2: Parallel coupling vs. perpendicular coupling
The dipole is alongz-direction, therefore~p= (0,0,1). Now we want to calculate the distance either in case of parallel coupling or perpendicular coupling :
kcoupling : d= ˆzd=⇒Rˆ = (0,0,1)
⊥coupling: d= ˆxd=⇒Rˆ = (1,0,0) RˆRˆ =
0 0 1
0 0 1
=
0 0 0 0 0 0 0 0 1
:k
:
RˆRˆ=
1 0 0
1 0 0
=
1 0 0 0 0 0 0 0 0
:⊥
k:
1 0 0 0 1 0 0 0 0
+ i
kR − 1 k2R2
1 0 0 0 1 0 0 0 −2
Go(R)k
⊥:
0 0 0 0 1 0 0 0 1
+ i
kR − 1 k2R2
−2 0 0 0 1 0 0 0 1
Go(R)k
Now, we need to calculate the scalar productGo·~pand also ~p·Go , whereGo = 4πReikR
o.
~
p·Go= 0 0 1
1 0 0 0 1 0 0 0 0
+ i
kR − 1 k2R2
1 0 0 0 1 0 0 0 −2
Go(R)k fork.
~ p·Go =
(0,0,0) + i
kR − 1 k2R2
(0,0,−2)
Go(R)k:k
~ p·Go =
(0,0,1) + i
kR − 1 k2R2
(0,0,1)
Go(R)k:⊥
Go·~p=
0 0 0
+ i
kR − 1 k2R2
+
0 0
−2
Go(R)k:kGo·~p=
0 0 1
+ i
kR − 1 k2R2
+
0 0 1
Go(R)k:⊥
~
p·S·~p=~p·GooαGo.~p
This is what we want to calculate for parallel and perpendicular, so:
k:
i
kR − 1 k2R2
2
4Go(d,0)·Go(0, d)oα(ω)k2
⊥:
1 +
i
kR − 1 k2R2
2
1Go(d,0)·Go(0, d)oα(ω)k2 k:
i
kR − 1 k2R2
2
4 e2ikd 16π22d2
oαk2
⊥:
1 + i
kd− 1 k2d2
2
e2ikd 16π22d2
oαk2 Now we can plug it into expression of decay rate:
Γk
Γo = 1+6π k k2Im
( i
kR − 1 k2R2
2
e2ikd 4π2od2α
) ,Γ⊥
Γo = 1+6π k k2Im
( i
kR − 1 k2R2
2
e2ikd 16π2od2α
) .
After cancellation of similar terms, we can write the equations as the following:
Γk
Γo = 1+ 3 2πk3Im
( i
kR − 1 k2R2
2
e2ikd k2d2α
) Γ⊥
Γo = 1+ 3 8πk3Im
( 1 + i
kR − 1 k2R2
2
e2ikd k2d2α
)
Figure 3: Γ/Γo as a function of distance Forkd1(Far Field):
Γk
Γo '1 + 3 2πk3
−1 k4d4
Imn
αe2ikdo , Γ⊥
Γo '1 + 3 8πk3 1
k2d2Im n
αe2ikd o
.
Forkd1(Near Field):
Γk Γo
' 3 2πk3
1 k6d6
Im{α}, Γ⊥
Γo ' 3 8πk3
1 k2d2
Im{α}. The quantum efficiencyη is defined asη = Γ ΓR
R+ΓN R. We can either calculateΓRorΓN R, but it is easier to calculateΓN R, because it is the power absorbed by the nanoparticle.
Figure 4:Γ/Γo vs. kd.
ΓN R
Γo
=Power absorbed by the Nanoparticle Pabs ∼ωImn
~
pN P ·E~∗o ,
E~ =Go(0, d)·p~ Field radiated by the emitter
~
pN P =oα ~E,
Pabs =ωIm{oα} |Go(0, d)·~p|2, k:|Go(0, d)·~p|2=
i kd− 1
k2d2
2 1
4π22od2k2,
⊥:|Go(0, d)·~p|2=
1 + i kd− 1
k2d2
2 1
16π22od2k2.
