Open Access Article
A.
García-Vela
Instituto de Física Fundamental, Consejo Superior de Investigaciones Científicas, Serrano 123, 28006 Madrid, Spain. E-mail: garciavela@iff.csic.es
First published on 13th March 2019
A unified weak-field control scheme to modify the two properties that determine the whole behavior of a resonance state, namely the lifetime and the asymptotic fragment distribution produced upon resonance decay, is proposed. Control is exerted through quantum interference induced between overlapping resonances of the system, by exciting two different energies at which the resonances overlap. The scheme applies a laser field consisting of a first pulse that excites the energy of the resonance to be controlled, and two additional pulses that excite another different energy to induce interference, with a delay time with respect to the first pulse. Each of the two additional pulses is used to control one of the two resonance properties, by adjusting its corresponding delay time: with a relatively short delay time the second pulse controls the resonance lifetime, while with a very long delay time the third pulse modifies the asymptotic fragment distribution produced. The efficiency of the control of each resonance property is found to be strongly dependent on the choice of the second interfering energy, which allows for a more flexible control optimization by choosing a different energy for each property. The theory underlying the interference mechanism of the control scheme is developed and presented, and is applied to analyze and explain the results obtained. The present scheme thus appears to be a useful tool for controlling resonance-mediated molecular processes.
Strategies to control the resonance lifetime based on quantum interference have been suggested in environments of both overlapping and isolated resonance states in the weak-field regime.35–39 Quantum interference was also the basis of different weak-field control schemes proposed to modify the fragment distribution produced upon resonance decay.40–44 Some of the above control schemes share the common feature that they apply a pump laser field consisting of two pulses with a time delay between them.36,37,39,42–44 Each of these two pulses is used to excite a different resonance energy in an environment of overlapping resonances, which then interfere. By varying the time delay between the pulses, the resonance interference can be controlled. Depending on how long is the time delay between the pulses, control of a different resonance property (either the lifetime or the fragment distribution) is achieved. More specifically, if the time delay between the pulses is relatively short, such that the two resonances are simultaneously populated in time, the lifetime of both resonances can be controlled.36,37,39 However, when the time delay is long enough such that the population of the resonance excited with the first pulse has decayed completely when the other resonance is excited with the second pulse, then the product fragment distribution associated with the first resonance can be modified in the asymptotic time regime.44 Thus, the time delay applied between pulses is related to the nature and time scale of the resonance property under control.
So far the above type of control scheme has been applied to modify separately either the resonance lifetime or the fragment distribution. However, it is possible – and desirable – to design a unified control scheme that allows for the control of the two resonance properties determining the behavior of a resonance-mediated molecular process. Indeed this can be done by applying a laser field consisting of several pulses, where the first pulse would excite the resonance to be controlled, while the subsequent pulses would be delayed with respect to the first one accordingly to the dynamical time scale of the resonance property which is to be modified. The practical advantage of such a unified scheme is that the behavior along the whole course of the process of interest can be controlled within a single experiment, just by choosing appropriately the time delay of the pulses that control each resonance property. The main goal of the present work is to demonstrate the possibility of this unified control scheme both numerically and formally, by developing the underlying equations of the theory. As in earlier works the scheme is applied to the vibrational predissociation of the Ne–Br2(B,ν′) complex, because this system features overlapping resonances in different regimes. Resonances are common to several types of weakly bound complexes.45
This paper is organized as follows. Section 2 presents the main features of the methodology applied, and the formal theory underlying the control scheme. In Section 3 the results are presented and discussed. Conclusions are given in Section 4.
The Ne–Br2(B,ν′,n′) excitation with a laser field and the subsequent predissociation were simulated with a full three-dimensional wave packet method (assuming J = 0) described in detail elsewhere.4,35 In order to assess the quality of the model applied, it is noted that the lifetime calculated with the present theoretical model for the decay of the Ne–Br2(B, ν′ = 16) ground intermolecular resonance was found to be 69 ps,38 while the corresponding lifetime estimated experimentally is 68 ± 3 ps.47 This good agreement implies that both the three-dimensional wave packet method and the potential surfaces used in the present simulations are realistic enough in order to describe this resonance decay process.
