Improving Kerr QND Measurement Sensitivity via Squeezed Light Stepan Balybin1 2Dariya Salykina1 2and Farid Ya. Khalili2 1Faculty of Physics M.V.Lomonosov Moscow State University Leninskie Gory 1 Moscow 119991 Russia

2025-05-08 0 0 418.58KB 8 页 10玖币
侵权投诉
Improving Kerr QND Measurement Sensitivity via Squeezed Light
Stepan Balybin,1, 2, Dariya Salykina,1, 2 and Farid Ya. Khalili2,
1Faculty of Physics, M.V.Lomonosov Moscow State University, Leninskie Gory 1, Moscow 119991, Russia
2Russian Quantum Center, Skolkovo IC, Bolshoy Bulvar 30, bld. 1, Moscow, 121205, Russia
In Ref. [1], the scheme of quantum non-demolition measurement of optical quanta that uses a resonantly
enhanced Kerr nonlinearity in optical microresonators was analyzed theoretically. It was shown that using the
modern high-𝑄microresonators, it is possible to achieve the sensitivity several times better than the standard
quantum limit. Here we propose and analyze in detail a significantly improved version of that scheme. We show,
that by using a squeezed quantum state of the probe beam and the anti-squeezing (parametric amplification) of
this beam at the output of the microresonator, it is possible to reduce the measurement imprecision by about one
order of magnitude. The resulting sensitivity allows to generate and verify multi-photon non-Gaussian quantum
states of light, making the scheme considered here interesting for the quantum information processing tasks.
I. INTRODUCTION
An ideal quantum measurement described by von Neu-
manns reduction postulate [2] does not perturb the measured
observable 𝑁. The sufficient condition for implementation of
such a measurement is the commutativity of the operator ˆ
𝑁
with the Hamiltonian ˆ
𝐻of the combined system “measured
object+meter” [3,4]:
[ˆ
𝑁, ˆ
𝐻]=0,(1)
where
ˆ
𝐻=ˆ
𝐻𝑆+ˆ
𝐻𝐴+ˆ
𝐻𝐼,(2)
ˆ
𝐻𝑆,ˆ
𝐻𝐴are, respectively, the Hamiltonians of the object and
the meter, and ˆ
𝐻𝐼is the interaction Hamiltonian. In the article
[5], the term “quantum non-demolition (QND) measurement”
was coined for this type of measurement.
In many cases, a sequence of measurement of a variable
𝑁(𝑡)is required, instead of a single measurement. The typical
example is detection of external force acting on the object.
In this case the value of ˆ
𝑁have to be preserved between the
measurements, which leads to another (also sufficient) com-
mutativity condition:
[ˆ
𝑁, ˆ
𝐻𝑆]=0,(3)
The observables which satisfy both conditions (1) and (3) are
known as QND observables.
It follows from Eqs. (1), (3) that the interaction Hamiltonian
have to commute with the measured observable:
[ˆ
𝑁, ˆ
𝐻𝐼]=0,(4)
In the particular case of the electromagnetic energy or number
of quanta measurement, this means that nonlinear interaction
of the electromagnetic field with the meter has to be used. A
semi-gedanken example of such a measurement based on the
radiation pressure effect was considered in Ref. [6].
sn.balybin@physics.msu.ru
farit.khalili@gmail.com
Later a more practical scheme based on the cubic (Kerr) op-
tical non-linearity [7] was proposed. In this scheme, the signal
optical mode interacts with another (probe) one by means of
the optical Kerr nonlinearity. As a result, the phase of the
probe mode 𝜑𝑝is changed depending on the photon number
𝑁𝑠in the signal one (the cross phase modulation, XPM). The
subsequent interferometric measurement of this phase allows
to retrieve the value of 𝑁𝑠with the precision depending on
the initial uncertainty of 𝜑𝑝, see details in Sec. IV of Ref. [1].
In the ideal lossless case, the photon numbers in both modes
are preserved. However, due to the XPM effect, the phase of
the signal mode is perturbed proportionally to the probe mode
energy uncertainty, fulfilling thus the Heisenberg uncertainty
relation.
The natural sensitivity threshold for the QND measurement
of the number of quanta is the standard quantum limit (SQL)
Δ𝑁SQL =𝑁 , (5)
where 𝑁is the mean number of the measured quanta. It
corresponds to the best possible sensitivity of a linear non-
absorbing meter [4], for example a phase-preserving linear
amplifier [8]. Starting from the initial work [9], many proof-
of-principle experiments based on the XPM idea were done,
see the review articles [1012]. The sensitivity exceeding the
SQL was demonstrated in these experiments, but the ultimate
goal of the single-photon accuracy was not reached due to
the insufficient values of the optical nonlinearity in highly
transparent optical media.
The recent advantages in fabrication of high-𝑄monolithic
and integrated microresonators [13], which combine very low
optical losses with high concentration of the optical energy
promises the way to overcome this problem. This possibil-
