Skip to main content
NCBI home page
Chemical Science logoLink to Chemical Science
. 2018 Jun 16;9(32):6659–6669. doi: 10.1039/c8sc00171e

Theory for polariton-assisted remote energy transfer†

Matthew Du a, Luis A Martínez-Martínez a, Raphael F Ribeiro a, Zixuan Hu b,c, Vinod M Menon d,e, Joel Yuen-Zhou a,✉
PMCID: PMC6115621  PMID: 30310599

graphic file with name c8sc00171e-ga.jpgA comprehensive theory is presented to mechanistically elucidate the long-range energy transfer between molecules strongly coupled to electromagnetic fields.

Abstract

Strong-coupling between light and matter produces hybridized states (polaritons) whose delocalization and electromagnetic character allow for novel modifications in spectroscopy and chemical reactivity of molecular systems. Recent experiments have demonstrated remarkable distance-independent long-range energy transfer between molecules strongly coupled to optical microcavity modes. To shed light on the mechanism of this phenomenon, we present the first comprehensive theory of polariton-assisted remote energy transfer (PARET) based on strong-coupling of donor and/or acceptor chromophores to surface plasmons. Application of our theory demonstrates that PARET up to a micron is indeed possible. In particular, we report two regimes for PARET: in one case, strong-coupling to a single type of chromophore leads to transfer mediated largely by surface plasmons while in the other case, strong-coupling to both types of chromophores creates energy transfer pathways mediated by vibrational relaxation. Importantly, we highlight conditions under which coherence enhances or deteriorates these processes. For instance, while exclusive strong-coupling to donors can enhance transfer to acceptors, the reverse turns out not to be true. However, strong-coupling to acceptors can shift energy levels in a way that transfer from acceptors to donors can occur, thus yielding a chromophore role-reversal or “carnival effect”. This theoretical study demonstrates the potential for confined electromagnetic fields to control and mediate PARET, thus opening doors to the design of remote mesoscale interactions between molecular systems.

1. Introduction

Enhancement of excitation energy transfer (EET) remains an exciting subfield of the chemical sciences. Although Förster resonance energy transfer1 (FRET) is one of the most extensively studied and well known forms of EET, its efficiency range is only at 1–10 nm.2 As such, exploration of EET schemes beyond that of a traditional pair of donor and acceptor molecules has been a highly active area of research. For instance, the theory of multichromophoric FRET3 has been applied to demonstrate the role of coherent exciton delocalization in photosynthetic light harvesting.4–8 This coherence, which is due to excitonic coupling between molecular emitters, has also been argued to increase EET in mesoscopic multichromophoric assemblies,9 with recent studies even reporting micron-sized transfer ranges in H-aggregates.10,11 Along similar lines, a well-studied process is plasmon-coupled resonance energy transfer,12 where molecules which are separated several tens to hundreds of nanometers apart can efficiently transfer energy between themselves due to the enhanced electromagnetic fields provided by the neighboring nanoparticles.13,14 Transfer between molecules across even longer distances can be mediated by the in-plane propagation of surface plasmons (SPs), with micron ranges reported in the literature15,16 (see ref. 17 for an example of micron-range EET via other types of electromagnetic modes). Notably, the plasmonic effects in these last examples occur in the so-called weak-coupling regime, where the frequency of energy exchange between excitons and plasmons is much slower than their respective decays.

An intriguing advancement in PARET has recently been reported by the Ebbesen group for cyanine dye J-aggregates strongly coupled to a microcavity mode.18 For spatially separated slabs of donor and acceptor dyes placed between two mirrors, it was found that increasing the interslab spacing from 10 to 75 nm led to no change in the relaxation rate between the hybrid light–matter states or polaritons, thus revealing a remarkable distance independence of the process. Importantly, such PARET phenomenon was already noted in an earlier work by the Lidzey group19 with a different cyanine-dye system, although the interslab spacing was not systematically varied there; similar work was also previously reported for hybridization of Frenkel and Wannier–Mott excitons in an optical microcavity.20 Motivated by these experiments, we hereby present a quantum-mechanical theory for polariton-assisted energy transfer which aims to characterize the various types of PARET afforded by these hybrid light–matter systems. To be concrete, we do so within a model where the “photonic modes” are SPs in a metal film and consider spatially separated slabs of donors and acceptor dyes which electrostatically couple to one another as well as to the SPs. We present a comprehensive formalism which encompasses the cases where either one or both types of chromophores are strongly coupled to the SPs. We apply our theory to a model system similar to those reported by the Ebbesen and Lidzey groups. Our work complements recent studies proposing schemes to enhance one-dimensional exciton conductance.21,22 In those studies, the delocalization afforded by strong-coupling (SC) is exploited to overcome static disorder within the molecular aggregate. Here, the emphasis is not on disorder (surmountable also by polaritonic topological protection23), but rather on PARET between two different types of chromophores, where energy harvested by one chromophore can be collected in another. This focus on long-range capabilities, as well as in-depth analyses of the rate contributions for the SC-induced states, provide fresh perspectives on PARET. In particular, we offer fascinating predictions for the experimentally unexplored scenario of “photonic modes” strongly coupled to one of donors or acceptors (the latter case was first theoretically investigated for the chromophores in a microcavity24).

As a preview, we highlight the structure and the main conclusions of this work (the latter are summarized in Table 1). We begin by introducing the general Hamiltonian for spatially separated slabs of donors and acceptor chromophores in Section 2. EET rates for a single or both types of chromophores strongly coupled to SPs are presented in Sections 2.1 and 2.2, respectively. In the former case, the rates are “FRET-like”1 and shown to be dependent on spectral overlap (of absorption and emission lineshapes).25,26 For SC to donors, EET can be tuned for enhancement or suppression. This result is in stark contrast with that of acceptors-SPs SC where, surprisingly, EET to acceptor polariton states vanishes for large-enough samples. For the case when both chromophores strongly interact with SPs, transfer is instead mediated by vibrational relaxation in analogy with the theories of Davydov27,28 and Redfield.25,26,29 Nevertheless, PARET is still achieved. In Section 3, we apply the formalism to study a model system resembling cyanine dye J-aggregates. Our numerical simulations demonstrate that applying SC exclusively to donors enables PARET up to 1 micron. We also show that sufficiently intense SC to acceptors induces a “carnival effect” that reverses the role of the donor and acceptor. Lastly, when both chromophores are strongly coupled to SPs, we obtain sizable PARET rates at chromophoric separations over hundreds of nanometers which are in good agreement with experiments.

Table 1. Comparison of different cases of PARET arising from SC to donors and/or acceptors.

