of 8
Article
https://doi.org/10.1038/s41467-023-38191-4
Quantum microscopy of cells at the
Heisenberg limit
Zhe He
1,2
, Yide Zhang
1,2
, Xin Tong
1,2
,LeiLi
1
& Lihong V. Wang
1
Entangled biphoton sources exhibit non
classical characteristics and have been
applied to imaging techniques such as
ghost imaging, quantum holography,
and quantum optical coherence tomography. The development of wide-
fi
eld
quantum imaging to date has been hindere
dbylowspatialresolutions,speeds,
and contrast-to-noise ratios (CNRs). H
ere, we present quantum microscopy by
coincidence (QMC) with balanced pa
thlengths, which enables super-
resolution imaging at the Heisenberg limit with substantially higher speeds
and CNRs than existing wide-
fi
eld quantum imaging methods. QMC bene
fi
ts
from a con
fi
guration with balanced pathleng
ths, where a pair of entangled
photons traversing symmetric paths wit
h balanced optical pathlengths in two
arms behave like a single photon with half the wavelength, leading to a two-
fold resolution improvem
ent. Concurrently, QMC resists stray light up to 155
times stronger than classical signals. The low intensity and entanglement
features of biphotons in QMC promis
e nondestructive bioimaging. QMC
advances quantum imaging to the microscopic level with signi
fi
cant
improvements in speed and CNR towar
d the bioimaging of cancer cells. We
experimentally and theoretically prove that the con
fi
guration with balanced
pathlengths illuminates an avenue fo
r quantum-enhanced coincidence ima-
ging at the Heisenberg limit.
Since the
fi
rst demonstration of entangled photon sources, the
biphoton state
1
3
has found extensive applications in quantum
computing
4
, quantum metrology
5
,
6
, and quantum information
7
,
8
.In
particular, the nonclassical behavior of biphotons motivates the search
for solutions that break classical limits, such as the uncertainty prin-
ciple or the diffraction limit
9
,
10
. The diffraction pattern of biphotons
has been demonstrated to be half as narrow as that of classical light
11
13
,
indicating the capability of biphoton imaging to achieve super reso-
lution beyond what is possible with classical light in diffraction-limited
linear imaging
14
.
A variety of approaches have been proposed for quantum imaging
using biphotons. Different nonlinear crystals, including
β
-barium
borate (BBO)
15
and periodically poled potassium titanyl phosphate
(PPKTP)
16
, were used for generating entangled photon pairs utilizing
the spontaneous parametric down-conversion (SPDC) effect
17
19
.In
addition, different types of detectors were employed for biphoton
detection. For example, single-photon avalanche diodes (SPADs) can
provide direct coincidence measurements based on the arrival times
of entangled photon pairs but do not have spatial resolution as they
are single-pixel detectors. Though SPAD-array cameras add spatial
resolution to single SPADs, they have a small number of pixels
15
,
20
22
.
Electron multiplying charge-coupled devices (EMCCDs) provide a
large number of resolvable pixels but are not capable of direct coin-
cidence measurements due to the low frame rate
23
25
. Thus far, two
methods have been developed and are frequently used to extract the
coincidence counts from an EMCCD camera
23
,
24
. However, these
methods typically require more than 2 × 10
6
frames to generate a single
coincidence image, which can take over 17 h, given the low frame rate.
Received: 15 August 2022
Accepted: 14 April 2023
Check for updates
1
Caltech Optical Imaging Laboratory, Andrew and Peggy Cherng Department of Medical Engineering, Department of Electrical Engineering, California
Institute of Technology, 1200 E. California Blvd., MC 138-78, Pasadena CA 91125, USA.
2
These authors contributed equally: Zhe He, Yide Zhang, Xin Tong.
e-mail:
LVW@caltech.edu
Nature Communications
| (2023) 14:2441
1
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1234567890():,;
The development of wide-
fi
eld quantum imaging, therefore, is ham-
pered by the low acquisition rate. In comparison to classical wide-
fi
eld
imaging, quantum imaging bene
fi
ts from stray light resistance
24
,
26
,
enhancement of two-photon absorption
27
,
28
, and enhanced resolution
as a result of quantum correlation
23
,
29
. Despite these advantages,
EMCCD-based wide-
fi
eld quantum imaging with spatial resolution
as
fi
ne as 1.4
μ
m has never been reported due to the use of low-
