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HAL Id: jpa-00210635

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Submitted on 1 Jan 1987

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Collective spontaneous emission from a system of two atoms with multiphoton transitions in a cavity

A.S. Shumovsky, Fam Le Kien, E.I. Aliskenderov

To cite this version:

A.S. Shumovsky, Fam Le Kien, E.I. Aliskenderov. Collective spontaneous emission from a system of two atoms with multiphoton transitions in a cavity. Journal de Physique, 1987, 48 (11), pp.1933-1937.

�10.1051/jphys:0198700480110193300�. �jpa-00210635�

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Collective spontaneous emission from a system of two atoms

with multiphoton transitions in a cavity

A. S. Shumovsky, Fam Le Kien and E. I. Aliskenderov

Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Head Post Office, P.O. Box 79, Moscow, U.S.S.R.

(Requ le 23 avril 1987, accept6 le 23 juin 1987)

Résumé.

-

On détermine les caractéristiques de l’émission spontanée d’un système formé de deux atomes à

deux niveaux avec transitions multiphotoniques excités dans une cavité résonnante sans perte. On trouve que le comportement collectif de la multiplicité de photons affecte considérablement la dynamique et la statistique

de photons.

Abstract.

-

Characteristics of the collective spontaneous emission of a system consisting of two two-level multiphoton-transition atoms excited in a lossless resonant cavity are calculated. The photon-multiplicity

collective behaviour is found to affect the photon dynamics and statistics considerably.

Classification

Physics Abstracts

32.80

-

42.50

Recent experimental observations [1-4] of spon- taneous emission of Rydberg atoms in cavities make

. possible the testing of simple exactly soluble models of interaction of a single-mode radiation field with a few atoms (for a review see [5]). Exact solutions for the collective spontaneous emission from an assem-

bly of N atoms, placed into a lossless resonant cavity

and excited to a state with only one atom in the

excited state, have been derived [6]. The influence of cavity damping has been rigorously examined for the case of symmetrical Dicke one-atom initial

excitation [7]. The exactly soluble model of two one-

photon-transition two-level atoms in a lossless cavity

has been discussed [8-12, 31]. It has been shown that

interesting quantum effects such as super-radiance,

radiation trapping, vacuum-field Rabi oscillations, collapse and revival of Rabi oscillations are also

possible. The emphasis, however, has been on the

time behaviour of the mean photon number and

atomic inversion. The spectrum and various charac- teristics of vacuum-field Rabi oscillations in one- and

two-photon-transition atoms have been examined

[31]. In this paper we treat collective spontaneous emission from a system of two two-level atoms with multiphoton transitions. The case when both atoms are excited is considered on the basis of an exact solution and a detailed analysis.

The Hamiltonian for two two-level atoms interact-

ing with a resonant single-mode radiation field in a

lossless resonant cavity via m-photon transitions in the rotating wave approximation reads as :

where Rj and Rf are the population inversion and transition operators of the j-th atom, a’ and a are

the photon creation and annihilation operators for the resonant field mode, w0 and «) = lù 0/ m are the frequencies of the atomic transition and the mode, g

is the atom-field coupling constant, and m is the

photon multiple of atomic transitions. We have

neglected the variation of the field over the distance between the two atoms. It should be mentioned here that the development of the laser has led to the study

and exploitation of highly nonlinear phenomena

such as multiphoton transitions and that the sequ-

ences of from 1- to as many as 28-photon transitions have recently been observed [13].

_

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198700480110193300

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1934

Let at the initial time t = 0 both the atoms be

prepared in the excited state and the radiation field be in the vacuum state. We expect that, in this situation, self-Rabi oscillation phenomena arise, as in the single-atom one-photon-transition spontane-

ous emission : the field radiated by the atoms is

stored in the cavity a long time, and is eventually

reabsorbed by the atoms. The situation has been studied for the case of many atoms with one-photon-

transitions [14-16, 5], and recently, for the case of multiphoton transitions [17-20].

On introducing the eigenstates of the free part HA + HF of the

the wave function of the total system in the interac- tion picture is quickly found to be :

where

and

From these equations we find the mean number of photons in the field

It is seen that (N (t )) undergoes cosine oscillations at two frequencies 2 f2 R and 4 n R. The presence of two types of vacuum-initial-field Rabi oscillations in the temporal behaviour of the mean photon number

is a feature of collective spontaneous emission from

a fully excited two-atom system [8].

Using equation (6) we obtain the maximum value of (N(t»

Note that this value is smaller than 2 m. The latter is the number of photons potentially emitted by two

separate excited single-atom systems. Thus, the system of two initially excited atoms considered here cannot give out all stored energy to radiation. This

implies the occurrence of the radiation trapping

effect [6] which is possible in the system due to interference between emission processes of the two atoms. The degree of trapping can be defined by the

factor :

For the cases of single- and two-photon-transitions,

i. e. when m = 1 and m = 2, we have R = 1/9 and R = 25/49, respectively. It is easily shown that the

larger is the photon-multiple m of atomic transitions,

the larger is the factor R, and consequently, the higher is the degree of trapping.

The times at which the photon number (N (t))

reaches the maximum value (7) are :

where tR is the Rabi half-period defined by :

We also see from equation (6) that (N (t )) is equal

to zero at the times to N = 2 K tR ( K = 0, 1, 2, ...).

So, the time tR is the characteristic duration of the collective spontaneous emission process in the sys- tem. The collective features become apparent if we compare the above results with the single-atom case,

where the wave function, mean photon number, radiation trapping factor and the characteristic time of emission are given by [18, 19, 5] :

respectively. From equations (10) and (lld) we find

that the characteristic time tR of the two-atom case is

shorter than the characteristic time t R (1) of the single-

atom case,

For the cases of single- and two-photon-transitions (m = 1, 2) we have tRltA!) = -V2/3, B/2/7, respect- ively. It is seen from equation (12) that the larger is

the photon-multiple m of transitions, the smaller is

the ratio tRltA!), and consequently, the higher is the

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degree of atomic co-operation in the collective process.