SC to Features
Donors only • PARET from donor polariton states; dominated by PRET contribution
• Rate of EET from donor dark states ≈ bare (i.e., no SPs) FRET rate
• “Förster regime” of PARET
Acceptors only • Low EET to acceptor polariton states due to their low density of states (compared to dark states) and delocalized character
• Rate of EET to acceptor dark states ≈ bare FRET rate
• “Carnival effect”: acceptor and donor reverse roles
• “Förster regime” of PARET
Donors and acceptors • Polariton states are delocalized across donors and acceptors
• Rate of PARET from polariton to dark states ≫ rate of PARET from dark/polariton to polariton states due to relative density of final states; dark-state manifolds are dense and act as traps
• PARET mediated by vibrational relaxation
• “Davydov/Redfield regime” of PARET
Open in a new tab

2. Theory

We begin by describing the polaritonic (plexcitonic) setup that we theoretically investigate. Let the chromophore slabs lie above (z > 0) and parallel to the metal film (z < 0) that sustains SP modes (example schematic diagrams are given in Fig. 1a, 2a, 3a, and 4a). We assume the metal film and the slabs are extended along the xy (longitudinal) plane. The slabs of C = D, A (donor, acceptor) chromophores consist of Nxy,C, Nz,C, and NC = Nxy,CNz,C molecules in the xy-plane, z-direction, and total, respectively. An effective Hamiltonian for this setup can be constructed as,

H = HD + HA + HP + HDA + HDP + HAP. 1

The term HC = H(sys)C + H(B)C + H(sys–B)C is the Hamiltonian for the slab with the C chromophores, where (denoting ℏ as the reduced Planck constant)

2. 2a
2. 2b
2. 2c

represent the system (excitonic), bath (phononic), and system–bath-coupling contributions, respectively. The label Cij refers to a C exciton located at the (i,j)-th molecule of the corresponding slab [(i,j) indexes an (xy,z) coordinate]. We take every Cij exciton to have energy ℏωC and neglect inter-site coupling since the latter provides an insignificant contribution to polariton dispersion when compared to the SP dispersion. Specifically, within the wavevector range of interest, inter-site coupling only induces a constant energy shift (which we assume to be included in ωC) to the exciton subsystem. Thus, the exciton dispersion is only relevant at much shorter wavelengths. Inline graphic labels the creation (annihilation) of a phonon of energy ℏωq,C at the q-th vibrational mode of the (i,j)-th molecule in the C slab. Given the molecular character of the problem, vibronic coupling is assumed to be local30 (in contrast to that for relatively ordered materials such as crystals31): exciton Cij couples linearly to Inline graphic and bq,Cij but not to modes in other molecules;32 these couplings are characterized by Huang–Rhys factors λq,C2.33 The SP Hamiltonian HP = H(sys)P + H(B)P + H(sys–B)P has similar form:34,35

2. 3a
2. 3b
2. 3c

where Inline graphic labels the creation (annihilation) of an SP of energy ℏωk[combining right harpoon above] and in-plane wavevector k[combining right harpoon above]. Bath modes indexed by q,P with corresponding operator Inline graphic and energy ℏωq,P are coupled to each SP mode k[combining right harpoon above] with strength gq,k[combining right harpoon above]. Specifically, these SP interactions occur with either electromagnetic or phonon modes and represent radiative and ohmic losses, respectively.35 The remaining rightmost terms in eqn (1) represent the dipole–dipole interactions amongst donors, acceptors, and SP modes. The HDA term is given by the electrostatic (near-field) dipole–dipole interactions between donors and acceptors,

2. 4

where μC = |μ⃑Cij| for transition dipole moment (TDM) μ⃑Cij corresponding to Cij, rijlm is the distance between Dji and Alm, and κijlm = μ̂Dij·μ̂Alm – 3(μ̂Dij·r[combining circumflex]ijlm)(μ̂Alm·r[combining circumflex]ijlm) is the orientational dependence of the interaction (we denote v[combining circumflex] as the unit vector corresponding to v[combining right harpoon above]). We have ignored the corrections to κijlm due to reflected waves from the metal—despite their prominent effects in phenomena such as photoluminescence36—since they are numerically involved and do not significantly change the order of magnitude of the bare dipole–dipole interaction;37 furthermore their expected effects in HDA will be overwhelmed by HCP, as we shall explain in Sections 2.1 and 3. For simplicity, we take the permittivity on top of the metal to be a real-valued positive dielectric constant εd. The light–matter interaction for species C in the rotating-wave approximation38 is also dipolar in nature and is described by39

2. 5

where (R[combining right harpoon above]i,C,zj,C) are the position coordinates of Cij and |G and |G〉 is the electronic ground state ( is the electronic ground state (i.e., with no excitons). Just like in HDA, the interaction between an SP mode and a chromophore (indexed by k[combining right harpoon above] and Cij, respectively) has an orientation-dependent parameter Inline graphic, where Inline graphic is the real-valued evanescent SP decay constant for the region above the metal. The light–matter coupling also includes the quantization length Lk[combining right harpoon above] (ref. 40) and area S of the SP. We refer the reader to ESI Section S1† for further details of these terms.

Fig. 1. (a) Schematic energy-level diagram showing the EET transitions from donors strongly coupled to SPs to bare acceptors. The thickness of the horizontal lines denotes the density of states while the thickness of arrows corresponds to rate of transition (thicknesses not drawn to scale). Inset: representation of the EET process from a thick and dense slab of donors (featuring SC to SPs) to a dilute monolayer of acceptors. (b) Rates as a function of donor–acceptor separation Δz for EET from donor polariton and dark states to acceptors (lines). The rate from dark states and for the bare-donor FRET (dots), are calculated in the same manner. (c) Contributions of rates for transfer from donor UP and LP to acceptor states due to donor–acceptor (FRET) and SP–acceptor (PRET) interactions (see eqn (12a) and immediately preceding discussion).

Fig. 1

Open in a new tab

Fig. 2. (a) Schematic energy-level diagram showing the EET transitions from bare donors to acceptors strongly coupled to SPs. The thickness of the horizontal lines denotes the density of states while the thickness of arrows corresponds to rate of transition (thicknesses not drawn to scale). Inset: representation of the EET process from a dilute monolayer of donors to a thick and dense slab of acceptors (featuring SC to SPs). (b) Rates as a function of donor–acceptor separation Δz for energy transfer from donors to acceptor polaritons and dark states (lines). The rate to dark states and for bare-acceptor FRET (dots), are calculated in the same manner.

Fig. 2

Open in a new tab

Fig. 3. (a) Schematic energy-level diagram showing the “carnival-effect”-EET role-reversal process from acceptor UP state to bare donors. Insets: (top) cartoon illustrating the “carnival effect” between donors and acceptors and (bottom) representation of the reversed-role EET process from a thick and dense slab of acceptors (featuring SC to SPs) to a dilute monolayer of donors. (b) Rate as a function of donor–acceptor separation Δz for energy transfer from acceptor UP to bare donors.

Fig. 3

Open in a new tab

Fig. 4. (a) Schematic energy-level diagram showing the EET transitions among polariton and dark states for both donors and acceptors strongly coupled to SPs. The SP mode is resonant with the donor transition (for polariton as initial state); the donor slab lies 1 nm above the metal and has fixed position (z > 0) while the acceptor slab is moved in the +z-direction to vary the donor–acceptor separation Δz. The thickness of the horizontal lines denotes the density of states while the thickness of arrows corresponds to rate of transition (thicknesses not drawn to scale). Insets: (top) cartoon illustrating vibrational relaxation, the EET mechanism for this case of SC, and (bottom) representation of the setup of thick and dense slabs for both types of chromophores (featuring SC to SPs) for both types of chromophores. (b) Rates for selected downhill transitions as a function of Δz.

Fig. 4

Open in a new tab

The general Hamiltonian in eqn (1) describes a complex many-body problem consisting of excitons, SPs, and vibrations, all coupled with each other. To obtain physical insight on the opportunities afforded by this physical setup, we consider in the next sections two limit cases where either one or both types of chromophores are strongly coupled to the SP. The study of these two situations already provides considerable perspective on the wealth of novel EET phenomena hosted by this polaritonic system.