In what follows the formal theory underlying the unified control scheme proposed in this work is developed. Let Ĥ be the total Hamiltonian of a molecular system that supports resonances. Following the discussion on the decay of a resonance state of Cohen-Tannoudji et al.,48 we can write Ĥ as Ĥ = Ĥ0 + W, where Ĥ0 is a zeroth-order Hamiltonian and W is a coupling. The spectrum of Ĥ0 consists of a set of discrete bound states χi (located in the interaction region) with associated energies Ei, and a set of continuum states φE,m (associated with the product fragments in the asymptotic region) with associated energies E and with m a global label for the fragment internal states. When W = 0 the χi states are true bound states, but when W ≠ 0, χi become resonances ψi that decay to the continuum of φE,m states. These states fulfill the orthogonality relations
| 〈χi|χj〉 = δij, 〈φE′,m′|φE,m〉 = δm′mδ(E′ − E), 〈χi|φE,m〉 = 0 | (1) |
![]() | (2) |
Let us now assume that within a vibrational manifold ν′ of Ne–Br2(B,ν′) featuring a group of intermolecular overlapping resonances, a given resonance energy Ea is excited with an electric field consisting of a Gaussian-shaped pulse,
, where A1 is the pulse amplitude, t1 is the time center of the pulse, σ is related to the pulse temporal width, ω1 is the photon frequency required to excite the resonance energy Ea from the ground vibronic state Ne–Br2 (X, ν′′ = 0, n′′ = 0), and ϕ1 is the pulse phase. It is noted that in a framework of overlapping resonances, several resonances may contribute at a given energy Ea, one of them providing the dominant contribution.49 Excitation of the system by
creates a wave packet ξEa(t) that can be expressed as
![]() | (3) |
and
. The basis of the control scheme suggested is to induce quantum interference between the overlapping resonances, and to achieve this goal (at least) two resonance energies are to be excited by applying a laser field with two Gaussian pulses,![]() | (4) |
is applied to excite the resonance energies Ea (excited by the pulse centered at t1) and Eb (excited by the pulse centered at t2), a wave packet is created,| Φ(t) = ξEa(t) + ξEb(t), | (5) |
. We shall assume that the two pulses of
are spectrally narrow enough such that they, and therefore ξEa(t) and ξEb(t), do not overlap in energy. Now, using eqn (3) we can write,![]() | (6) |
![]() | (7) |
![]() | (8) |
and
.
Eqn (8) shows that Ia(t) consists of four terms. The first term,
, is the survival probability that would be obtained if a single resonance energy Ea was excited with the
field. The lifetime associated with this
survival probability would be the “isolated resonance lifetime”, τisoa. The three additional terms of eqn (8) arise from the excitation of amplitude at the second energy Eb and its interference with the resonance amplitude excited at Ea. Those three terms are nonzero as long as the
and
amplitude coefficients are simultaneously nonzero. Such a condition is fulfilled if the two energies are excited simultaneously, which is achieved if the two pulses of
overlap in a temporal range. The effect of these interference terms is “dressing” the isolated resonance survival probability
, and therefore changing its shape. As a result of this change in shape, the lifetime associated with Ia(t) also changes from τisoa to a different value. By varying the delay time Δt between the pulses, one can modify the range of temporal overlap between them, and therefore the relative magnitude of the
and
amplitudes excited simultaneously. This causes variation of the interference terms in a controlled manner, which leads to a change in the shape of Ia(t) and to the control of the associated lifetime.
As shown by eqn (8), the basis of the resonance lifetime control is the quantum interference between resonance amplitudes generated simultaneously in the interaction region of Ĥ by different pulses of the laser field applied, with a delay time between them. Clearly, this interference is not possible if the amplitudes are not generated at the same time, and the interference effect vanishes when the resonance population decays completely. Thus the requirement of simultaneous population of the interfering amplitudes implies a temporal overlap of the pulses to a certain extent, which means that the delay time between them must be smaller than the sum of their half temporal widths. It is noted from the above equations that the quantum interference on which the control effect is based does not require particularly high amplitudes of the pulses (A1 and A2), which allows application of the control scheme under weak-field consditions.
