collapses and revivals in two-level atoms in a superposed state interacting with a single mode...
TRANSCRIPT
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International Journal of Modern Physics BVol. 22, No. 17 (2008) 2725–2739c© World Scientific Publishing Company
COLLAPSES AND REVIVALS IN TWO-LEVEL
ATOMS IN A SUPERPOSED STATE INTERACTING
WITH A SINGLE MODE SUPERPOSED
COHERENT RADIATION
HARI PRAKASH∗,† and RAKESH KUMAR∗,‡
∗Department of Physics, University of Allahabad, Allahabad 211 002, India†M. N. Saha Centre of Space Studies, Institute of Interdisciplinary Studies,
University of Allahabad, Allahabad 211 002, India‡Department of Physics, Udai Pratap Autonomous College,
Varanasi 221 002, India†prakash [email protected]
Received 17 May 2007
Collapses and revivals phenomenon in system of a single two-level atom and two two-levelatoms existing in some superposed states and interacting with a single mode superposedcoherent radiation is studied. For superposed Dicke states |1/2, ±1/2〉 of a single two-level atom interacting with even or odd coherent state, only odd revivals occur. Fortwo two-level atoms, it is found that the collapse and revival times for even and oddcoherent states are equal to one half of the corresponding times for coherent state. Forthis system, Rabi oscillations occur with a main mean frequency and also some secondharmonics are present, in general. However, if the two atoms are in the superradiantstate, only the second harmonics with large amplitude are obtained. The appearance ofweak double frequency revivals for superposed atomic and coherent states was studiedand a condition for their disappearance is found.
Keywords: Two-level atoms; coherent radiation; collapses and revivals.
PACS numbers: 42.50.Dv, 42.50.-P, 42.50.ct, 42.50.Md
1. Introduction
The Jaynes–Cummings (J–C) model1–3 of a two-level atom interacting with a single
mode of radiation provides non-classical effects in interaction between electromag-
netic field and matter. One of the important aspects of the J–C model is that it is
exactly solvable for the arbitrary atom–field coupling constant and field strength.
The J–C model describes many interesting effects such as Rabi oscillations,4–9 col-
lapses and revivals of the atomic inversion,4–13 photon antibunching,14–16 quadra-
ture squeezing13,17–19 etc. One interesting phenomenon is the behavior of atomic
inversion under Rabi oscillations. Semi-classical treatment of two two-level atoms
2725
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2726 H. Prakash & R. Kumar
with a classical field or a quantum theory of interaction of two-level atom with a
pure occupation number radiation state involves Rabi oscillations with a fixed fre-
quency. However, if radiation is superposition of several occupation number states,
there is an initial collapse of Rabi oscillations followed by regular revivals that slowly
become broader and less intense and eventually overlap. The revival–collapse phe-
nomenon is a pure quantum mechanical effect having its origin in the granular
structure of the photon number distribution of the field.4–9,20 It has been extended
for multi-atom system21–24 as well as multi-level system.25,26 Some extensive study
of this phenomenon has also been carried out for single photon transition,27 two-
photon coherent state,28,29 binomial state,30 mixed coherent chaotic state31 and
coherent superposition states.29,32 Recently, Faisal A A El-Orany studied the re-
lation between the atomic inversions in particular the occurrence of collapse and
revival phenomenon with, fluctuation of quadrature field,33,34 higher order fluctu-
ation of quadrature fields components35 and wigner function36 in the multiphoton
J–C model. He also studied the same for a single mode field interacting with two
two-level atoms.37 Collapse and revival phenomenon in J–C model has also been
discussed earlier by several authors,38–40 but they consider only excited or de-
excited state atomic assembly interacting with coherent, binomial or superposed
coherent states. Faisal A A El-Orany33,34 considered the superposition of atomic
state interacting with an orthogonal even coherent state and find regular revivals.
Experimental observation of collapses and revivals has been reported by Rempe
et al.41 and Rabi oscillation has been observed by Gentile et al.
42
In this paper, we consider a superposed atomic state having equal weightages
of the lower and upper states, |l〉 and |u〉, interacting with radiation in a super-
posed state of coherent state |α〉 and | − α〉 in equal proportion, i.e., initial state,
1/√
2(|1/2, 1/2〉+eiθ|1/2,−1/2〉)Kγ(|α〉+eiγ |−α〉), where Kγ is the normalization
constant. We obtain only odd revivals in the four special cases, γ = 0 or π and
θ + θα = 0 or π (θα is the phase of the coherent state, i.e., α = |α|eiθα). We also
find that the revival time for γ = 0 or π, is only one half of the revival time for
γ = π/2.