2.1. Case (i): SC to only one chromophore C

We consider the case where one of the chromophores C (D or A) is strongly coupled to an SP but the other, C′, is not. This can happen when the concentration or thickness of the C slab is sufficiently high and that of the C′ slab low. Under these circumstances, we write eqn (1) as H = H(i)0 + V(i), where we define the zeroth-order Hamiltonian as H(i)0 = H(i)sys + HB + Hsys–B. The system, bath, and their coupling are respectively characterized by H(i)sys = H(sys)D + H(sys)A + H(sys)P + HCP, HB = H(B)D + H(B)A + H(B)P, and Hsys–B = H(sys–B)D + H(sys–B)A + H(sys–B)P. The perturbation describing the weak interaction between chromophore C′ and the SC species is V(i) = HDA + HC′P, i.e., the electrostatic interaction as in Förster1 theory.25,26 To diagonalize H(i)sys, we introduce a collective exciton basis comprised of bright C states with in-plane momenta matching those of the SP modes and ignore the very off-resonant SP–exciton couplings beyond the first Brillouin zone (FBZ) of the molecular system:39,41 Inline graphic where

2.1. 6a
2.1. 6b

For each k[combining right harpoon above]-mode in the FBZ, there is only one “bright” collective exciton state Inline graphic that couples to the k[combining right harpoon above]-th SP mode Inline graphic, where Inline graphic. In addition to the weakly coupled C′ states, H(i)sys has two polariton eigenstates Inline graphic for α = UP, LP (upper polariton and lower polariton, respectively), which are also eigenstates of H(k[combining right harpoon above])bright,C for each k[combining right harpoon above] ∈ FBZ; throughout this work, cmn = = 〈m|n〉. Furthermore, there is a large reservoir of . Furthermore, there is a large reservoir of NC – Nxy,C = Nxy,C(Nz,C – 1) “dark” (purely excitonic) eigenstates |dC,k[combining right harpoon above]〉 ( (d = 0, 1,…, Nz,C – 2) which are also eigenstates of Hdark,C with bare chromophore energy ℏωC.

EET rates between C and uncoupled C′ states can be derived by applying Fermi's golden rule; the corresponding perturbation V(i) connects vibronic-polariton eigenstates of H(i)0 as in FRET and MC-FRET theories.3,42–44 For simplicity, we also invoke weak system-bath coupling Hsys–B, from which the following expression can be obtained,45,46

2.1. 7

This is the rate of transfer between H(i)sys eigenstates |I eigenstates |I〉 and |F〉, where and |F eigenstates |I〉 and |F〉, where , where JF,I is the spectral overlap between absorption and emission spectra, which depend on HB and Hsys–B (see Section S2.1† for derivation of γF←I and expression for JF,I). Since our focus is to understand the general timescales expected for the PARET problem, in Section 3 we treat the broadening of electronic/polaritonic levels due to Hsys–B as Lorentzian, although more sophisticated lineshape theories can be utilized if needed.33 Furthermore, we can in principle also refine eqn (7) to consider the complexities of vibronic mixing between the various eigenstates of H(i)sys, as done in recent works by Jang and Cao.3,42–44

It follows from eqn (7) that the rates from donor states—either polaritons with given wavevector k[combining right harpoon above] or a uniform mixture of dark states with occupation Inline graphic for all d,k[combining right harpoon above]—to the incoherent set of all bare acceptor states are,

2.1. 8a
2.1. 8b

Here, we notice that Inline graphic in eqn (8a) can be enhanced or suppressed relative to bare (in the absence of metal) FRET due to additional SP-resonance energy transfer47 (PRET) channel given by HAP, as well as the spectral overlap Inline graphic that can be modified by tuning the energy of |αD,k[combining right harpoon above]〉. Similar findings were obtained for electron transfer with only donors strongly coupled to a cavity mode.. Similar findings were obtained for electron transfer with only donors strongly coupled to a cavity mode.48 Given that |αD,k[combining right harpoon above]〉 corresponds to a delocalized state, one would expect a superradiant enhancement of the rate; corresponds to a delocalized state, one would expect a superradiant enhancement of the rate;5,6 in practice, this effect is minor due to the distance dependence of HDA (see Section S2.3†). On the other hand, eqn (8b) presents an average rate γA←darkD from the dark states and hence does not feature a PRET term. In fact, it converges (see Section S2.5†) to the bare FRET rate (eqn (12b) below) in the limit of large ND≫Nxy,D (when there are many layers of chromophores along z) and isotropically averaged and orientationally uncorrelated TDMs μ⃑Cij for both C = D, A.

In contrast, strongly coupling the acceptor states to SPs yields the following rates:

2.1. 9a
2.1. 9b

Here, we have calculated average rates over the ND possible initial states at the D slab and summed over all final states for each polariton/dark band. Given the asymmetry of Fermi's golden rule with respect to initial and final states (rates scale with the probabilities of occupation of initial states and with the density of final states),5 the physical consequences of eqn (9) are quite different to those of its counterpart in eqn (8) when NA ≫ Nxy,A and all TDMs are isotropically averaged and feature no orientational correlations amongst them. Seemingly counterintuitive in light of the various recently reported phenomena which are enhanced upon exciton delocalization,57 the rate of EET to polariton states is reduced substantially compared to the bare FRET rate (at short donor–acceptor separations; see Section S2.7 for a formal derivation of this statement).49 Nevertheless, this statement is easily understood from a final-density-of-states argument (see eqn (9a)): only Nxy,A bright acceptor collective modes contribute to Inline graphic, whereas NA localized acceptor states contribute to the bare FRET rate. On the other hand, γdarkA←D behaves similarly to eqn (8b) in that it converges (see eqn (13b) and (S30b)†) to the bare FRET rate. Thus, at donor–acceptor separations where the square of the FRET coupling exceeds on average that for PRET, the inequality γαA←D≪γdarkA←D is expected to hold.

Our analyses of eqn (8) and (9) reveal one of the main conclusions of this letter: while strongly coupling to D but not to A might yield a significant D → A EET rate change with respect to the bare case, strongly coupling to A but not to D will change that process in a negligible manner. Interestingly, these trends have also been observed for transfer between layers of donor and acceptor quantum dots selectively coupled to metal nanoparticles in the weak-interaction regime.50 However, polariton formation with A is not useless, for one may consider the intriguing prospect of converting A states into new donors. As we shall show in the next paragraphs, this role reversal or “carnival effect” can be achieved when the UP is higher in energy than the bare donor states. These findings are quite general and should apply to other molecular processes as long as the interactions between reactants and products (taking the roles of donors and acceptors) also decay at large distances, a scenario that is chemically ubiquitous.51