The asymptotic probability of the fragment state φE,m at energy E can be expressed as
![]() | (9) |
is a constant and Φ(t) is the wave packet created by the electric field applied. Let us suppose now that we want to control the energy-resolved asymptotic fragment distribution produced upon decay of the resonance associated with energy Ea. To achieve this goal by quantum interference we again apply the two-pulse laser field
of eqn (4), that excites the same two resonance energies Ea and Eb, and thus creates a wave packet Φ(t) like that of eqn (5). The only difference with the previous situation of the control of the resonance lifetime is that now the delay time Δt = t2 − t1 between the two pulses is very long. The reason for the long delay time of the second pulse exciting the Eb energy with respect to the first one is to allow enough time for the first resonance excited at Ea to decay completely and to reach the asymptotic time regime of the fragment distribution produced. Then, by using the expression of Φ(t) of eqn (6), where the asymptotic fragment states φEa,m have been populated after the decay of the population excited to Ea, we can project out Φ(t) onto the fragment states φEa,m to calculate the distribution at energy Ea,![]() | (10) |
![]() | (11) |
Eqn (11) is very similar to eqn (8) in that it also consists of a sum of four terms, three of which arise from the excitation of both the Ea and Eb energies and the interference between them. If a single-pulse
field is applied to excite Ea, then ξEa(t) ≠ 0, ξEb(t) = 0, and the distribution becomes
, where interference is absent. Excitation of the second energy Eb by applying
induces interference between the overlapping resonances which manifests itself in the three additional terms of eqn (11). It is stressed that the interference terms of eqn (11) will appear as long as the amplitude ξEb(t) is created by the second pulse of
, and this can be done at any asymptotic time as long as desired, and as many times as desired (using further successive pulses after the second one in the laser field).44
The mechanism of interference between amplitudes produced in continuum fragment states by exciting two overlapping resonances with a long delay time between the two excitations may appear somewhat ellusive. It can be described as follows. Initially the first pulse of
excites the resonance energy Ea creating the ξEa(t) wave packet amplitude. After a long time, once this amplitude has decayed completely to the continuum states and has reached the asymptotic behavior, the second pulse of
excites the resonance energy Eb creating the ξEb(t) amplitude. Since both resonances overlap they share common continuum states φE′,m′ in a range of energies E′. The second pulse initially populates the χk states in the interaction region with an amplitude
. After some time this amplitude decays to the continuum states φE′,m′, spreading and redistributing temporarily among those φE′,m′ states which are shared by both ξEa and ξEb, producing the amplitude
. The appearance of this amplitude is what causes interference with the “asymptotic”
amplitude generated much earlier by the decay of the resonance amplitude excited by the first pulse. The amplitude
, however, is generated in the φEa,m states only temporarily, during the time that the second delayed pulse excites amplitude to Eb that will further decay initially to φEa,m states shared with ξEa. After the second pulse is over all the
amplitude temporarily generated in φEa,m states vanishes, redistributing among φEb,m states that contribute to the asymptotic distribution Pm(Eb,t∞), because the amplitude excited at Eb cannot contribute to the asymptotic Ea distribution Pm(Ea,t∞). As a result, the interference effect ceases, and Pm(Ea,t∞) converges to
. This is the expected result, in agreement with the previous prediction50 that no permanent weak-field coherent control of fragment distributions is possible after the excitation pulse has vanished.
The weak-field strategy applied to control the fragment distribution and reflected in the interference of eqn (11) has similarities with that used in strong-field control techniques. Indeed, the second pulse of
plays a similar role as the control field in strong-field techniques, in the sense that it produces the desired control effect while it is on. The difference is that the control effect on the fragment distribution ceases when the control pulse is over in the present weak-field scheme, while it remains in the strong-field case. This, however, does not prevent an effective control of the fragment distribution in the case of the weak-field scheme, if the fragments are detected or moved to other vibronic states of interest (applying a further laser pulse) while the interference effect takes place.
The origin and the basis of the interference in eqn (8) and (11), which govern the control of the resonance lifetime and the fragment diistribution, respectively, are essentially the same, and they only differ in the magnitude of the delay time between the pulses exciting Ea and Eb (relatively short in the case of the lifetime, and very long, in the asymptotic time regime for the fragment distribution). This common origin of the interference effect allows one to design a unified, single control scheme for the two resonance properties. Indeed, a simple way to control both the lifetime and the fragment distribution using a single scheme is to apply two “control pulses”, with a different delay time, with each of these pulses controlling one of the two resonance properties. More specifically, the electric field applied would consist of a combination of three Gaussian pulses,
![]() | (12) |
, but now with a very long delay Δt13 = t3 − t1 which allows for the control of the fragment distribution following eqn (11). In the simulations t1 is fixed at t1 = 0, which implies that Δt12 = t2 and Δt13 = t3. Thus, application of a single electric field makes possible the control of the two resonance properties that govern a molecular process by just using the appropriate delay time between the different pulses involved in the field.