ΓkN R Γo = 3k3
2π 1
k4d4 + 1 k6d6
Im{α},Γ⊥N R Γo = 3k3
8π 1
k4d4 + 1
k6d6 − 1 k2d2
Im{α}.
=⇒ ΓR= Γ−ΓN R
Forkd1 (Far-field): ΓN R '0 Forkd1 (Near-field): ΓN R' k61d6.
3 Nanoparticles as Nanoantennas
Modification of the radiation pattern by a metal nanoparticle, as indicated below:
The radiation pattern shown above will create superposition of both radiations at the far field.
Figure 5: Interaction between induced dipole and emitter’s dipole.
E(r,~ 0;ω)∼Go(~r,0;ω)·~p
~
pN P =oα ~E(d,~ 0;ω)
So, starting fromE(r,~ 0, ω), we calculate ~pN P, then the induced dipole - of the nanoparticle - radiates energy.
E~N P(~r) =Go(~r, ~d;ω)·~pN P, E(~~ r) =Go(~r,0;ω)·~p.
E~tot =E~N P +E ...this creates new radiation pattern~ E~N P(~r) =Go(~r, ~d;ω)oαGo(d,~ 0;ω)·~p,
E~tot 'h
Go(~r, ~d;ω)oαGo(d,~ 0;ω) +Go(~r,0;ω)i
·~p.
whereGo(~r, ~d;ω)oαGo(d,~ 0;ω)is for the nanoparticle, whileGo(~r,0;ω)for the free space with- out the nanoparticle.
In the Far-field: kr1
Go(~r,0;ω)'(1−RˆR)ˆ eikR 4πoRk, whereRˆ =
cosφsinθ sinφsinθ
cosθ
Emitter
Figure 6: Distance vectors.
Rˆ−dˆ= ˆR−zˆ fork,Rˆ−xˆ for⊥ Rˆ−dˆ=
cosφsinθ cosφsinθ cosθ−1
fork nanoparticle
=
cosφsinθ−1 cosφsinφ
cosθ
for⊥ eik|R−~ d|~
4πo |R~ −d~|' eik|R−~ d|~ 4πor
~
p is along z:
0 0 po
(1−RˆR)ˆ
0 0 1
=
RxRy
RyRz 1−R2z
=
cosφsinθcosθ sinφsinθcosθ
sin2θ
Go(d,0)·~p= i
kd− 1 k2d2
eikd 4πod
0 0
−2
pokk
Go(d,0)·~p=
1 + i kd− 1
k2d2
eikd 4πod
0 0 1
pok⊥ For the NP:
h1−( ˆR−d)( ˆˆ R−d)ˆi
0 0 1
or
0 0
−2
=
(Rx−dx)(Rz−dz) (Ry −dy)(Rz−dz) 1−(Rz−dz)(Rz−dz)
(1) or (−2)
=
cosφsinθ(cosθ−1) sinφsinθ(cosθ−1)
(−2)
(cosφsinθ−1) cosθ sinφsinθcosθ
E~tot =
cosφsinθcosθ sinφsinθcosθ
sin2θ
+
cosφsinθ(cosθ−1) sinφsinθ(cosθ−1)
1−(cosθ−1)2
oα(−2) i kd− 1
k2d2 eikd 4πod
eikr 4πr
E~tot =
cosφsinθcosθ sinφsinθcosθ
sin2θ
+
(cosφsinθ−1) cosθ sinφsinθcosθ
sin2θ
oα
1 + i kd− 1
k2d2
e2ikd 4π2od
eikr 4πr
Radiation Pattern:
P(Ω)r2dΩ =|Etransv |2 r2dΩ P(Ω) =r2 |Etransv |2
Ex,y,z −→Eθ, Eφ, where
|Etransv |2=|Eθ|2 +|Eφ|2