2.2. Case (ii): SC to both donor and acceptor chromophores

We next consider the SC of SPs to both donors and acceptors. We rewrite eqn (1) as H = H(ii)0 + V(ii), where H(ii)0 = H(ii)sys + HB and the perturbation is V(ii) = Hsys–B for interslab distance large enough to neglect interaction HDA in V(ii). Here, H(ii)sys = H(sys)D + H(sys)A + HDP + HAP + HDA + HP is the polariton Hamiltonian. As in the Davydov model,27,28 the EET pathways of interest become those where Hsys–B induces vibrationally mediated relaxation (faster than dipole–dipole coupling in typical organic chromophores separated by 1–10 nm (ref. 2)) among the delocalized states resulting from SC.25,26 The transfer rates describing these processes can be deduced by Fermi's golden rule too, the resulting expressions coinciding with those derived with Redfield29 theory.25,26,52 Although not necessary, we take Nxy,D = Nxy,A = Nxy to avoid mathematical technicalities about working with two k[combining right harpoon above] grids of different sizes, a complication that does not give more insight into the physics of interest. As done in Section 2.1, we rewrite H(ii)sys in k[combining right harpoon above]-space: Inline graphic, where

2.2. 10

and the terms labeled dark are defined analogously to those in eqn (6b). For each k[combining right harpoon above] ∈ FBZ, there are three polariton eigenstates of H(k[combining right harpoon above])bright that are linear combinations of |Dk[combining right harpoon above]〉, |A, |Ak[combining right harpoon above]〉, and |, and |k[combining right harpoon above]〉, and we call them UP, middle polariton (MP), and LP, according to their energy ordering. In addition, the presence of , and we call them UP, middle polariton (MP), and LP, according to their energy ordering. In addition, the presence of Hdark,C yields NC – Nxy,C dark C eigenstates.

The resulting expressions for the rates of transfer from a single polariton state or average dark state to an entire polariton or dark state bands are

2.2. 11a
2.2. 11b
2.2. 11c

for α, β = UP, MP, LP and C = D, A (see Section S3.1† for derivation of eqn (11)). To intuitively understand eqn (11a), note that Inline graphic and Inline graphic are the fractions of exciton |Cij〉 in the polariton states |α in the polariton states |αk[combining right harpoon above]〉 and and Inline graphic, respectively, while Inline graphic is the single-molecule rate of vibrational relaxation at the energy difference Inline graphic. More specifically, Inline graphic, where Θ(ω) is the Heaviside step function, Inline graphic is the Bose–Einstein distribution function (kB is the Boltzmann constant and T is temperature) for zero chemical potential μ = 0, and Inline graphic is the spectral density for chromophore C.52 Hence, one can interpret β ← αk[combining right harpoon above] as a sum of incoherent processes (over C and i,j) where the (local) vibrational modes in Cij absorb or emit phonons concomitantly inducing population transfer between the various eigenstates of H(ii)sys. Eqn (11b) and (11c) can be interpreted in a similar light. As an aside, we note that these transitions are analogous to the so-called intraband relaxation among collective exciton states in J-aggregates.53 We now comment on some important qualitative trends in these rates while for simplicity assuming that Nz,D = Nz,A = Nz. First, EET from polariton or dark states to a polariton band (eqn (11a) and (11b)) scale as Inline graphic. To see this, note that both Inline graphic and Inline graphic are O(1), while Inline graphic and Inline graphic are Inline graphic, but the summations Inline graphic and Inline graphic are respectively carried over Nxy and NxyNz terms. On the other hand, Inline graphic takes values that are on the order of the single-molecule decay Inline graphic. For sufficiently large Nz, these scalings are consistent with previous studies on relaxation dynamics of polaritons54–56 and can be summarized as follows: the dominant channels of relaxation are from the polariton states to a reservoir of dark states that share the same exciton character; their timescales are comparable to those of the corresponding single-chromophore vibrational relaxation; given the large density of states in this reservoir compared to the polariton bands, the dark states act as a population sink or trap from which population can only leak out very slowly.56,57

3. Application of the theory

The theory above is now applied to study EET kinetics associated with slabs of chromophores with ℏωD = 2.1 eV, ℏωA = 1.88 eV; these transition energies are chosen to match those of the J-aggregated cyanine dyes (TDBC and BRK5714, respectively) used in previous polariton experiments.18,58 For simplicity, this section assumes T = 0 and thus only considers downhill transfers to/from polariton and dark states. We describe the metal with Drude permittivity of silver (ωP = 9.0 eV, ε∞ = 1;59 see Section S1†) and all media at z > 0 (including molecular slabs) with εd = 1. We model spectral overlaps (eqn (8) and (9)) with Lorentzian functions Inline graphic whose parameters are estimated as in Section S2.2;† we set ΓA ≈ ΓD = 47 meV to represent observed values for absorption of TDBC60 and Inline graphic,39 where vg(k[combining right harpoon above]) is the SP group velocity. Rigorous treatments of lineshape functions have been previously reported in MC-FRET literature and could be applied to this problem as well,43,44,61,62 although this effort is beyond the scope of our work. We also neglect differences in TDMs and assign μD = μA = 10 D, a typical number for cyanine dyes.63

We now proceed to simulations for Case (i), where only one of the molecular species forms polaritons. For simplicity, we assume isotropically oriented and spatially uncorrelated dipoles, upon which we find the interesting observation that the transfer rates in eqn (8) can be approximately decomposed into incoherent sums of FRET and PRET rates (see Sections S2.4 and S2.5† for more explicit expressions, derivations, and justification of validity),

3. 12a
3. 12b

where, as explained above, only Inline graphic differs from γbare FRET. More concretely, we consider a 35 nm-thick slab of donors with 1 × 109 molecules per μm3 on top of a 1 nm spacer placed on a plasmonic metal film. We set the monolayer slab of acceptors with 1 × 104 molecules per μm2 at varying distances from the donors (Fig. 1a). Then the collective couplings of the donor-resonant SP mode (|k[combining right harpoon above]| = 1.1 × 107 m–1) to donors and acceptors is gD(k[combining right harpoon above]) = 155 meV and gA(k[combining right harpoon above]) ≤ 2.5 meV, respectively. When there is no separation between donor and acceptor slabs, rates >1 ns–1 (Fig. 1b) are obtained for transfer to acceptors from the UP (∼10 ns–1), LP (∼100 ns–1), or the set of dark states (∼10 ns–1). As separation increases however, the rate from dark states decays much faster than those from either UP or LP. This difference stems from the slowly decaying PRET contribution of the polaritons, as well as the totally excitonic character of the dark states, which can only undergo FRET but not PRET (Fig. 1a and b). In fact, for large distances, the FRET contribution becomes significantly overwhelmed by PRET (Fig. 1c), in consistency with previous studies in the weak SP-coupling regime.64 As the distance between slabs approaches 1 μm, it is fascinating that while transfer from dark states (and thus bare FRET) practically vanishes, the rate from either LP (∼1 ns–1) or UP (∼0.01 ns–1) is still at or above typical fluorescence decay rates (0.01–10 ns–1).65 Roughly speaking (in FRET language), this PARET has a Förster distance in the μm range, or 1000-fold greater than the typical nm-range.66 Interestingly, the LP rate exceeds the UP one by 1–2 orders of magnitude at all separations due to greater spectral overlap with the acceptor (Fig. 1a and S1†).