Also, we consider collapses and revival in the interaction of (i) two two-level
atoms with even and odd coherent states and (ii) for initial state 1/√
2(|1, 1〉 +
eiθ|1,−1〉)Kγ(|α〉 + eiγ | − α〉), where Kγ is the normalization constant. We get
oscillations with mean frequencies 2g√
n̄ and 4g√
n̄. We find that the collapse and
revival times for even and odd coherent states are only one half of the corresponding
times for coherent state. For the state |1, 0〉 interacting with even and odd coherent
state of radiation, only mean frequency 4g√
n̄ is obtained and oscillations occur
with large amplitude. For atoms initially in states 1/√
2(|1, 1〉+eiθ|1,−1〉)Kγ(|α〉+eiγ | −α〉), weak double frequency revivals are seen to occur if θ + 2θα 6= π at times
midway between the main revivals. We find that the amplitude of oscillations of
double frequency revival depends on the value of θ+2θα. It is largest for θ+2θα = 0
and disappears for θ + 2θα = π.
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Collapses and Revivals in Two-Level Atoms 2727
In Secs. 2 and 3, we study collapses and revivals for a single two-level atom and
for two two-level atoms in superposed states, respectively, interacting with a single
mode superposed coherent state. In Sec. 4, we discuss our results.
2. Collapses and Revivals in a Single Two-Level Atom in
Superposed State Interacting with a Single-Mode Superposed
Coherent Radiation
For a single two-level atom interacting with a single mode coherent radiation, the
Hamiltonian43,44 is
H = H0 + HI , H0 = HF + HA , (1a, b)
HF = ω0N , HA = ω0Sz , HI = g(aS+ + a+S−) , N = a+a , (2a, b, c)
where subscripts F, A, and I refer to field, atoms, and interaction; N , a and a+
are number, annihilation, and creation operators for radiation, respectively, g is the
coupling constant and S±,z are the Dicke’s collective atom operators44 and ω0 is
the common atomic and radiation frequency. We note that
[H0, HI] = 0 (3)
and hence the complete time evolution operator U = e−iHt can be written as
U = e−iHt = U0UI , U0 = e−iH0t , UI = e−iHt
I (4)
where UI is the time evolution operator in the interaction picture and may be
written as45–47
UI = exp(−iHIt) =
cos gt√
N + 1 −iasin gt
√N√
N
−ia +sin gt
√N + 1√
Ncos gt
√N
. (5)
Let us consider the initial state,
1√2
(∣
∣
∣
∣
1
2,1
2
⟩
+ eiθ
∣
∣
∣
∣
1
2,−1
2
⟩)
Kγ(|α〉 + eiγ | − α) , (6)
where
Kγ =1
√
2(1 + cos γe−2n̄)(7)
is the normalization constant. For γ = 0 or π, the state Kγ(|α〉+eiγ |−α〉) becomes
even or odd coherent state, respectively.
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2728 H. Prakash & R. Kumar
Using Eqs. (5)–(7) the atomic inversion is given by
〈Sz〉 =e−n̄
4(1 + cos γe−2n̄)
∞∑
n=0
n̄n
n![1 + cos γ(−1)n]
×[
cos 2√
n + 1 gt − cos 2√
n gt + 2 sin(θ + θα)sin 2
√n + 1 gt√
n + 1. (8)
Equation (8) can be broken into two parts and written as
〈Sz〉 = 〈Sz1〉 + sin(θ + θα)〈Sz2〉 , (9)
where
〈Sz1〉 =e−n̄
4(1 + cos γe−2n̄)
∞∑
n=0
n̄n
n![1 + cos γ(−1)n][cos 2
√n + 1 gt − cos 2
√n gt] ,
(10)
〈Sz2〉 =e−n̄
2(1 + cos γe−2n̄)
∞∑
n=0
n̄n
n![1 + cos γ(−1)n]
[
sin 2√
n + 1 gt√n + 1
]
. (11)
We note that while 〈Sz1〉 is a feature in all cases, contribution of 〈Sz2〉 is propor-
tional to sin(θ+θα), and it may be zero for θ+θα = 0 or π. Dependence on γ comes
through the factor [1 + cos γe−2n̄] in the denominator and [1 + cos γ(−1)n] in the
numerator in the summation over n. Since for practical cases of interest, n̄ � 1 and
one may take e−2n̄ ∼= 0 and the factor [1 + cos γe−2n̄] in the denominator becomes
inconsequential.