intensity light.
When quantum entanglement is applied for resolution beyond the
classical limit
5
,
N
entangled photons may improve spatial resolution by
N
times, corresponding to the Heisenberg limit
30
.Usingabiphoton
NOON state in quantum lithography
1
enhances resolution by two fold,
and using an SPDC source also achieves the Heisenberg limit
11
.Both
methods utilize co-propagating biphotons to enhance resolution by a
factor of 2
30
,
31
. Moreover, recent studies indicate that resolution at the
Heisenberg limit could be realized even without requiring both entan-
gled photons to pass through the imaging object
23
.
Here, inspired by the wide-
fi
eld imaging method introduced in
refs.
23
,
32
, we develop quantum microsc
opy by coincidence (abbre-
viated as QMC in our work) with balanced pathlengths using an EMCCD
camera. Previous studies could not be used for practical microscopy for
the following reasons. First, they
did not have the option for high-
resolution imaging due to the small numerical aperture (NA) of the
imaging system. Second, they had a low imaging speed, requiring a
large number of frames for coincidence measurements. In our techni-
que, we improve the spatial resolution and speed by introducing a high-
NA microscopy design and a more ef
fi
cient algorithm. QMC relies on
the nonclassical properties of biphotons for super-resolution micro-
scopy with up to 5 times higher speeds, 2.6 times higher CNRs, and 10
times more resistance to stray light than existing wide-
fi
eld quantum
imaging techniques
23
,
24
. In contrast to the quantum imaging techniques
at the standard quantum limit
1
,
29
,
33
, QMC improves resolution by a factor
of 2 at the Heisenberg limit
23
. We demonstrate QMC for imaging cancer
cells with a 1.4
μ
mresolutionanda100×50
μ
m
2
fi
eld of view (FOV).
The combination of the improved s
peed, enhanced CNR, more robust
stray light resistance, super resolution, and low-intensity illumination
empowers QMC toward bioimaging.
Results
Experimental setup
The experimental setup of QMC is presented in Fig.
1
(see
Methods
for details). The
fi
rst prism separates the signal and idler photons into
two arms, and the optical pathlengths of the separated arms are
balanced (see
Discussion
). The arm associated with the object is
considered by itself the classical part for imaging, which can be
regarded as a wide-
fi
eld microscope. Therefore, an image acquired by
this arm alone is deemed a classical image.
Despite being used to image distinct types of objects, the previous
methods
23
,
24
(Supplementary Fig. 1) and QMC are based on similar
theories. However, the previous works demonstrated only macro-
scopic imaging because the two arms share the same lenses with a
small NA and a large
fi
eld of view (FOV). In comparison, QMC evenly
splits the beam at the source Fourier plane into the signal and idler
arms using a right-angle prism, which allows integrating high-NA
objectives in each arm. As shown in Fig.
1
, the two arms are built
symmetrically to ensure balanced optical pathlengths and magni
fi
ca-
tion ratios, which are the key conditions for super resolution at the
Heisenberg limit (see
Discussion
).
Estimation of coincidence
As shown in Fig.
2
a, we develop a covariance algorithm to ef
fi
ciently
estimate the coincidence intensity of signal and idler photons using an
EMCCD camera. The signal and idler photons are detected by the left
and right regions of the camera, respectively. The calibration for the
EMCCD is shown in Supplementary Fig. 2. The total intensity
I
L
ð
I
R
Þ
is
related to the coincidence intensity of biphotons
I
coin
and the intensity
of noise
I
L
noise
ð
I
R
noise
Þ
,where
L
and
R
represent the left and right regions,
respectively. In QMC, we use the mean value of coincidence intensity
I
coin
to estimate the intensity correlation
G
ð
2
Þ
QMC
. Studies have demon-
strated that the distributions of entangled photon pairs in both regions
are symmetric about a center point due to their momentum antic-
orrelation in the far
fi
eld of the crystal
32
; therefore, the left and right
images can be inversely registered pixel by pixel according to the
symmetric center. The intensities of each pair of inversely registered
pixels in the left and right images are given by
I
L
=
I
coin
+
I
L
noise
:
ð
1
Þ
I
R
=
I
coin
+
I
R
noise
:
ð
2
Þ
The covariance between
I
L
and
I
R
is de
fi
ned by
cov
ð
I
L
,
I
R
Þ
=
1
N
X
N
i
ð
I
L
i