In contrast, strongly coupling the acceptors to a resonant SP mode does not lead to the aforementioned PARET from donors to acceptors (Fig. 2). Making the same assumptions as above, i.e., taking isotropically oriented and spatially uncorrelated dipoles, we obtain (Section S2.7†),

3. 13a
3. 13b

We consider (Fig. 2a) a 50 nm-thick acceptor slab with a concentration of 1 × 109 molecules per μm3 on top of the 1 nm spacer placed on the metal, and a monolayer of donors with concentration 1 × 104 molecules per μm2 at varying distances from the acceptors. Notice that γdarkA←D becomes another bare FRET rate like in eqn (12b). For γαA←D, we see that PRET still dominates over FRET for long distances (Fig. S2†). However, due to the suppression of γαA←D relative to γdarkA←D explained in Section 2.1, the limited spatial range of interactions of HDA and HDP, and the fact that the donor energy is lower than that of |UPA,k[combining right harpoon above]〉 for most for most k[combining right harpoon above] ∈ FBZ (Fig. S3†), the rates to the acceptor UP band fall below fluorescence timescales65 and therefore offer no meaningful enhancements with respect to the bare FRET case (Fig. 2b). While the first two reasons also explain the similarly low rates to the LP band, the major factor is that most states |LPA,k[combining right harpoon above]〉 essentially overlap only with acceptors that are closer to the metal—and thus farther from the donors—due to the evanescent nature of the SP–exciton coupling ( essentially overlap only with acceptors that are closer to the metal—and thus farther from the donors—due to the evanescent nature of the SP–exciton coupling (eqn (5)).

Coupling SPs to acceptors need not, however, be a disappointment. Increasing the acceptor slab thickness to 140 nm affords for the acceptor-resonant SP mode (|k[combining right harpoon above]| = 9.8 × 106 m–1) the collective coupling gA(k[combining right harpoon above]) = 237 meV while keeping gD(k[combining right harpoon above]) = 1.7 meV. Consequently, the acceptor UP energy Inline graphic is lifted higher than ℏωD (Fig. 3a and S4†), thus allowing for the carnival effect where the donors and acceptors reverse roles. Due to sufficient spectral overlap between the acceptor UP and donor states (Fig. 3a and S4†), transfer from UP occurs at ∼100 ns–1 for donor–acceptor separation of 1 nm and drops only to ∼1 ns–1 when this separation approaches 1 μm (Fig. 3b). On the other hand, neither the acceptor dark nor LP states contribute to this reversed PARET given their lack of spectral overlap with the donors and detailed balance (especially at T = 0). This result provides the second main conclusion of our work: polaritons offer great versatility to control spectral overlaps without actual chemical modifications to the molecules and can therefore endow them with new physical properties. Before proceeding to simulations for Case (ii), it should first be noted that while our model neglects intermediate- and far-field donor–acceptor dipole–dipole interactions that become relevant at ∼μm distances, these couplings are expected to be small compared to PRET couplings and therefore should not qualitatively change our results for Case (i). The relative insignificance of the far-field, or radiative, contributions is consistent with their correspondence to emission followed by absorption (of a real photon).67 Regardless, these additional interactions can be modeled using a quantum electrodynamics treatment68 of energy transfer in bulk media according to previous literature.69 Second, we highlight that the PARET from polariton states for the donors-only and reversed cases of SC may not be efficient in experiments due to its competition with vibrational relaxation from UP to dark states (∼10–100 fs for exciton-microcavity systems54,70–73) and/or radiative decay (dominated by fast cavity leakage ∼10–100 fs for both microcavities72–74 and SPs75,76). However, conditions may be optimized to suppress these deleterious pathways by detuning the SP energy relative to that of the strongly coupled chromophore such that the polariton state is mostly excitonic and has an enhanced lifetime.77

Finally, when both chromophores are strongly coupled to SPs, we limit ourselves to donor–acceptor separations >10 nm to ignore HDA terms (an approximation discussed in Section 2.2 and validated by the calculations above demonstrating that FRET coupling is significantly diminished at such distances). The thickness (35 nm) and density (1 × 109 molecules per μm3) of each slab is large enough to allow for SC of the donor-resonant SP mode (|k[combining right harpoon above]|=1.1 × 107 m–1, gD (k[combining right harpoon above]) = 155 meV, and gA(k[combining right harpoon above]) = 142 meV) to both chromophores separated up to ∼400 nm (Fig. S6b†). To evaluate the rates derived (Section S3.2†) from eqn (11) under the condition NC ≫ Nxy,C for C = D, A, we introduce a spectral density representing intramolecular exciton–phonon coupling of TDBC: Inline graphic, where

3. 14

Γ = 47 meV is equal to the chromophore decay energy, and BTDBC is the discrete set (Section S3.2†) of localized vibrational modes which significantly couple to each TDBC exciton. Such coupling has been experimentally70–73,78 and theoretically54,55,79–81 supported as the mechanism of vibrational relaxation for the dye; our spectral density has been reconstructed from the works of Agranovich and coworkers.54,55 By placing the donor slab on top of the spacer on the metal and varying the acceptor position above the donors (Fig. 4a), we find that for all donor–acceptor separations, the rates of PARET from UP to dark donors (∼105 ns–1) and MP to dark acceptors (∼104–105 ns–1) are substantially higher compared to those from dark donors to MP (∼103 ns–1) and dark acceptors to LP (∼103 ns–1) (Fig. 4b). These observations are in agreement with our discussion above, where the dark state manifolds act as population sinks due to their high density of states. Indeed, we also notice that the rates for UP → darkD and MP → darkA are enhanced (Fig. 4b) compared to those of UP → MP and MP → LP, respectively, by approximately Nz = 35, the analytically estimated ratio solely based on the associated density of final states. Another interesting detail seen from Fig. 4b is that the UP → MP (MP → LP) rate with respect to the interslab distance Δz is essentially parallel to that of UP → darkD (MP → darkA). This is a consequence of the MP (LP) essentially having donor (acceptor) energy and character for most points in the FBZ (see dispersion curve, Fig. S6†). The UP → darkA and UP → LP processes behave similarly (Fig. S5†).

These calculated rates establish consistency with a number of recent notable experiments. First, our results corroborate the experimental observation of efficient PARET for separated donor and acceptor slabs of cyanine dyes strongly coupled to a microcavity.18,19 While our SP model for the SC of both excitons cannot account for the exact distance-independent PARET18 between donor and acceptor slabs in a microcavity, the rates are essentially constant over hundreds of nanometers due to the slowly decaying SP fields. Additional validation of our theory is obtained by defining rate parameters Inline graphic (functions of the γ rates above, see Sections S3.3 and S3.4†) that can be directly compared to those experimentally reported (Table 2).19 Since experimental Inline graphic have not been determined for the setup of our work, we instead use those describing a blend of two cyanine dyes where physical separation of the dyes did not significantly change the observed photoluminescence.19 In our work, we obtained rates that assume zero temperature and sum across the whole polariton band in the FBZ; in practice, experiments occur at room temperature and probe polariton photoluminescence around a narrow window of wavevectors close to the anticrossings (∼107 m–1 in (ref. 82)). If we take these experimental details into account when calculating Inline graphic, we notice good agreements with our theory (see Table 2). As an aside, we reiterate that there are other experimental subtleties, notably competing processes such as radiative decay, that we have not considered but may compromise the longevity of the polariton states and thereby influence the observation of the EET phenomena predicted throughout this work for the two cases of SC.