For γ = 0 or π (i.e., cos γ = 1 or −1 which correspond to the even or odd
coherent states, respectively), summation is over even or odd terms only. It is
seen that in both cases there is no material difference in the envelope, and the
characteristics are rather decided by the fact that the values of n increase in intervals
of two.
Thus, for even and odd coherent states (γ = 0 or π, respectively), 〈Sz1〉 gives
revivals when, for n close to n̄, all terms cos(2√
n + 1 gt) in Eq. (10) contribute in
phase to each other and out of phase to cos(2√
n gt) terms. Thus, we should have all
terms cos(2√
n gt) in Eq. (10) with even n contributing in the same phase and out
of phase to all terms cos(2√
ngt) with n odd. This happens when 2gt√
n̄ + r + 1−2gt
√n̄ + r = (2m+1)π, or gt = gtrevival = (2m+1)π
√n̄, m = 1, 2, . . . which shows
that only odd revivals occur. These odd revivals of 〈Sz1〉 are shown in Fig. 1 the
case, for n̄ = 64, which gives gtrevival = (2m + 1)8π, i.e., odd multiples of 25.12.
For even or odd coherent state (γ = 0 or π, respectively), 〈Sz2〉 gives revivals
when all terms sin(2√
n + 1 gt) in Eq. (11) contribute in phase. Since in the sum-
mation over n, n increases by two, this demands
2gt√
n̄ + r + 2 − 2gt√
n̄ + r = 2mπ
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Collapses and Revivals in Two-Level Atoms 2729
Fig. 1. Variation of 〈Sz1〉 with coupling time gt for (Kγ/√
2)(|1/2, 1/2〉 + eiθ |1/2,−1/2〉)(|α〉 +eiγ | − α〉) (similar envelope for γ = π).
Fig. 2. Variation of 〈Sz2〉 with coupling time gt for (Kγ/√
2)(|1/2, 1/2〉 + eiθ |1/2,−1/2〉)(|α〉 +eiγ | − α〉) (similar envelope for γ = π).
or
gt = gtrevival = mπ√
n̄ ,
which shows all revivals. The revivals of 〈Sz2〉 are shown in Fig. 2 for the typical
case, n̄ = 64, and revivals are seen to occur at gt = 25.12, 50.24, etc. Since 〈Sz〉 =
〈Sz1〉 + sin(θ + θα)〈Sz2〉, for θ + θα = 0 and π, 〈Sz〉 = 〈Sz1〉 and only odd revivals
are seen which have been shown in Fig. 1 and revivals seen at gt = 25.12, 75.36,
etc. Variation 〈Sz〉 = 〈Sz1〉 + 〈Sz2〉 with gt, for θ + θα = π/2 is shown in Fig. 3.
The variation for θ + θα = −π/2 also gives a similar envelope.
For γ = π/2, consider 〈Sz1〉 first. Here, summation in Eq. (10) runs over all
integral values of n. At time gt = (2m+1)π√
n̄, according to what we discussed for
the case γ = 0 or π, terms cos(2√
n gt) contribute in one phase for n even and out
of phase with terms for n odd. For γ = π/2, therefore, the cos(2√
n + 1 gt) term
tends to cancel with cos(2√
n gt) term for each value of n. Hence, we get revivals
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2730 H. Prakash & R. Kumar
Fig. 3. Variation of 〈Sz〉 with coupling time gt for (Kγ/√
2)(|1/2, 1/2〉 + eiθ |1/2,−1/2〉)(|α〉 +eiγ | − α〉) for (γ, θ + θα) = (0, π/2) (similar envelope are seem for all four cases (γ, θ + θα) =(0,±π/2) and (π,±π/2)).
only at gt = 2mπ√
n̄ at which these two terms have phase difference 2π and hence
support each other. For 〈Sz2〉, similarly, all terms contribute in phase only when,
2gt√
n̄ + r + 1 − 2gt√
n̄ + r = 2mπ or gt = gtrevival = 2mπ√
n̄ .
