A model of a single-mode field, initially prepared in a coherent state, coupled to a two-level atom surrounded by a nonlinear Kerr-like medium contained inside a very good quality cavity is considered. We derive the photon number-phase uncertainty relation in the evolution of the field for a weak and strong nonlinear coupling respectively, within the Hermitian phase operator formalism of Pegg and Barnett, and discuss the effects of nonlinear coupling of the Kerr-like medium on photon number-phase uncertainty relation of the field

Fan, An-Fu

Sun, Nian-Chun

English

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/ /
Photon number-phase uncertainty relation
in the evolution of the field in a Kerr-like medium
Fan An-fu
Department of Opto-electronics Science and Technology,
Sichuan University, Chengdu 610064, China
and
China Center of Advanced Science and Technology(World Laboratory),
P. O. Box 8730, Beijin9 100080, China
Sun Nian-Chun
Southwest Institute of Technical Physics Chengdu, 610041, China
Abstract
A model of a single-mode field, initially prepared in a coherent state, coupled to a two-level
atom surrounded by a nonlinear Kerr-like medium contained inside a very good quality cavity
is considered. We derive the photon number-phase uncertainty relation in the evolution of
the field for a weak and strong nonlinear coupling respectively, within the Hermitian phase
operator formalism of Pegg and Barnett, and discuss the effects of nonlinear coupling of thr
Kerr-like medium on photon number-phase uncertainty relation of the field.
1 Introduction
Recently, Agarwal et al[1] have considered the propagation of a single-mode resonant field through
a nonlinear Kerr-medium. Bu_ek et al[2] have dealed with a combination of two models: the
Jaynes-Cummings model (JCM) describing the interaction of a single-mode cavity field with a
single two-level atom, and a nonlinear Kerr-like medium inside a cavity which may be modelled
by an anharrnonic oscillator[I,3]. Particularly, they have showed that with increasing nonlinear
coupling the period between the revivals of the atomic inversion is shortened and its time evolution
becomes more regular. Besides, they also described the squeezing of the cavity mode and the time
evolution of the photon-number distribution.
As is well-known, the phase properties of light field is very important in quantum optics. Lately,
Pegg and Barnett[4-6] have shown that an Hermitian phase operator of radiation field exists. It
can be constructed from the phase states. This new phase operator formalism makes it possible
to describe the quantum properties of optical phase in a fully quantum mechanics. Gerry['/'] has
studied the phase fluctuations of coherent light interacting with the anharmonic oscillator using
the Hermitian phase operator. Gantsog et al[8,9] have studied the phase properties of self-squeezed
states generated by the anharmonic oscillator, elliptically polarized light propagating through a
Kerr medium and a damped anharmonic oscillator using the Hermitian phase operator.
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https://ntrs.nasa.gov/search.jsp?R=19960025071 2020-06-16T04:04:46+00:00Z
In this paper we consider a generalized JCM with an additional Kerr-like medium, namely, a
combined model that comprises the JCM and the anharmonic oscillator model (AOM) used to
describe a Kerr medium. We deal with not only the field-Kerr medium interaction, but also the
field-atom interaction. We derive the photon number-phase uncertainty relation in the evolution
of the field for a weak and strong nonlinear coupling respectively, within the Hermitian phase
operator formalism of Pegg and Barnett, and discuss the effects of nonlinear coupling of the Kerr
medium on the number-phase uncertainty relation of the field.
2 The model
We consider a model which consists of a single two-level atom surrounded by a nonlinear Kerr-like
medium contained in a high-Q single-mode cavity. The cavity mode is coupled to the Kerr-like
medium as well as to the two-level atom. The Kerr-like medium can be modelled as an anharmonic