I
L
Þð
I
R
i


I
R
Þ
:
ð
3
Þ
where
N
is the number of frames, and the subscript
i
refers to the frame
index. Eq. (
3
) can be simpli
fi
ed to
cov
ð
I
L
,
I
R
Þ
=
I
2
coin
I
coin
Þ
2
+
I
L
noise
I
R
noise

I
L
noise

I
R
noise
:
ð
4
Þ
while the
fi
rst two terms represent the variance of the signal, the
last two terms represent the covariance of the detection noise. Because
266 nm
CW laser
GL
HWP
VWP
BBO
BPF
0
Source Fourier plane (
P
0
)
1
1
2
2
Object plane (
P
obj
)
2
2
Reference plane (
P
ref
)
1
1
Intermediate plane
3
4
Detection plane (
P
det
)
EMCCD
BPF
Fig. 1 | Experimental setup of QMC.
CW continuous wave, GL Glan-Laser polarizer,
HWP half-wave plate, VWP variable wave plate, BBO
β
-barium borate crystal, BPF
532 nm bandpass
fi
lter, PBS polarizing beam splitter, EMCCD electron multiplying
charge-coupled device camera.
f
0
= 50 mm,
f
1
= 180 mm,
f
2
= 9 mm,
f
3
= 300 mm,
and
f
4
= 200 mm. The source Fourier plane P
0
is set at the Fourier plane of the BBO
crystal.
Article
https://doi.org/10.1038/s41467-023-38191-4
Nature Communications
| (2023) 14:2441
2
the noise is primarily caused by the detector, which can be assumed to
be uncorrelated between the left an
d right regions, the covariance of
the detection noise approximately vanishes. In Supplementary Fig. 3, we
demonstrate that
I
L
noise
I
R
noise

I
L
noise

I
R
noise
I
2
coin

I
coin

2
.Further,as
the coincidence intensity follows a Poisson distribution
17
,forwhichthe
variance equals the mean, we have
34
cov
ð
I
L
,
I
R
Þ
=
I
2
coin