Thus, for both 〈Sz1〉 and 〈Sz2〉, and therefore, 〈Sz〉 = 〈Sz1〉 + sin(θ + θα)〈Sz2〉,revival time is (2π
√n̄/g) which is double of the earlier obtained revival time π
√n̄/g
for γ = 0 and π. These revivals are shown in Fig. 4 and for θ+θα = π/2 and n̄ = 64.
Revivals are seen to occur at gt = 2mπ√
n̄ = 16mπ = 50.4× m.
The cases for γ = ±π/2 and θ + θα = 0 or π have an additional feature in that
a node occurs at the exact revivals (see Fig. 5). Occurrence of a node in the middle
of revivals, i.e., at gt = 2mπ√
n̄ exactly, for the cases γ = π/2 and θ + θα = 0 or
π (see Fig. 5) can be explained by combining the two cosine terms. We can write
Fig. 4. Variation of 〈Sz〉 with coupling time gt for (Kγ/√
2)(|1/2, 1/2〉 + eiθ |1/2,−1/2〉)(|α〉 +eiγ | − α〉) (similar envelope for θ + θα = −π/2).
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Collapses and Revivals in Two-Level Atoms 2731
Fig. 5. Variation of 〈Sz1〉 with coupling time gt for (Kγ/√
2)(|1/2, 1/2〉 + eiθ |1/2,−1/2〉)(|α〉 +eiγ | − α〉) (similar envelope for θ + θα = π).
〈Sz〉 = 〈Sz1〉 and, for terms with n ∼= n̄, i.e., for the terms that matter, the pairs of
two cosine terms in square brackets in Eq. (10) are of the form
cos 2√
n + r + 1 gt − cos 2√
n + r gt
= cos 2√
n̄
(
1 +r + 1
2n̄
)
gt − cos 2√
n̄(
1 +r
2n̄
)
gt
= sin n̄
(
2 +2r + 1
2√
n̄
)
gt singt
2√
n̄,
which vanishes at exact revival times gt = 2mπ√
n̄. This explains the appearance
of nodes.
3. Collapses and Revivals in Two Two-Level Atoms in Superposed
State Interacting with a Single-Mode Superposed Coherent
Radiation
The time evolution operator for two two-level atoms in the form48 is
UI =exp(−iHIt) =
1 + (N + 1)C(N + 1) −iS(N + 1)a C(N + 1)a2
−ia+S(N + 1) cos(gt√
4N + 2) −iS(N)a
a+2C(N + 1) −ia+S(N) 1 + NC(N − 1)
,
(12)
N = a+a, and functions C(N) and S(N) are defined as
C(N) = [cos(√
4N + 2 gt) − 1]/(2N + 1) ,
S(N) = [sin(√
4N + 2 gt)]/√
(2N + 1) .(13)
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2732 H. Prakash & R. Kumar
For a system of two two-level atoms in the states |1, 1〉, |1,−1〉, and |1, 0〉 inter-
acting with coherent radiation, it is seen that
〈Sz〉 = e−n̄
∞∑
n=0
n̄n
n![{1 + (n + 1)C(n + 1)}2 − (n + 1)(n + 2){C(n + 1)}2] , (14)
〈Sz〉 = e−n̄
∞∑
n=0
n̄n
n![{n̄C(n + 1)}2 − {1 + nC(n − 1)}2] , (15)
and
〈Sz〉 = e−n̄
∞∑
n=0
n̄n
n![{√
n̄ S(n + 1)}2 − {√
n + 1 S(n)}2] , (16)
respectively.
It has been seen that38,39 the |1,±1〉 give stronger Rabi oscillations with Rabi
frequencies 2g√
n together with weak oscillations with double frequencies 4g√
n.
Revival times for mean frequencies 2g√
n̄ and 4g√
n̄ are 2π√
n̄/g and π√
n̄/g,
respectively. For the state |1, 0〉, however, oscillations with frequency 2g√
n̄ are
suppressed as is clear from Eq. (16) which involves only S2 terms and no S terms.
Behavior of initial states |1, 1〉 and |1, 0〉 are shown in Figs. 6 and 7. State |1,−1〉gives an envelope for collapse and revivals similar to that |1, 1〉.