ity was analyzed in detail in Ref. [1]. It was shown that the
sensitivity of the Kerr nonlinearity based QND measurement
schemes is limited by the interplay of two undesirable effects:
the optical losses and the self phase modulation (SPM) of the
probe mode, which perturbs the probe mode phase proportion-
ally to the energy uncertainty of this mode.
It was shown in Ref. [14], that in the ideal lossless case,
the SPM effect can be compensated using the measurement of
the optimal quadrature of the output probe field instead of the
phase one. However, in presence of the optical losses, only
partial compensation is possible, limiting the sensitivity by the
arXiv:2210.00857v2 [quant-ph] 14 Aug 2023
2
value
(Δ𝑁𝑠)2=1
Γ2
𝑋1
4𝜂𝑁𝑝+ (1𝜂)𝑁𝑝Γ2
𝑆,(6)
see Eq. (32) of [1]. Here Δ𝑁𝑠is the measurement error, 𝑁𝑝is
the photon number in the probe mode, Γ𝑋,Γ𝑆are the dimen-
sionless factors of, respectively, the cross and the self phase
modulation, see Eqs. (25) and (40), and 𝜂is the quantum ef-
ficiency of the measurement channel. The second term here
stems from the SPM. Due to this term, the optimal value of
𝑁𝑝exists, which provides the minimum of Δ𝑁𝑠:
(Δ𝑁𝑠)2=Γ𝑆
Γ2
𝑋
𝜖 , (7)
where
𝜖=1𝜂
𝜂(8)
is the normalized loss factor. It was shown in Ref. [1], that
using the best microresonators available now, the sensitivity
Δ𝑁𝑠102-103could be achieved.
Eqs. (6), (7) imply that the probe mode is prepared in the
coherent quantum state. At the same time, in was shown by
C.Caves in the work [15], that the sensitivity of optical inter-
ferometric measurements can be improved without increasing
the optical power by using the non-classical squeezed states
of light. Currently, this method is routinely used in the laser
gravitational-wave detectors [16,17]; see also the review [18].
In the same work [15], C. Caves proposed also to use an addi-
tional degenerate optical parametric amplifier (anti-squeezer)
at the output of the interferometer to reduce impact of the
losses in the optical elements located after this amplifier, in-
cluding the photodetector(s) inefficiency. Note that usually, it
is the output losses constitute the major part of the total losses
budget in the optical interferometers. Recently, this method
was demonstrated experimentally [19].
In the current work we show that sensitivity of the QND
measurement scheme, considered in Ref. [1], can be radically
improved using these techniques. This paper is organized
as follows. In Sec. II, we derive the linearized input/output
relations for the microresonator. In Sec.III, we calculate the
measurement error, taking into account the SPM effect and
the losses in the probe mode. In Sec. IV, we estimate the
sensitivity, which can be achieved using the best available
microresonators. In Sec. Vwe consider the effect of optical
losses in the signal mode both in the measurement and in the
quantum state preparation scenarios. In Sec. VI, we discuss
possible applications of the considered scheme to quantum
information processing. We summarize the results of this
paper in Sec. VII.
FIG. 1. The scheme of the QND measurement of the photon number
in signal mode via XPM effect. DOPA: degenerate optical parametric
amplifier, HD: homodyne detector.
II. EVOLUTION OF THE OPTICAL FIELDS IN THE
MICRORESONATOR
The measurement scheme is shown in Fig. 1. Here the
strong coherent beam is split by the unbalanced beamsplitter
with the transmissivity 𝑇1 into the probe and the reference
beams. The probe beam is squeezed by the degenerate op-
tical parametric amplifier DOPA 1 and then injected into the
microresonator. There it interacts with the signal beam and
then passes through the second optical parametric amplifier
DOPA 2 and finally is recombined with the reference beam in
the homodyne detector.
Taking into account that the main goal of this paper is to
show the advantages provided by the squeezing, and in or-
der to simplify the calculations, we, similar to the paper [1],
do not take into account explicitly the optical losses in the
microresonator, but assume instead that
𝑄load
𝑄intr 𝜏
𝜏𝜖2,(9)
where 𝑄load is the loaded quality factor, 𝑄intr is the intinsic
one, 𝜏is the interaction time, and 𝜏is the relaxation time of
the microresonator.
In this case, the interaction of the signal and probe modes
in the non-linear microresonator can be described by the fol-
lowing Hamiltonian [1]:
ˆ
𝐻=
𝑥=𝑝,𝑠 𝜔𝑥ˆ
𝑁𝑥𝛾𝑆
2ˆ
𝑁𝑥(ˆ
𝑁𝑥1)𝛾𝑋ˆ
𝑁𝑝ˆ
𝑁𝑠,(10)
where
ˆ
𝑁𝑝,𝑠 =ˆ𝑎
𝑝,𝑠 ˆ𝑎𝑝,𝑠 (11)
are the photon number operators in the probe and signal modes,
respectively, ˆ𝑎𝑝,𝑠, ˆ𝑎
𝑝,𝑠 are the corresponding annihilation and
creation operators for these modes, 𝜔𝑠, 𝑝 are their frequen-
cies, 𝛾𝑆,𝛾𝑋— coefficients of SPM and XPM interactions,
摘要:

ImprovingKerrQNDMeasurementSensitivityviaSqueezedLightStepanBalybin,1,2,∗DariyaSalykina,1,2andFaridYa.Khalili2,†1FacultyofPhysics,M.V.LomonosovMoscowStateUniversity,LeninskieGory1,Moscow119991,Russia2RussianQuantumCenter,SkolkovoIC,BolshoyBulvar30,bld.1,Moscow,121205,RussiaInRef.[1],theschemeofquant...

展开>> 收起<<
Improving Kerr QND Measurement Sensitivity via Squeezed Light Stepan Balybin1 2Dariya Salykina1 2and Farid Ya. Khalili2 1Faculty of Physics M.V.Lomonosov Moscow State University Leninskie Gory 1 Moscow 119991 Russia.pdf

共8页,预览2页

还剩页未读, 继续阅读

声明:本站为文档C2C交易模式,即用户上传的文档直接被用户下载,本站只是中间服务平台,本站所有文档下载所得的收益归上传人(含作者)所有。玖贝云文库仅提供信息存储空间,仅对用户上传内容的表现方式做保护处理,对上载内容本身不做任何修改或编辑。若文档所含内容侵犯了您的版权或隐私,请立即通知玖贝云文库,我们立即给予删除!
分类:图书资源 价格:10玖币 属性:8 页 大小:418.58KB 格式:PDF 时间:2025-05-08

开通VIP享超值会员特权

  • 多端同步记录
  • 高速下载文档
  • 免费文档工具
  • 分享文档赚钱
  • 每日登录抽奖
  • 优质衍生服务
/ 8
客服
关注