A few remarks on the above control scheme are now due. In the previous discussion of the equations we have restricted to the excitation of the resonance energies (i.e., the energy of the resonance lineshape peak) for Ea and Eb. However, this is not a requirement of the scheme, and any other energies Ea and Eb different from the resonance ones can be excited, as long as the resonances involved overlap at those energies. The only avantage of exciting the resonance energies is that the control scheme becomes more efficient in principle, because the amplitude generated at the lineshape peaks associated with Ea and Eb is maximized (then maximizing the intensity of interference) with respect to other pairs of energies. For simplicity of the above description excitation of only two energies has been considered. But in the scheme the number of energies excited is not restricted, and excitation of more than two energies also increases the efficiency of the interference effect for the control of both the lifetime37 and the fragment distribution.44 All the above indicates that the applicability of the control scheme is quite flexible and general.
field applied in the simulations, for simplicity it is assumed that ϕ1 = ϕ2 = ϕ3 = 0. The amplitudes are A1 = A2 = 1.0 × 10−6 a.u., and A3 = 3.0 × 10−6 a.u. in the case of ν′ = 27, while for ν′ = 35 the values are A1 = A2 = 1.0 × 10−6 a.u., and A3 = 2.0 × 10−6 a.u. All these amplitudes correspond to a maximum pulse intensity of the order of 104 W cm−2, within the weak-field regime. The same full width at half maximum, FWHM = 200 ps (related to σ), is used for all the pulses in the different simulations. With this temporal width the corresponding spectral profiles of the pulses of
are narrow and do not overlap.
Two electric fields are applied in the simulations, namely
and
, in order to compare the results obtained for both the resonance lifetime and the fragment distribution in the situations of the absence of interference when exciting a single energy, and when two interfering energies are excited. In both cases the survival probability associated with the ground intermolecular resonance of either the ν′ = 27 or ν′ = 35 vibrational manifolds is calculated according to eqn (8) as Ik=0(t) = |〈ψk=0|Φ(t)〉|2, where ψk=0 is the wave function associated with the ground resonance, and Φ(t) is the wave packet prepared by the electric field applied. Now the corresponding lifetime, τ, is obtained by fitting Ik=0(t) to the function
![]() | (13) |
or
and A an amplitude scaling parameter.
The energy-resolved product fragment state distribution is calculated as follows. In the simulations the wave packet is represented in Jacobian coordinates (R,r,θ), where R is the distance between the Ne atom and the Br2 center of mass, r is the Br–Br internuclear distance, and θ is the angle between the vectors associated with R and r. In this representation the rovibrational eigenstates associated with the Br2(B,v,j) fragment are ζ(j)v(r)Pj(cos
θ), where ζ(j)v(r) are the vibrational eigenfunctions of Br2(B) with associated energies Ev,j and Pj(cos
θ) are Legendre polynomials, v and j being the Br2 vibrational and rotational quantum numbers, respectively. The population of the Br2(B,v,j) fragment states is computed along time by projecting out the wave packet onto the corresponding states
![]() | (14) |
| kv,j = [2μBr2(E − Ev,j)]1/2, | (15) |
![]() | (16) |
In the first set of simulations the Ne–Br2(B, ν′ = 27, n′ = 0) ground intermolecular resonance is excited. As shown in the associated excitation spectrum (Fig. 1), this resonance overlaps with some orbiting resonances of Ne–Br2(B, ν = ν′ − 1 = 26).5,35 The main peak of the spectrum located at Ea = −61.8 cm−1 corresponds to the Ne–Br2(B, ν′ = 27, n′ = 0) ground resonance, while the peak at Eb = −60.63 cm−1 and a weak peak at E = −59.5 cm−1 correspond to two v = 26 orbiting resonances overlapping with each other and with the ν′ = 27 ground resonance. The spectral profiles of the three pulses of
(A1 = A2, A3 = 3A1; the first pulse of
coincides with that of
) are plotted in Fig. 1. As shown in the figure, there is no spectral overlap between the first pulse of
and the other two.
As discussed above, when the single-pulse field
is applied to excite only the energy Ea, there is no possibility of interference and the asymptotic fragment distribution becomes
. In the case of Ne–Br2(B, ν′ = 27), when the energy Ea = −61.8 cm−1 is excited by
, the energy-resolved Br2(B,vf) vibrational distribution associated with Ea, calculated with eqn (14)–(16), is shown in Fig. 2. The population distributes among four vibrational final states, νf = ν′ − 1, ν′ − 2, ν′ − 3, and ν′ − 4, and these populations reach their asymptotic, constant values for t > 1000 ps.