From Eqs. (14)–(16) and definition Eq. (13), we note the features:
(i) appearance of non-zero average value terms in 〈Sz〉 for the state |1, 0〉, which
is small and becomes noticeable for this state [see Eq. (16)] where amplitude of
oscillations and revivals are small (see, e.g., Fig. 7), and appearance of collapse and
revivals (ii) for mean frequency 2g√
n̄ (for the states |1,±1〉) as well as (iii) for the
mean frequency 4g√
n̄ (for the states |1,±1〉 and |1, 0〉).Revival times of mean Rabi frequencies 2g
√n̄ and 4g
√n̄ for the initial states
|1,±1〉 can be evaluated by considering reinforcement of terms of the form
Fig. 6. Variation of 〈Sz〉 with coupling time gt for |1, 1〉|α〉 (similar envelope for |1,−1〉|α〉).
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Collapses and Revivals in Two-Level Atoms 2733
Fig. 7. Variation of 〈Sz〉 with coupling time gt for |1, 0〉|α〉.
cos gt√
4n + 2 and cos 2gt√
4n + 2 in 〈Sz〉, respectively. Former (oscillation with
mean frequency 2g√
n̄) gives revivals at gt√
4n̄ + 4r + 6 − gt√
4n̄ + 4r + 2 = 2mπ,
which gives, gtrevival = 2mπ√
n̄, m = 1, 2, . . . .
For latter (oscillations with mean frequency 4g√
n̄) similarly, we get
2gt√
4n̄ + 4r + 6 − 2gt√
4n̄ + 4r + 2 = 2mπ, which leads to gtrevival = mπ√
n̄.
Now, consider initial states |1, 1〉K±(|α〉 ± | − α〉), |1,−1〉K±(|α〉 ± | − α〉), and
|1, 0〉K±(|α〉 ± | − α〉), which leads to
〈Sz〉 = 2K2±e−n̄
∞∑
n=0
n̄n
n![1 ± (−1)n][{1 + (n + 1)C(n + 1)}2
− (n + 1)(n + 2){C(n + 1)}2] , (17)
〈Sz〉 = 2K2±e−n̄
∞∑
n=0
n̄n
n![1 ± (−1)n][{n̄C(n + 1)}2 − {1 + nC(n − 1)}2] , (18)
and
〈Sz〉 = 2K2±e−n̄
∞∑
n=0
n̄n
n![1 ± (−1)n][{
√n̄ S(n + 1)}2 − {
√n + 1S(n)}2] , (19)
respectively, with K± = K0,π and Kγ = 1/√
2(1 + cos γe−2n̄) [see Eq. (7)].
We find that the collapse and revival times for the case of even and odd coherent
states are only one half of the corresponding times for coherent state. It is clear from
a comparison of Figs. 8 and 9 with Figs. 6 and 7. This happens because summation
over n is for values at interval of 2. Revival times for mean frequency 2g√
n̄ (usual
revivals) can be estimated for the state |1, 1〉K±(|α〉 ± | − α〉) using Eq. (17) by
writing gt√
4n̄ + 4r + 14 − gt√
4n̄ + 4r + 6 = 2mπ, which gives, gtrevival = mπ√
n̄,
m = 1, 2, . . . . For revivals of mean frequency 4g√
n̄ (double frequency revivals), we
have 2gt√
4n̄ + 4r + 10 − 2gt√
4n̄ + 4r + 6 = 2mπ, or gtrevival = mπ√
n̄/2. We can
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2734 H. Prakash & R. Kumar
Fig. 8. Variation of 〈Sz〉 with coupling time gt for K+|1, 1〉(|α〉 + | − α〉) (similar envelope forK−|1, 1〉(|α〉 − | − α〉) and K±|1,−1〉(|α〉 ± | − α〉)).
Fig. 9. Variation of 〈Sz〉 with coupling time gt K+|1, 0〉(|α〉 + | − α〉) (similar envelope forK−|1, 0〉(|α〉 − | − α〉)).
find revival times for the state |1,−1〉K±(|α〉±|−α〉) similarly, and obtain identical
results.