oscillator [1,3]. In the adiabatic limit, the effective Hamiltonian of the system involving only the
photon and atomic operators in rotating-wave approximation, is[l,2!
1
H_I ! = tu_(a+a + -_) + tU_oS z + hxa+2a 2 + hg(S+a + a+S-), (2.1)
where a and a + are the annihilation and creation opreators of the field mode, S* and S = are the
spin-flip and inversion operators of the atom respectively, g is the field-atom coupling constant
and X describes the strength of the quadratic nonlinearity modelling the Kerr medium, w0 is the
frequency of the atomic transition, the frequency w is
w = w! - Az/(wk -- Wl), (2.2)
Where w I and wk are the fi'equency of the field mode and the anharmonic oscillator modelling the
Kerr medium respectively, and A is the field-Kerr medium coupling constant.
To isolate the effects of the nonlinear coupling of the Kerr medium from that of the finite
detuning, we restrict in the case of the resonance (i.e.,w0 = w). Let us assume that the atom is
initially in the excited state [e > and the field mode is prepared in a coherent state la >. The
initial state vector [¢(0) > of the system is
oo
I¢(0) >= la > ®le >= b, e"'3ln,e >, (2.3)
n----0
b,, = exp(-f_/2)(fi'*/n!) 1/2.
where
(2.4)
In the interaction picture, the state vector of the system at a later time t is found from the
Hamiltonian (2.1) to be
b ei"ae -i×'h ,;r_,-.or1 o _ .2xn 1
I¢(t) >= z., ,, "tt '°k2'*"nX + z-fl-_.xsin(_fl,_xt)]ln, e >
r_----O
2gv_+ 1 1
z' fl,_x sin(2fl'_xt) In + 1 , g > }, (2.5)
582
where Ig > is the ground state of the atom, fl.x is the generalized Rabi frequency defined by
fl, x = [492(n + 1) + 4x_n2] '/2, (2.6)
It is obvious that, for X = 0, the state vector [¢(t) > given by Eq.(2.5) describes the dynamics of
the ordinary JCM.
3 The phase variance of the cavity field
Based on the Hermitian phase formalism of Pegg and Barnett[4-6], The complete set of s + 1
orthonormal phase state is defined by
1
10,, >= _ __oexp(inO_)ln >, (3.1)
where 0,, = Oo+27rrn/(s+ 1), m = 0, 1, 2,..., s, and 0m is an arbitrary real number. The Hermitian
phase operator is given by
a
'_o---- _ 0,_10,_ >< 0,_], (3.2)
rn----O
Clearly, phase state [0m > are eigenstates of _0 with the eigenvalues 0,,. The eigenvalues 0m are
restricted to lie within a phase window between 00 and (00 + 27r). It has to be noted That, after
all expectation values of the phase variables associated with the phase properties of the field have
been calculated in the finite (s + 1)-dimensional space, s is allowed to tend to infinity. The phase
distribution of the state given by Eq.(2.5) is
p(O,,,t) = [< 0role(t) > Is, (3.3)
with the expectation value and the variance
< _o >= _ O,,P(O,_,t), (3.4)
< A(i,_ >= _(0m- < _o >)2P(O,,,t). (3.5)
We choose the reference phase 00 =/3- 7rs/(s + 1), and introduce a new phase label # = rn- s/2,
which goes in integer steps from (-s/2) to (s/2). Then the phase distribution becomes symmetric
in #. In the limit as s tends to infinity, the continuous phase variable can be introduced replacing
#2rc/(s + 1) by 0 and 21r/(s + 1) by dO. Then we can find a continuous phase distribution
where
1
P(O,t) = _--_{1 + 2 _ b,,bw[A..¢cos[(n- n')O + (n 2 - na)xt]
+B,,., sin[(n - n')O + (n 2 - n2)xt]]},
492_(n + 1)(n' + 1) + 4x2nn '
1A,,, = cos(gt,_×t) cos(_g_,_,×t) + sin(_nxt) sin(_n'xt)
(3.6)
583
. 1
B.., = (2X./_x) sm(_D...xtlcos(1C_,xt) _ (2X.,/C_,x)cos(l f1_xtl .sm(_f_,xt1.1
The function P(0, t) is normalized so that
(3.7)
/: P(O, tldO = 1.
It
(3.81
If the mean photon number in the field is large, fi >> 1, the coefficient bn in Eq.(2.4) can be well
approximated by a continuous Gaussian distribution
bn = (2n'fi)-U' exp[-(_ - n)_14,_]. (3.9)
If Eq. (3,9) is substituted into Eq.(3.6) and the summation in Eq. (3.6) is replaced by an appropriate
integral over the variable n, one can appraximately work the phase distribution.
We will consider two limit cases:
(1)The weak nonlinear coupling which is defined by the condition g2fi >> X2fi2, with fi >> 1.
In this case the generalized Rabi frequency can be approximated as
1
a.,,,_.gl(n),/2+.(n)-,/_](1+ _), (3.101
where
Then using Eqs.(3,9) and (3.10)
integral over n, we obtain
cx = (X2n2192fi) U2" (3.11)