Now, in order to exert control on both the Ne–Br2(B, ν′ = 27) ground resonance lifetime and the associated fragment distribution, the
field of eqn (12) is applied. The first and second pulses (centered at t1 and t2, respectively) excite the Ea and Eb energies, respectively, with a delay time Δt12 = 160 ps. The reason for choosing this specific delay time Δt12 is because it was previously shown that it maximizes the lifetime of the Ne–Br2(B, ν′ = 27) ground resonance.36 With such a delay time the first and second pulses of
overlap in time to some extent, as shown by the
temporal profile of Fig. 3(a). The next step is the modification of the Br2(B,vf) fragment vibrational distribution, by applying the third pulse (centered at t3) of
to excite again the Eb energy, but with a long delay time Δt13 within the asymptotic time region t > 1000 ps of the distribution. Specifically, two values Δt13 = 1500 and 2200 ps have been chosen. The reason for using two different Δt13 values instead of only one is to illustrate the fact that the interference effect can be induced in the asymptotic fragment distribution as many times as desired, as discussed above. The whole temporal profiles of the
fields applied with the two Δt13 delays are shown in Fig. 3(a).
The survival probability of the Ne–Br2(B, ν′ = 27) ground resonance, Ik=0(t), calculated when the single-pulse field
and the
fields of Fig. 3(a) are applied are displayed in Fig. 3(b). When
is used,
displays the shape of the convolution of the Gaussian pulse cross-correlation curve with the exponential decay associated with a single resonance, reflected by eqn (13). By fitting Ik=0(t) with eqn (13) the associated lifetime τisok=0 = 23.5 ps is obtained.36 By applying
the Ea and Eb energies are excited by the first two pulses, and they interfere. This interference manifests itself in pronounced undulations in Ik=0(t) in the time range where the two interfering resonances remain populated. This is the interference effect reflected by eqn (8). As previously shown,36 those undulations are separated by a constant time interval which is the inverse of the energy difference Eb − Ea. By fitting now this Ik=0(t) function with eqn (13) a lifetime τk=0 = 75 ps is obtained.36 Thus an enhancement of the resonance lifetime by a factor of three can be achieved by means of quantum interference. The survival probability of Fig. 3(b) shows that when the third pulse of
is applied to excite Eb with the two Δt13 delays, the ground resonance is populated again, which is the behavior expected for resonances that overlap at different energies, among them Eb.
The Br2(B, νf < ν′) fragment distributions obtained when the
fields of Fig. 3(a) are applied are shown in Fig. 3(c). A clear modification of the asymptotic vibrational populations is induced when the third pulse of
excites the Eb energy at the two Δt13 delays, as previously found.44 During the application of the third pulse the populations display some undulations that reflect the interference effect predicted by eqn (11). As discussed above, once the third pulse is over and the resonance excited at Eb has decayed completely, the asymptotic populations converge back to the values
of the populations of Fig. 2. The interference effect is increasingly more intense as the vibrational population is larger in magnitude, because the larger is the amplitude
the larger will be the interference terms of eqn (11). In this sense it is noted that the second pulse of
also causes an interference effect on the vibrational populations of Fig. 3(c) around Δt12 = 160 ps, although much weaker since A2 = A3/3.
The results of Fig. 3 provide a practical illustration of the predictions of eqn (8) and (11). They demostrate that it is indeed possible to design a unified control scheme to modify the two resonance properties, namely the lifetime and the fragment distribution produced upon resonance decay, which govern a resonance-mediated molecular process. The above fact remains valid when we move to a stronger overlapping regime, as shown in the following.
The excitation spectrum associated with the Ne–Br2(B, ν′ = 35, n′ = 0) ground intermolecular resonance is shown in Fig. 4. It displays a stronger, more congested overlapping regime between different intermolecular resonances. The main peak of the spectrum, located at energy Ea = −56.34 cm−1, corresponds to the ν′ = 35 ground resonance. This resonance lies below the Ne + Br2(B, ν′ − 1 = 34, j′ = 0) dissociation threshold, and therefore it is embedded in the spectrum of intermolecular resonances of the ν′ − 1 = 34 vibrational manifold, which allows the remaining features of the spectrum of Fig. 4 to originate.51 Those resonances are broad enough so as to produce a stronger overlapping regime than in the case of Ne–Br2(B, ν′ = 27).