Revival time for the state |1, 0〉K±(|α〉 ± | − α〉), where we have only the mean
frequency 4g√
n̄, can be found using Eq. (19) and demanding that the two cosine
terms are out of phase. This leads to
2gt√
4n̄ + 4r + 6 − 2gt√
4n̄ + 4r + 2 = (2m + 1)π ,
or
gtrevival =1
2(2m + 1)π
√n̄ .
That is, only odd revivals occurs (see Fig. 9). We also note the fact that amplitude
of oscillations at the mean frequency 4g√
n̄ (which is the only mean frequency here)
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Collapses and Revivals in Two-Level Atoms 2735
is large unlike the previous cases of atomic states |1,±1〉. This can be easily seen
from Eq. (19) by writing the oscillating terms in 〈Sz〉 as
1
2K2
±e−n̄
∞∑
n=0
n̄n
n![1 ± (−1)n]
×[
− n̄
2n + 3cos(2
√4n + 6 gt) +
n + 1
2n + 1cos(2
√4n + 2 gt) . (20)
Let us now consider the collapses and revivals for the initial state, (1/√
2)(|1, 1〉+eiθ|1,−1〉)Kγ(|α〉 + eiγ | − α〉. Straight calculations lead to
〈Sz〉 =e−n̄
2(1 + cos γe−2n̄)
∞∑
n=0
n̄n
n![1 + cos γ(−1)n][2{(n + 1)C(n + 1)}− n{C(n − 1)}
−{n̄2 − n − 1 − 2n̄ cos(θ + 2θα)}{C(n + 1)}2 − {nC(n − 1)}2] . (21)
We can separate the terms involving C(n) and (C(n))2 and write
〈Sz〉 = 〈Sz1〉 + 〈Sz2〉 , (22)
where
〈Sz1〉=e−n̄
(1 + cos γe−2n̄)
∞∑
n=0
n̄n
n![1 + cos γ(−1)n][{(n + 1)C(n + 1)}− n{C(n − 1)}] ,
(23)
〈Sz2〉 =e−n̄
2(1 + cos γe−2n̄)
∞∑
n=0
n̄n
n![1 + cos γ(−1)n]
× [{n̄2 − n − 1 − 2n̄ cos(θ + 2θα)}{C(n + 1)}2 − {nC(n − 1)}2] , (24)
and C(n) is defined by Eq. (13). We see that 〈Sz1〉 gives Rabi oscillations with mean
frequency 2g√
n̄, while 〈Sz2〉 gives Rabi oscillations with double mean frequency
4g√
n̄. These revivals occur at multiples of gt = 25.12 and gt = 12.56 as shown in
Figs. 10 and 11, respectively. We also see the interesting behavior that for 〈Sz1〉,a node occurs at the center of each revival and, for small gt, the amplitude of
oscillations first increases from zero to a maximum and then collapses.
For all values of γ 6= π/2 in summation, values of n change by 2 and hence
revivals for mean frequency 2g√
n̄ occur when gt√
4n̄ + 4r + 14−gt√
4n̄ + 4r + 6 =
2mπ, which gives, gtrevival = mπ√
n̄. For n̄ = 64, revivals are seen to occur at
coupling times which are multiples of π√
n̄ = 25.12 (see Fig. 12).
For γ = π/2, values of n change by one in summation over n and hence revivals
occur when gt√
4n̄ + 4r + 10− gt√
4n̄ + 4r + 6 = 2mπ, giving, gtrevival = 2mπ√
n̄,
and hence for n̄ = 64, revivals occur at coupling times which are multiples of
2π√
n̄ = 50.24 (see Fig. 13).
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2736 H. Prakash & R. Kumar
Fig. 10. Variation of 〈Sz1〉 with coupling gt for (Kγ/√
2)(|1, 1〉 + eiθ |1,−1〉)(|α〉 + eiγ | − α〉)(similar envelope for γ = π).
Fig. 11. Variation of 〈Sz2〉 with coupling time gt for (Kγ/√
2)(|1, 1〉+eiθ |1,−1〉)(|α〉+eiγ |−α〉)(similar envelope for γ = π).
Fig. 12. Variation of 〈Sz〉 with coupling time gt for (Kγ/√
2)(|1, 1〉+ eiθ |1,−1〉)(|α〉+ eiγ | −α〉)(similar envelope for γ = π).