We now consider the radiation rate I (t ) calculated

from equation (6),

It is easily established that I (t ) reaches the maximum value

at times

where the notation

and the characteristic time

Fig. 1.

-

Evolution of the radiation rate I (t ) in the case of two-photon transitions (m = 2). The time unit is l/g. The

full line corresponds to emission (I > 0), the dotted line to

reabsorption (I 0). The asymmetry of the emission

curve relative to the peak time is seen.

have been introduced. Further, I (t ) is equal to zero

at the times tOJ = KtR’ K = 0, 1, 2,

...

Finally, at

times

the rate I(t) takes the negative minimum value

I miD = - I max’ This is in agreement with the reab-

sorption process.

The relation (17) between the characteristic time tD for peaks and the characteristic time tR for nulls of the radiation rate I(t) shows that t D - t Rand

tD > tR/2. The latter inequality indicates that the

shape of the curve describing the evolution of

I (t ) in the time interval 0 , t _ t R is asymmetrical

relative to the peak time tD (see Fig. 1). This is a

feature of the collective behaviour. In the case of a

single atom in a lossless cavity [21, 22, 5], the

radiation-rate oscillations described by the sine-

function are symmetrical relative to the peaks.

According to equation (llb), the radiation rate

1(1 >(t), its maximum value I maX and the characteristic time t bI for the single-atom case are given by

From equations (17), (18c) and (10) we find that the ratio tD/tbl) is smaller than unity and decreases

rapidly when the photon multiple m increases. In

particular, for the cases of one-, two-, three- and

ten-photon-transitions one obtains tD/tbl):::::: 0.934,

0.648, 0.380 and 0.0004, respectively. Using equations (14), (16), (5) and (18b), one can further

show that 2 lmax/ImaX 4 for the case m =1, Imax/Imax 2 when m > 2, and Imax/I max 1 when

m > 4. Moreover, numerical calculations for the

cases m =1, 2, 3, 4 and 10 give the values

Imax/I (m’a)x 2.241, 1.968, 1.284, 0.727 and 0.014, respectively. Thus, the collective behaviour of the system considered here is strictly distinguished from

the super-fluorescent behaviour of an assembly of

excited atoms in a low-Q cavity [23-26, 5] where the

maximum radiation rate is proportional to the square of the atom number. The above results clearly show

the influence of the trapping effect which leads to limited superradiance in the case m = 1 and to

subradiance in the cases m > 2.

We now study the photon statistics in collective

spontaneous emission using the solution given by

equations (3) and (4). For this aim we calculate the

normalized correlation function defined as :

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1936

Here N(t)> is the mean photon number given by equation (6), and (N2(t) is the mean square value of the photon number found from equations (3) and (4) to be :

With the definition (19), the photon antibunching (sub-Poissonian statistics) condition can be written simply as g2(t) 1 [27, 28]. For t =F 2 KtR ; K = 0, 1, 2, ..., we can easily show that

and

This means that the statistics of the photons emitted spontaneously and collectively by the system of two

atoms is, in the case of one-photon-transitions, sub- Poissonian, and in the other multiphoton-transition

cases, super-Poissonian, for all times except for the

moments at which the field is in the vacuum state.

The maximum amount of photon antibunching being possible only in the case m = 1, is characterized by

the factor gm2n = 9/16, see equation (21). The

situation is different for the system consisting of a single atom excited. In this case the correlation function g(2)(t) is found from equations (lla) and (19) to read

From equation (23) we find that the photon anti- bunching effect can occur for any photon multiple m

in the single-atom case, and the corresponding

maximum amount of photon antibunching is deter-

mined by the factor gm2n = 1 - 11m. Thus, the

effect of either cooperativity or photon multiplicity

is generally to reduce the possibility and magnitude

of photon antibunching. This reduction is somewhat similar to the reduction of antibunching and squeez-

ing in resonance fluorescence [19, 30].

In conclusion, we have presented a rigorous and

detailed treatment for collective spontaneous emis- sion from a system of two two-level atoms with multiphoton transitions in a lossless resonant cavity.

The characteristics of the photon dynamics and

statistics have been calculated. It has been shown that interesting quantum effects such as self-induced Rabi oscillations, radiation trapping, limited super- radiance (in the case m = 1), subradiance (in the

case m , 2) and photon antibunching (in the case

m = 1) are possible. The considerable influence of the cooperativity and photon multiplicity on the

behaviour of the emission has been found to reduce the characteristic times and the possibility and magnitude of photon antibuching. An asymmetry of the emission curve relative to the peak time as a

feature of the collective behaviour has been noted.

The effect of cavity damping on the dynamics and

statistics of photons in the system will be discussed in

a subsequent paper.

References

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[5] HAROCHE, S. and RAIMOND, J. M., Adv. At. Mol.

Phys. 20 (1985) 347, D. R. Bates and B. Beder-

son eds. (Academic Press, New York) 1985.

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[9] VAN, C. L., Acta Phys. Pol. A 68 (1985) 647.

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[11] WALLS, D. F., J. Phys. A 4 (1971) 813.

[12] BARNETT, S. M. and KNIGHT, P. L., Opt. Acta 31 (1984) 435, 1203.

[13] BLOOMFIELD, L. A., STONEMAN, R. C. and GAL-

LAGHER, T., F., Phys. Rev. Lett. 57 (1986) 2512.

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[20] COMPAGNO, G., PENG, J. S. and PERSICO, F., Opt.

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