In a first simulation the energy Eb of the spectrum of Fig. 4 chosen to induce interference is Eb = −57.75 cm−1. While in a strong overlapping regime like that of Fig. 4 several resonances of the ν′ − 1 = 34 manifold (along with the ground resonance of ν′ = 35) overlap at this energy, it was previously determined that among them the dominant resonance is n = 9. The same as in Fig. 1, the spectral profiles of the three pulses of
(A1 = A2, A3 = 2A1) are plotted in Fig. 4.
In the case of the control of the behavior of the Ne–Br2(B, ν′ = 35) ground resonance, an
laser field with a Δt12 = 120 ps delay time has been applied (see Fig. 5(a)). As found previously,39 this is the delay time that maximizes the enhancement of the ν′ = 35 ground resonance lifetime. As in the previous case of Ne–Br2(B, ν′ = 27), the same Δt13 delays, namely Δt13 = 1500 and 2200 ps, are used.
![]() | ||
| Fig. 5 The same as Fig. 3 but for Ne–Br2(B, ν′ = 35), with Ea = −56.34 cm−1 and Eb = −57.75 cm−1. | ||
The survival probabilities associated with the Ne–Br2 (B, ν′ = 35, n′ = 0) resonance when the
and
fields are applied are shown in Fig. 5(b). A qualitatively similar interference pattern to that of Fig. 3(b) is found in Ik=0(t) when the
field is applied, as compared to the plain survival probability curve obtained with
. However, the intensity of interference and the change of the shape of Ik=0(t) appear to be more pronounced in the present case than for ν′ = 27. Actually, the τisok=0 lifetime associated with the survival probability obtained with
is τisok=0 = 3.8 ps, while the lifetime found when applying
is τk=0 = 61.0 ps.37,39 Thus the ν′ = 35 ground resonance lifetime is enhanced by a factor of 15, compared to the factor of 3 obtained for ν′ = 27. This larger effect of interference in the lifetime enhancement is likely due to the stronger overlapping between the n′ = 0 and the n = 9 resonances compared to the ν′ = 27 situation of Fig. 1. As discussed below, this result is related to the magnitude of the coefficients
and
of eqn (8), which depend on the intensity of the excitation spectrum at Ea and Eb, which is expected to be higher for stronger resonance overlap. As the overlap between the resonances increases, the magnitude of the amplitudes
and
in eqn (8) increases as well, producing a more intense interference effect. This is supported by the result that when the pair of resonances excited is n′ = 0 and n = 7 (located at −60.76 cm−1 in the spectrum of Fig. 4), with a weaker overlap than n′ = 0 and n = 9, τk=0 was enhanced only up to τk=0 = 37.0 ps under the same laser field conditions, i.e., somewhat more than half the enhancement achieved with the n′ = 0 and n = 9 resonances.39 Thus the main effect of increasing the intensity of resonance overlap would be to enhance the degree of control of the resonance lifetime.
The energy-resolved Br2(B, νf < ν′ = 35) fragment distributions obtained by applying the
fields of Fig. 5(a) are displayed in Fig. 5(c). Since the Ne–Br2(B, ν′ = 35, n′ = 0) resonance lies below the Ne + Br2(B, ν′ − 1 = 34, j′ = 0) dissociation threshold, the ν′ − 1 dissociation channel is closed, and the only open channels are νf ≤ ν′ − 2. For ν′ = 35 there are twice the number of open channels than for ν′ = 27. The vibrational populations reach their asymptotic, constant values for t > 500 ps. The interesting result is that a similar interference effect to that of the distributions of Fig. 3(c) is found in the present distributions when the third pulse of
is applied. So again the same qualitative interference behavior is found regardless of the intensity of resonance overlap. In Fig. 5(c) the intensity of the interference effect is somewhat weaker than in Fig. 3(c), which is not surprising since now A2 = 2A1, while for ν′ = 27 A2 = 3A1. However, the same as with the resonance lifetime, the stronger resonance overlap is also expected to favor the intensity of interference in the asymptotic fragment distribution. Indeed, again related to the
and
coefficients of eqn (6), the interfering amplitudes
and
of eqn (11) will be correspondingly larger for a stronger resonance overlap.
laser fields of Fig. 3(a) and 5(a), exciting the same Ea resonance energies as before (i.e., Ea = 61.8 cm−1 for ν′ = 27 and Ea = 56.34 cm−1 for ν′ = 35), but now changing Eb to values of 61.12 and 60.85 cm−1 for ν′ = 27, and 57.10 and 60.76 cm−1 for ν′ = 35. The additional Eb energies excited are indicated by arrows in Fig. 1 and 4 for ν′ = 27 and 35, respectively. Survival probabilities and energy-resolved Br2(B,vf) fragment distributions are calculated with the new Eb energies, and they are compared in Fig. 6 and 7 with those shown in Fig. 3 and 5.