Table 2. Comparison between PARET rate parameters Inline graphic for donor and acceptor cyanine dye J-aggregates strongly coupled to SP (theory) and microcavity (experiment) modes a .

graphic file with name c8sc00171e-t66.jpg SP (theory) b Microcavity (experiment) c
graphic file with name c8sc00171e-t67.jpg (2.9–3.2 fs)–1 (34 fs)–1
graphic file with name c8sc00171e-t68.jpg (177–259 ps)–1 (603 ps)–1
graphic file with name c8sc00171e-t69.jpg (6.9–12 fs)–1 (8.5 fs)–1
graphic file with name c8sc00171e-t70.jpg (178–243 ps)–1 (228 ps)–1
Open in a new tab

aSee Sections S3.3 and S3.4 for additional details.

bRanges of the rate parameters calculated from eqn (S45), plotted in Fig. S7, and accounting for the facts that typical polariton photoluminescence experiments occur at room temperature and probe only final polariton states near the anticrossings.82

cRate parameters that were obtained from experimental fitting of a kinetic model and that describe the PARET processes for a blend of J-aggregating NK-2707 (donors) and TDBC (acceptors) cyanine dyes both strongly coupled to a microcavity mode.19

Given the significant differences between the microcavity-83,84 and SP-based85 systems, let alone experimental uncertainty, the accordance between our theory and the aforementioned experiments highlights the remarkable robustness of cavity SC of donor and acceptor excitons as a method for PARET. Moreover, we have arrived at the third main conclusion of this paper: when donor and acceptors are both strongly coupled to a photonic mode, efficient energy exchange over hundreds of nm can occur via vibrational relaxation; more generally, local vibrational couplings can induce nonlocal transitions given sufficient delocalization of the polariton species—irrespective of spatial separation. Seemingly “spooky”, this action at a (far) distance is a manifestation of donor–acceptor entanglement resulting from strong light–matter coupling.86 While this relaxation mechanism and entanglement is present in typical molecular aggregates,87,88 the novelty in the polariton setup is the remarkable mesoscopic range of interactions that is effectively produced.

4. Conclusions

In summary, we have theoretically calculated experimentally consistent rates of PARET for various cases of SC. We employed a polariton (plexciton) setup consisting of a metal whose SP modes couple to donor and/or acceptor chromophores. For the case where a single type of chromophore is strongly coupled to SPs, we have demonstrated that energy transfer starting from delocalized states can be enhanced due to increased spectral overlap compared to the bare FRET case. Astonishingly, this transfer can remain fast up to 1 μm due to slowly decaying PRET coupling with respect to metal–chromophore separation when compared to the faster decaying interchromophoric dipole–dipole coupling. Also, we have shown that delocalizing the acceptors is a poor strategy to enhance EET starting from the donors, but can lead to an intriguing and efficient role-reversed (”carnival-effect”) EET starting from the acceptors. These observations shed new light on the timely debate of how to harness coherence to enhance molecular processes.49 Given their generality, they can also be applied to guide the design of polaritonic systems to control other chemical processes that have similar donor–acceptor flavor (e.g., charge transfer,89 electron transfer,48 singlet fission77) or reactant-product nature (e.g., cis–trans isomerization,41,90 dissociation89). Finally, our calculated rates support vibrational relaxation as the mechanism of PARET when both donors and acceptors are strongly coupled to a cavity mode. The results obtained in this work affirm light–matter SC as a promising and novel means to engineer novel interactions between molecular systems across mesoscopic length scales, thus opening doors to remote-controlled chemistry.

Conflicts of interest

There are no conflicts to declare.

Supplementary Material

Click here for additional data file. (921.3KB, pdf)

Acknowledgments

M. D., R. F. R., and J. Y.-Z. acknowledge funding from the NSF CAREER Award CHE-164732. L. A. M.-M. was supported by the UC-Mexus CONACyT scholarship for doctoral studies. M. D., R. F. R., J. Y.-Z., and L. A. M.-M. are also grateful for generous UCSD startup funds. V. M. M. acknowledges funding from DOE BES through grant no. DE-SC0017760. M. D. thanks Jorge Campos-González-Angulo and Rahul Deshmukh for useful discussions.

Footnotes

†Electronic supplementary information (ESI) available. See DOI: 10.1039/c8sc00171e