and replacing the summation in Eq.(3.6) by an appropriate
I 2_'fi 12
P(O,t) = _-_r(1+ 16fi2xZt2 • {(1 + Cx)exp[ 2F_ [2nxt + (0 2g_/._)21]I + 16fi2x2t 2
_+(1-¢x)exp[ 1 + 16fi2X2t 2[2nXt+(O+ )211}. (3.12)
According to Eqs.(3.4) and (3.5), using Eq.(3.121, and taking into account 0m = 0 + 8, we can
directly find an expectation value of the phase operator and its variance
gt
< C0 >= _ + ex';-'__ (1 - 4flex), (3.13)
-iVn
1 (gt) 2 , 16_2x1. (3.141< a_] >= _ +-_-(l +
(2)The strong nonlinear coupling which is defined by the condition g2fi << X2fi2, with fi >> 1.
In this case the generalized P_bi frequency can be approximated as
12
n,= _ 2Xfi(1 + _e,), (3.15)
where
6, = (g2n/x2n2)_/2. (3.16)
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Then, we find
2fi
P(a,t) = (8¢n)'/22,r(1+ lOn2x2t2)-1/2exp[- 1+ 16_2x2t2(O+ 2_) 2] (3.17)
< 6, >=/_- 2fiXt, (3.18)
1
< A&_ >= _ + 4fi(xt) 2. (3.19)
We see that the average value of the phase is not equal to the initial quantity/_, and the
phase variance is always enhanced. For the weak nonliner coupling, the enhancement of the phase
variance is proportional to (gt)2/4_, this is similar to that of the resonance field in coherent state
JCM[10]. For the strong nonlinear coupling, the enhancement of the phase variance is proportional
to 4fi(xt) 2. Obviously, the enhancement of the phase variance in the strong nonlinear coupling
case is larger than that in the weak nonlinear coupling case.
4 The number-phase uncertainty relation
It is not difficult to calculate the variance of the photon-number for the state given by Eq.(2.5).
Using h = a+a, for the weak nonlinear coupling we obtain
< (Ah) 2 >=< h2 > - < h >2_ fi+ V_gtexp[_(gt)2/2]sin(2v/_gt). (4.1)
_From Eqs.(3.14) and (4.1),we findthat the number-phase uncertainty relationis
i 4 lO_ 2 16v_gt6_exp[-(gt)2/2]sin(2J'_gt)}. (4.2)< (A_)2>< A_2 >_ _+ (_)2{i+ +
For the strong nonlinear coupling, we find
< (Ah)2 >_ n + 2nxte2exp[-2_(xt)2]sin(2nxt), (4.3)
1
< (A_)2>< z_&2>_ _ + 4n2(xt)2(1+ 2Xte2exp[_2_Cxt)2]sin(2_xt)}. (4.4)
We see that, the uncertainty product during the evolution is expanded. The expansion of the
uncertainty product is fast in strong nonlinear coupling case. This is similar to that of the
self-squeezed state generated by the anharmonic oscillator[8]. This occurs because both the field-
atom interaction[11] and the field-Kerr medium interaction are nonlinear, moreover the nonlinear
interaction strength of the latter is larger than that of the former.
5 Summary
In the present paper we consider a generalized JCM in the presence an additional Kerr-like
medium, we have derived the photon munber-phase uncertainty relation in the evolution of a
resonant field for a weak mid strong nonlinear coupling, within the Hermitian phase operator
$8$
formalism of Pegg and Barnett. We have shown that the nonlinear coupling of the cavity mode to
Kerr-like medium leads to the enhancement of the phase variance of the field and the expansion of
the uncertainty product. Particularly, the expansion of the uncertainty product is fast in strong
nonlinear coupling case. We have indicated that this is similar to that of the self-squeezed state
generated by the anharmonic oscillator. We have also indicated that the nonlinear interaction
strength of the field-Kerr medium is larger than that of the field-atom.
Acknowledgments
This work is supported by the National Natural Science Foundation of China.
References
[1] G.S.Agarwal and R.R.Puri, Phys.Rev.A39, 2969(1989).
[2] V.Bu_ek and I.Jex, Optics Comm.78, 125(1990).
[3] B.Yurke and D.Stoler, Phys.Rev.Lett.57, 13(1986).
[4] D.T.Pegg and S.M.Barnett, Europhys Lett.6, 483(1988).
[5] S.M.Barnett and D.T.Pegg, J.Mod.Opt.36, 7(1989).
[6] D.T.Pegg and S.M.Barnett, Phys.Rev.A39, 1965(1989).
[7] C.C.Gerry, Optics Comm.75, 168(1990).
[8] Ts.Gantsog and R. Tana_, J.Mod. Opt.38, 1021(1991);ibid,38, 1537(1991).
[9] Ts.Gantsog and Tana§, Phys.Rev.A44, 2086(1991).
[10] A.F.Fan, Optics Comm.98,340(1993).
[11] A.F.Fan, Z.W.Wang mid N.C.Sun, Acta Phys.Sin.44, 536(1995).
586


Photon Number-Phase Uncertainty Relation in the Evolution of the Field in a Kerr-Like Medium

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