![]() | ||
Fig. 6 Comparison of the (a) survival probabilities of the Ne–Br2(B, ν′ = 27) ground intermolecular resonance and (b) energy-resolved Br2(B,vf) fragment vibrational populations in the νf = ν′ − 2 final vibrational state associated with the Ea = −61.8 cm−1 energy, when three different Eb energies, Eb = −60.63, −61.12 and −60.85 cm−1, are excited by applying the electric fields of Fig. 3(a). | ||
![]() | ||
Fig. 7 Comparison of the (a) survival probabilities of the Ne–Br2(B, ν′ = 35) ground intermolecular resonance and (b) energy-resolved Br2(B,vf) fragment vibrational population in the νf = ν′ − 2 final vibrational state associated with the Ea = −56.34 cm−1 energy, when three different Eb energies, Eb = −57.75, −57.10 and −60.76 cm−1, are excited by applying the electric fields of Fig. 5(a). | ||
The Ik=0(t) survival probabilities found for the three different Eb energies for ν′ = 27 (Fig. 6(a)) and ν′ = 35 (Fig. 7(a)) indeed show an interference pattern in the temporal region where the first and second pulses of
overlap, indicating that resonance lifetime control is achieved in all cases. However, a clear trend – which is the same for ν′ = 27 and 35 – is found for the intensity of interference when the Eb energy changes: the interference intensity decreases remarkably as the corresponding excitation spectrum intensity (see Fig. 1 and 4) associated with the specific Eb energy decreases. The same effect is also displayed in the survival probability peaks appearing at Δt13 = 1500 and 2200 ps. The maximum interference intensity occurs for the resonance energies Eb = −60.63 cm−1 and Eb = −57.75 cm−1, which have associated the maximum intensity in the spectra of Fig. 1 and 4, respectively. The interference effect decreases for the other two values of Eb proportionally to the associated decrease in the spectrum intensity.
The explanation of the trend found in Fig. 6(a) and 7(a) for the interference intensity is provided by eqn (6) and (8), and more specifically by the amplitude coefficients
of eqn (8). Such coefficients denote the amplitude excited by the second (and third) pulse of
at energy Eb. This amplitude will depend on both the pulse amplitude A2 (or A3) and the spectrum intensity at Eb, which in turn is the sum of all the contributions of the different overlapping resonances at that energy. If A2 (or A3) does not change – since the
field is the same in the three simulations of Fig. 6 and 7 –
only changes due to the change of spectrum intensity when Eb is varied, and this variation affects the intensity of the interference terms of eqn (8). The implication is that the change in shape of Ik=0(t) is smaller for the two additional Eb energies for ν′ = 27 and 35, which is reflected in a lower enhancement of the ground resonance lifetime. A clear illustration of this effect is the case mentioned above for ν′ = 35, that τk=0 is enhanced from 3.8 ps to 61.0 ps when the resonance energy Eb = −57.75 cm−1 is excited, while it is only enhanced up to 37.0 ps when the energy Eb = −60.76 cm−1 (with a lower spectrum intensity associated) is exccited. The magnitude of the
coefficients also explains why the lifetime enhancement is maximized when Eb coincides with a resonance energy, and why a stronger overlap between resonances, which is expected to increase the spectrum intensity, favors the intensity and efficiency of lifetime control.