References

  1. Förster T. Ann. Phys. 1948;2:55–75. [Google Scholar]
  2. Govorov A., Martínez P. L. H. and Demir H. V., Understanding and Modeling Förster-type Resonance Energy Transfer (FRET): Introduction to FRET, Springer, Singapore, 2016. [Google Scholar]
  3. Jang S., Newton M. D., Silbey R. J. Phys. Rev. Lett. 2004;92:218301. doi: 10.1103/PhysRevLett.92.218301. [DOI] [PubMed] [Google Scholar]
  4. Jang S., Newton M. D., Silbey R. J. J. Phys. Chem. B. 2007;111:6807–6814. doi: 10.1021/jp070111l. [DOI] [PubMed] [Google Scholar]
  5. Kassal I., Yuen-Zhou J., Rahimi-Keshari S. J. Phys. Chem. Lett. 2013;4:362–367. doi: 10.1021/jz301872b. [DOI] [PubMed] [Google Scholar]
  6. Lloyd S., Mohseni M. New J. Phys. 2010;12:075020. [Google Scholar]
  7. Engel G. S., Calhoun T. R., Read E. L., Ahn T.-K., Mančal T., Cheng Y.-C., Blankenship R. E., Fleming G. R. Nature. 2007;446:782. doi: 10.1038/nature05678. [DOI] [PubMed] [Google Scholar]
  8. Duque S., Brumer P., Pachón L. A. Phys. Rev. Lett. 2015;115:110402. doi: 10.1103/PhysRevLett.115.110402. [DOI] [PubMed] [Google Scholar]
  9. Scholes G. D. Annu. Rev. Phys. Chem. 2003;54:57–87. doi: 10.1146/annurev.physchem.54.011002.103746. [DOI] [PubMed] [Google Scholar]
  10. Haedler A. T., Kreger K., Issac A., Wittmann B., Kivala M., Hammer N., Kohler J., Schmidt H.-W., Hildner R. Nature. 2015;523:196–199. doi: 10.1038/nature14570. [DOI] [PubMed] [Google Scholar]
  11. Saikin S. K., Shakirov M. A., Kreisbeck C., Peskin U., Proshin Y. N., Aspuru-Guzik A. J. Phys. Chem. C. 2017;121:24994–25002. [Google Scholar]
  12. Hsu L.-Y., Ding W., Schatz G. C. J. Phys. Chem. Lett. 2017;8:2357–2367. doi: 10.1021/acs.jpclett.7b00526. [DOI] [PubMed] [Google Scholar]
  13. Zhang X., Marocico C. A., Lunz M., Gerard V. A., Gunâko Y. K., Lesnyak V., Gaponik N., Susha A. S., Rogach A. L., Bradley A. L. ACS Nano. 2014;8:1273–1283. doi: 10.1021/nn406530m. [DOI] [PubMed] [Google Scholar]
  14. Ding W., Hsu L.-Y., Schatz G. C. J. Chem. Phys. 2017;146:064109. doi: 10.1063/1.4975815. [DOI] [PubMed] [Google Scholar]
  15. Bouchet D., Cao D., Carminati R., De Wilde Y., Krachmalnicoff V. Phys. Rev. Lett. 2016;116:037401. doi: 10.1103/PhysRevLett.116.037401. [DOI] [PubMed] [Google Scholar]
  16. de Torres J., Ferrand P., Colas des Francs G., Wenger J. ACS Nano. 2016;10:3968–3976. doi: 10.1021/acsnano.6b00287. [DOI] [PubMed] [Google Scholar]
  17. Götzinger S., Menezes L. d. S., Mazzei A., Kühn S., Sandoghdar V., Benson O. Nano Lett. 2006;6:1151–1154. doi: 10.1021/nl060306p. [DOI] [PubMed] [Google Scholar]
  18. Zhong X., Chervy T., Zhang L., Thomas A., George J., Genet C., Hutchison J. A., Ebbesen T. W. Angew. Chem., Int. Ed. 2017;56:9034–9038. doi: 10.1002/anie.201703539. [DOI] [PMC free article] [PubMed] [Google Scholar]
  19. Coles D. M., Somaschi N., Michetti P., Clark C., Lagoudakis P. G., Savvidis P. G., Lidzey D. G. Nat. Mater. 2014;13:712–719. doi: 10.1038/nmat3950. [DOI] [PubMed] [Google Scholar]
  20. Slootsky M., Liu X., Menon V. M., Forrest S. R. Phys. Rev. Lett. 2014;112:076401. doi: 10.1103/PhysRevLett.112.076401. [DOI] [PubMed] [Google Scholar]
  21. Feist J., García-Vidal F. J. Phys. Rev. Lett. 2015;114:196402. doi: 10.1103/PhysRevLett.114.196402. [DOI] [PubMed] [Google Scholar]
  22. Schachenmayer J., Genes C., Tignone E., Pupillo G. Phys. Rev. Lett. 2015;114:196403. doi: 10.1103/PhysRevLett.114.196403. [DOI] [PubMed] [Google Scholar]
  23. Yuen-Zhou J., Saikin S. K., Zhu T., Onbasli M. C., Ross C. A., Bulovic V., Baldo M. A. Nat. Commun. 2016;7:11783. doi: 10.1038/ncomms11783. [DOI] [PMC free article] [PubMed] [Google Scholar]
  24. Basko D. M., Bassani F., La Rocca G. C., Agranovich V. M. Phys. Rev. B: Condens. Matter Mater. Phys. 2000;62:15962–15977. [Google Scholar]
  25. Yang M., Fleming G. R. Chem. Phys. 2002;282:163–180. [Google Scholar]
  26. Zimanyi E. N., Silbey R. J. Philos. Trans. R. Soc., A. 2012;370:3620–3637. doi: 10.1098/rsta.2011.0204. [DOI] [PubMed] [Google Scholar]
  27. Davydov A. S. J. Exp. Theor. Phys. 1948;18:210–218. [Google Scholar]
  28. Davydov A., Theory of molecular excitons, McGraw-Hill, New York, 1962. [Google Scholar]
  29. Redfield A., in The theory of relaxation processes, Elsevier, 1965, vol. 1, pp. 1–32. [Google Scholar]
  30. Philpott M. R. J. Chem. Phys. 1970;52:5842–5850. [Google Scholar]
  31. Soules T. F., Duke C. B. Phys. Rev. B: Solid State. 1971;3:262–274. [Google Scholar]
  32. Holstein T. Ann. Phys. 1959;8:325–342. [Google Scholar]
  33. Mukamel S., Principles of nonlinear optical spectroscopy, Oxford University Press, 1995. [Google Scholar]
  34. Walls D. and Milburn G., Quantum Optics, Springer-Verlag, 1994. [Google Scholar]
  35. Waks E., Sridharan D. Phys. Rev. A: At., Mol., Opt. Phys. 2010;82:043845. [Google Scholar]
  36. Yuen-Zhou J., Saikin S. K. and Menon V., ArXiv e-prints, arXiv: 1711.11213.
  37. Zhou F., Liu Y., Li Z.-Y. Opt. Lett. 2011;36:1969–1971. doi: 10.1364/OL.36.001969. [DOI] [PubMed] [Google Scholar]
  38. Scully M. and Zubairy M., Quantum Optics, Cambridge University Press, New York, New York, 1997. [Google Scholar]
  39. González-Tudela A., Huidobro P. A., Martín-Moreno L., Tejedor C., García-Vidal F. J. Phys. Rev. Lett. 2013;110:126801. doi: 10.1103/PhysRevLett.110.126801. [DOI] [PubMed] [Google Scholar]
  40. Archambault A., Marquier F., Greffet J.-J., Arnold C. Phys. Rev. B: Condens. Matter Mater. Phys. 2010;82:035411. [Google Scholar]
  41. Martínez-Martínez L. A., Ribeiro R. F., Campos Gonzalez Angulo J. A., Yuen-Zhou J. ACS Photonics. 2017 [Google Scholar]
  42. Jang S., Jung Y., Silbey R. J. Chem. Phys. 2002;275:319–332. [Google Scholar]
  43. Jang S., Silbey R. J. J. Chem. Phys. 2003;118:9312–9323. [Google Scholar]
  44. Ma J., Cao J. J. Chem. Phys. 2015;142:094106. doi: 10.1063/1.4908599. [DOI] [PubMed] [Google Scholar]
  45. Baghbanzadeh S., Kassal I. Phys. Chem. Chem. Phys. 2016;18:7459–7467. doi: 10.1039/c6cp00104a. [DOI] [PubMed] [Google Scholar]
  46. Baghbanzadeh S., Kassal I. J. Phys. Chem. Lett. 2016;7:3804–3811. doi: 10.1021/acs.jpclett.6b01779. [DOI] [PubMed] [Google Scholar]
  47. Liu G. L., Long Y.-T., Choi Y., Kang T., Lee L. P. Nat. Methods. 2007;4:1015. doi: 10.1038/nmeth1133. [DOI] [PubMed] [Google Scholar]
  48. Herrera F., Spano F. C. Phys. Rev. Lett. 2016;116:238301. doi: 10.1103/PhysRevLett.116.238301. [DOI] [PubMed] [Google Scholar]