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Collapses and Revivals in Two-Level Atoms 2737
Fig. 13. Variation of 〈Sz〉 with coupling time gt for (Kγ/√
2)(|1, 1〉 + eiθ |1,−1〉)(α〉 + eiγ | − α〉)(similar envelope for γ = −π/2).
Occurrence of the nodes in the center of revivals of Rabi frequency 2g√
n̄, can
be understood by writing Eq. (21) as
〈Sz〉 = K2±e−n̄
∞∑
n=0
n̄n
n![1 ± (−1)n]
[
n + 1
(2n + 3)
{
cos
(
2√
n̄ +2(n − n̄) + 3
2√
n̄
)
gt
}
− n
(2n − 1)
{
cos
(
2√
n̄ +2(n − n̄) − 1
2√
n̄gt
)}]
.
Since difference of angles in two cosine terms is 2gt/√
n̄ which is a multiple of 2π
at revivals for all cases of γ, the amplitude of oscillations in 〈Sz〉 is nearly
〈Sz〉 = K2±e−n̄
∞∑
n=0
n̄n
n![1 ± (−1)n]
[
n + 1
(2n + 3)− n
(2n − 1)
]
,
≈ K2±e−n̄
∞∑
n=0
n̄n
n![1 ± (−1)n]
[
− 1
n̄
]
≈ − 1
2n̄,
which is very small.
For revivals with double frequency 4g√
n̄, we note that 〈Sz2〉 [see Eq. (24)] can
be further simplified by taking approximation, |α|2 = n̄ � 1 and, we get
〈Sz2〉 ≈e−n̄
2(1 + cos γe−2n̄)
∞∑
n=0
n̄n
n![1 + cos γ(−1)n]
× [(−n)(1 + cos(θ + 2θα))][(C(n − 1))2] . (25)
Equation (25) shows that the amplitude of double frequency revivals depend on
(1+cos(θ +2θα)). Hence, the amplitude of oscillation for double frequency revivals
is largest for θ + 2θα = 0 and disappears for θ + 2θα = π.
For 〈Sz2〉, when γ 6= π/2, values of n increase by 2 in summation and hence
revival occurs when 2gt√
4n̄ + 4r + 14−2gt√
4n̄ + 4r + 6 = 2mπ, or gt = gtrevival =
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2738 H. Prakash & R. Kumar
(mπ√
n̄/2) For n̄ = 64, the variation shown in Figs. 11 and 12 show first revival at
gt = gtrevival = (π√
n̄/2) = 12.56.
When γ = π/2, values of n increase by one in summation and hence revival occur
when 2gt√
4n̄ + 4r + 10 − 2gt√
4n̄ + 4r + 6 = 2mπ which gives, gt = gtrevival =
mπ√
n̄. For n̄ = 64, Fig. 13 shows the first revival at double frequency at gt = 25.12.
4. Conclusion and Summary
In this paper, we studied collapses and revivals of Rabi oscillations in interaction
of (i) a single two two-level atom having equal weightage of lower and upper states
and (ii) two two-level atom with radiation in superposed state ∼ (|α〉 + eiγ | − α〉).For (i), we find that only odd revivals in special cases γ = 0 or π and θ + θα = 0
or π. We also find that the time of revival for γ = 0 or π, is just one half of the
time for revival for γ = π/2. For γ = π/2 and θ + θα = 0 or π, we also note the
occurrence of nodes in the middle of revivals.
For (ii), in general, Rabi oscillation with mean frequencies 2g√
n̄ and 4g√
n̄
are obtained. For superradiant atomic state, however, the fundamental is absent
and the second harmonic has large amplitude. When radiation is in even or odd
coherent state, the collapse and revival times are exactly one half of those for a
coherent state. Revival time for second harmonic of Rabi frequency is obtained at
one half of that for Rabi frequency. The second harmonic oscillations are absent if
θ + θα = π.
Acknowledgments
We are thankful to Professors N. Chandra and R. Prakash for their interest and
critical comments, and to Dr. R. S. Singh, Dr. D. K. Singh, Dr. Pankaj Kumar,
Mr. D. K. Mishra, Mr. A. Dixit, Miss P. Shukla, Miss Shivani, Miss S. Shukla, Miss
N. Shukla and Mr. Anurag Singh for helpful and stimulating discussions. One of
the authors (HP) is grateful to Indian Space Research Organization, Bangalore for
financial support.
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