The energy-resolved Br2(B, νf = ν′ − 2) fragment populations associated with the ground resonance energies Ea = 61.8 cm−1 for ν′ = 27 and Ea = 56.34 cm−1 for ν′ = 35, obtained when the three different Eb energies are excited, are displayed in Fig. 6(b) and 7(b), respectively. For the sake of the clarity of the figures only the νf = ν′ − 2 population is shown, but the remaining Br2(B,vf) populations display the same behavior with Eb as that of ν′ − 2. Similarly to the resonance survival probability, the behavior of the fragment distribution also depends on the choice of Eb, and again both ν′ = 27 and 35 show the same trend. In this case the intensity of the interference effect in the fragment populations does not appear to depend only on the corresponding excitation spectrum intensity, but also on the proximity of Eb to the energy Ea for which the fragment distribution is calculated. Indeed, for ν′ = 27 the intensity of the interference effect is similar for Eb = −60.63 and −60.85 cm−1, while it increases appreciably for Eb = −61.12 cm−1, which is closer to the energy Ea = −61.8 cm−1. The trend is more clear for ν′ = 35 where, with respect to the result obtained for Eb = −57.75 cm−1, the interference intensity decreases remarkably (by about a factor of two) when Eb gets far away from Ea to Eb = −60.76 cm−1, while in contrast the intensity increases by a factor of three for the closer energy Eb = −57.10 cm−1. The spectral intensity associated with the two additional Eb energies is lower, both for ν′ = 27 and 35, than that associated with the resonance energies Eb = −60.63 and −57.75 cm−1.
The explanation of the behavior of the intensity of the interference effect in the fragment distribution lies in eqn (2), (6), and (11). As reflected by eqn (2), a stationary eigenfunction ψE(t) can be expressed as a superposition of continuum fragment states φE′,m′ with amplitudes
. It is expected that the maximum amplitude coefficients will be those associated with the energy E′ = E,
, and that the magnitude of
will gradually decrease as E′ gets far away from E. Thus, when a given energy Eb is excited (with a narrow bandwidth around it), in the corresponding eigenfunction ψEb(t) the maximum amplitudes are
.
As discussed above, the long-delayed third pulse of
that excites the Eb energy produces temporarily the amplitude
(see eqn (6), (10), and (11)) that interferes with the asymptotic
amplitude previously generated by the first pulse of
. The dependence again on the
coefficients indicates that the interference effect in the fragment distribution depends also on the spectral intensity at energy Eb, as in the case of the survival probability. But
depends on the magnitude of the
coefficients as well. And the
coefficients in the superposition of the ψEb(t) eigenfunction (and of those in the narrow bandwidth around) populated by the third pulse of
will be higher – thus making also the
amplitudes in eqn (11) higher – as long as Eb becomes closer to Ea. This explains the trend found in the results of Fig. 6(b) and 7(b) for the intensity of the interference effect. The dependence of
on the spectral intensity at Eb also explains the similarity of the interference intensity found at the two energies Eb = −60.63 and −60.85 cm−1 for ν′ = 27, because the smaller separation between Ea and Eb = −60.85 cm−1 is probably compensated by the lower spectral intensity at that energy compared to Eb = −60.63 cm−1.
The results of Fig. 6 and 7 have an interesting implication. From the theory developed above it is clear that control can be selectively exerted on each of the two resonance properties by properly choosing the magnitude of the delay time between the pulses that excite the two interfering energies Ea and Eb. This temporal selectivity is related to the nature and time scale of the properties: the resonance survival probability and the associated lifetime are relatively short-time scale properties, while the fragment distribution is an asymptotic, long-time scale property. But in addition to this generic dependence of the control of the delay time between pulses, there is a strong dependence of the degree and efficiency of the control of the location of the second energy excited to induce the interference. And this dependence is different for the two resonance properties. The clear implication is that it is possible to optimize the control of the two properties by choosing properly a different Eb energy for each of them: optimization of lifetime control requires to maximize the spectral intensity at Eb, regardless of the separation between Ea and Eb, while optimal fragment distribution control requires minimization of the separation between Ea and Eb, but also keeping high enough spectral intensity at Eb.
The scheme is applied to two different situations where the intensity of resonance overlap is relatively weak and stronger. In both cases the control scheme works in a qualitatively similar way, although the interference effect becomes more intense as the overlap intensity increases, making the scheme more efficient. The degree and efficiency of the control achieved are shown to depend strongly on the choice of the second energy excited to induce interference with the energy of the resonance to be controlled. This dependence is found to be different for the two resonance properties, which implies that the control over each property can be optimized by choosing properly a different interfering energy in each case.
The formal theory underlying the unified interference control scheme is developed and presented. Such a theory explains all the results found when the control scheme is applied in different situations, and allows the design of the suitable conditions for the optimal control of the resonance properties. Due to the simplicity of the scheme, a wide application to control resonance-mediated molecular processes is envisioned.
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