  49. Scholes G. D., Fleming G. R., Chen L. X., Aspuru-Guzik A., Buchleitner A., Coker D. F., Engel G. S., van Grondelle R., Ishizaki A., Jonas D. M., Lundeen J. S., McCusker J. K., Mukamel S., Ogilvie J. P., Olaya-Castro A., Ratner M. A., Spano F. C., Whaley K. B., Zhu X. Nature. 2017;543:647. doi: 10.1038/nature21425. [DOI] [PubMed] [Google Scholar]
  50. Ozel T., Hernandez-Martinez P. L., Mutlugun E., Akin O., Nizamoglu S., Ozel I. O., Zhang Q., Xiong Q., Demir H. V. Nano Lett. 2013;13:3065–3072. doi: 10.1021/nl4009106. [DOI] [PubMed] [Google Scholar]
  51. Hutchison J. A., Schwartz T., Genet C., Devaux E., Ebbesen T. W. Angew. Chem., Int. Ed. 2012;51:1592–1596. doi: 10.1002/anie.201107033. [DOI] [PubMed] [Google Scholar]
  52. May V. and Kühn O., Charge and Energy Transfer Dynamics in Molecular Systems, Wiley, 2011. [Google Scholar]
  53. Bednarz M., Malyshev V. A., Knoester J. J. Chem. Phys. 2002;117:6200–6213. doi: 10.1063/1.1643720. [DOI] [PubMed] [Google Scholar]
  54. Agranovich V. M., Litinskaia M., Lidzey D. G. Phys. Rev. B: Condens. Matter Mater. Phys. 2003;67:085311. [Google Scholar]
  55. Litinskaya M., Reineker P., Agranovich V. M. J. Lumin. 2004;110:364–372. [Google Scholar]
  56. del Pino J., Feist J., Garcia-Vidal F. J. New J. Phys. 2015;17:053040. [Google Scholar]
  57. Canaguier-Durand A., Genet C., Lambrecht A., Ebbesen T. W., Reynaud S. Eur. Phys. J. D. 2015;69:24. [Google Scholar]
  58. Zhong X., Chervy T., Wang S., George J., Thomas A., Hutchison J. A., Devaux E., Genet C., Ebbesen T. W. Angew. Chem., Int. Ed. 2016;55:6202–6206. doi: 10.1002/anie.201600428. [DOI] [PubMed] [Google Scholar]
  59. Palik E., Handbook of Optical Constants of Solids II, Academic Press, 1985. [Google Scholar]
  60. Bellessa J., Bonnand C., Plenet J. C., Mugnier J. Phys. Rev. Lett. 2004;93:036404. doi: 10.1103/PhysRevLett.93.036404. [DOI] [PubMed] [Google Scholar]
  61. Ma J., Moix J., Cao J. J. Chem. Phys. 2015;142:094107. doi: 10.1063/1.4908600. [DOI] [PubMed] [Google Scholar]
  62. Moix J. M., Ma J., Cao J. J. Chem. Phys. 2015;142:094108. doi: 10.1063/1.4908601. [DOI] [PubMed] [Google Scholar]
  63. Valleau S., Saikin S. K., Yung M.-H., Guzik A. A. J. Chem. Phys. 2012;137:034109. doi: 10.1063/1.4732122. [DOI] [PubMed] [Google Scholar]
  64. Govorov A. O., Lee J., Kotov N. A. Phys. Rev. B: Condens. Matter Mater. Phys. 2007;76:125308. [Google Scholar]
  65. Valeur B. and Berberan-Santos M., Molecular Fluorescence: Principles and Applications, Wiley, 2nd edn, 2012. [Google Scholar]
  66. Medintz I. and Hildebrandt N., FRET – Förster Resonance Energy Transfer: From Theory to Applications, Wiley, 2013. [Google Scholar]
  67. Andrews D. L. Chem. Phys. 1989;135:195–201. [Google Scholar]
  68. Juzeliūnas G., Andrews D. L. Phys. Rev. B: Condens. Matter Mater. Phys. 1994;49:8751–8763. doi: 10.1103/physrevb.49.8751. [DOI] [PubMed] [Google Scholar]
  69. Dung H. T., Knöll L., Welsch D.-G. Phys. Rev. A: At., Mol., Opt. Phys. 2002;66:063810. [Google Scholar]
  70. Coles D. M., Michetti P., Clark C., Tsoi W. C., Adawi A. M., Kim J.-S., Lidzey D. G. Adv. Funct. Mater. 2011;21:3691–3696. [Google Scholar]
  71. Virgili T., Coles D., Adawi A. M., Clark C., Michetti P., Rajendran S. K., Brida D., Polli D., Cerullo G., Lidzey D. G. Phys. Rev. B: Condens. Matter Mater. Phys. 2011;83:245309. [Google Scholar]
  72. Coles D. M., Michetti P., Clark C., Adawi A. M., Lidzey D. G. Phys. Rev. B: Condens. Matter Mater. Phys. 2011;84:205214. [Google Scholar]
  73. Somaschi N., Mouchliadis L., Coles D., Perakis I. E., Lidzey D. G., Lagoudakis P. G., Savvidis P. G. Appl. Phys. Lett. 2011;99:143303. [Google Scholar]
  74. Lidzey D. G., Fox A. M., Rahn M. D., Skolnick M. S., Agranovich V. M., Walker S. Phys. Rev. B: Condens. Matter Mater. Phys. 2002;65:195312. [Google Scholar]
  75. van Exter M., Lagendijk A. Phys. Rev. Lett. 1988;60:49–52. doi: 10.1103/PhysRevLett.60.49. [DOI] [PubMed] [Google Scholar]
  76. Sönnichsen C., Franzl T., Wilk T., von Plessen G., Feldmann J., Wilson O., Mulvaney P. Phys. Rev. Lett. 2002;88:077402. doi: 10.1103/PhysRevLett.88.077402. [DOI] [PubMed] [Google Scholar]
  77. Martínez-Martínez L. A., Du M., Ribeiro R. F., Kéna-Cohen S., Yuen-Zhou J. J. Phys. Chem. Lett. 2018;9:1951–1957. doi: 10.1021/acs.jpclett.8b00008. [DOI] [PubMed] [Google Scholar]
  78. Coles D. M., Grant R. T., Lidzey D. G., Clark C., Lagoudakis P. G. Phys. Rev. B: Condens. Matter Mater. Phys. 2013;88:121303. [Google Scholar]
  79. Chovan J., Perakis I. E., Ceccarelli S., Lidzey D. G. Phys. Rev. B: Condens. Matter Mater. Phys. 2008;78:045320. [Google Scholar]
  80. Michetti P., La Rocca G. C. Phys. Rev. B: Condens. Matter Mater. Phys. 2008;77:195301. [Google Scholar]
  81. Michetti P., La Rocca G. C. Phys. Rev. B: Condens. Matter Mater. Phys. 2009;79:035325. [Google Scholar]
  82. Hakala T. K., Toppari J. J., Kuzyk A., Pettersson M., Tikkanen H., Kunttu H., Törmä P. Phys. Rev. Lett. 2009;103:053602. doi: 10.1103/PhysRevLett.103.053602. [DOI] [PubMed] [Google Scholar]
  83. Skolnick M. S., Fisher T. A., Whittaker D. M. Semicond. Sci. Technol. 1998;13:645. [Google Scholar]
  84. Holmes R. J., Forrest S. R. Org. Electron. 2007;8:77–93. [Google Scholar]
  85. Törmä P., Barnes W. L. Rep. Prog. Phys. 2015;78:013901. doi: 10.1088/0034-4885/78/1/013901. [DOI] [PubMed] [Google Scholar]
  86. Garcia-Vidal F. J., Feist J. Science. 2017;357:1357–1358. doi: 10.1126/science.aao4268. [DOI] [PubMed] [Google Scholar]
  87. Kenkre V. and Reineker P., Exciton Dynamics in Molecular Crystals and Aggregates, Springer-Verlag, 1982. [Google Scholar]
  88. Sarovar M., Ishizaki A., Fleming G. R., Whaley K. B. Nat. Phys. 2010;6:462–467. [Google Scholar]
  89. Flick J., Ruggenthaler M., Appel H., Rubio A. Proc. Natl. Acad. Sci. U. S. A. 2017;114:3026–3034. doi: 10.1073/pnas.1615509114. [DOI] [PMC free article] [PubMed] [Google Scholar]
  90. Galego J., Garcia-Vidal F. J., Feist J. Nat. Commun. 2016;7:13841. doi: 10.1038/ncomms13841. [DOI] [PMC free article] [PubMed] [Google Scholar]

Associated Data

This section collects any data citations, data availability statements, or supplementary materials included in this article.

Supplementary Materials

Click here for additional data file. (921.3KB, pdf)

Articles from Chemical Science are provided here courtesy of Royal Society of Chemistry

RESOURCES