
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-
mann’s 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 [10–12]. 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