I
coin

2
=
I
coin
:
ð
5
Þ
With enough frames, Eq. (
5
) directly estimates the expected
value of the coincidence intensity, which is not directly provided by
the existing algorithms
23
,
24
,
32
. Figure
2
b compares QMC with the
existing methods
23
,
24
in terms of the CNR versus the number of
frames. The CNR calculation work
fl
ow is shown in
Methods
and Supplementary Fig. 4. To achieve a CNR of 3, QMC requires
10
5
frames (10 ms per frame), which is approximately 40% and
20% of the required frames in refs.
23
,
24
, respectively. When
2×10
6
frames are used, QMC outperforms the methods given
in refs.
23
,
24
with 1.5 times and 2.6 times higher CNR, respectively
(see Supplementary Fig. 4). As expected, CNR increases with the
number of frames (Supplementary Fig. 5).
Resistance to stray light is a major advantage of quantum imaging.
Eq. (
5
) indicates that the covariance algorithm suppresses uncorre-
lated noise, such as stray light. While the methods introduced in
refs.
23
,
24
were reported to be effective in preventing stray light in
images using over 2 × 10
6
frames, their effectiveness is limited, espe-
cially when the frame number is less than 10
5
.Figure
2
cshowsthe
dependence of CNR on stray light intensity with 10
5
frames. The data
processing work
fl
ow for the stray light resistance in Fig.
2
cis
demonstrated in Supplementary Fig.
6. When the stray light intensity is
~12 times greater than the classical signal, the classical image is severely
disrupted because the CNR falls below unity; the methods in refs.
23
,
24
cannot maintain the CNR either. Nonetheless, with 10
5
frames, the CNR
of QMC remains higher than unity even when the stray light is ~120
times stronger than the classical signal. Figures
2
d,edisplaytheclas-
sical and QMC images of carbon
fi
bers in the presence of stray light
that is 8 times stronger than the class
ical signal. Whereas the classical
image is overwhelmed by the stray light (CNR = 0.92 ± 0.11), the QMC
1
L
R
2
3
Intensity
cov(
,
)≫cov(
,
)
a
bc
Classical
1
0
Quantum
1
0
de
Fig. 2 | Coincidence measurement of QMC. a
The coincidence measurement relies
on the fact that the covariance between entangled photons in a sequence of frames
is much larger than the covariance between two random photons.
L
and
R
refer to
the left and right regions of the EMCCD, which are used to detect the signal and
idler photons, respectively.
r
2,
s
and
r
2,
i
are symmetric positions on the detector for
the signal and idler photons.
r
2,
i
is a random position in the right region and
different from
r
2,
i
. Inset, intensities (
I
) at the three positions in different frames.
b
CNRs of QMC and the wide-
fi
eld quantum imaging methods in refs.
23
,
24
using
different numbers of frames. Data are plotted as means ± standard errors of the
means (
n
= 10).
c
CNRs of QMC and the wide-
fi
eld quantum imaging methods in
refs.
23
,
24
with 10
5
frames in the presence of stray light with different intensities.
Data are plotted as means ± standard errors of the means (
n
= 10). The mean
number of photons incident on the EMCCD is 0.49 per pixel per frame. Classical (
d
)
and QMC (
e
)imagesofcarbon
fi
bers in the presence of stray light with an intensity
of 8
I
0
, acquired using 2 × 10
6
frames. Scale bars, 20
μ
m.
Article
https://doi.org/10.1038/s41467-023-38191-4
Nature Communications
| (2023) 14:2441
3
image eliminates the stray light nearly completely by extracting the
coincidence intensity (CNR = 8.03 ± 1.22). In fact, with 2 × 10
6
frames,
QMC effectively suppresses stray light that is ~155 times stronger than
the classical signal (Supplementary Fig. 7). The stray light resistance
reaches its limit when the accidental coincidence caused by the stray
light equals the true coincidence. The covariance algorithm proves to
be the most effective at
fi
nding true coincidences of entangled pho-
tons and eliminating uncorrelated noise, providing the highest CNR
under the same stray light intensity.
Quanti
fi
cation of super resolution at the Heisenberg limit
We next quantify the enhanced spatial resolution of QMC. Figure
3
a
shows a simpli
fi
ed schematic of QMC. Figure
3
b demonstrates the
classical image of group 7 of a US Air Force (USAF) resolution
target that includes stripes of varying widths (from 2.76 to 3.91
μ
m),
which approximate the highest resolution of our classical imaging
setup. In Fig.
3
c, the QMC image shows a higher resolution than the
classical image. We evaluate the resolution enhancement by deter-
mining the full width at half maximum (FWHM) of the line spread
functions (LSFs) near the focal point (see
Methods
for details).
Figure
3
d shows that the highest resolutions of classical imaging
and QMC are 2.9
μ
m and 1.4
μ
m, respectively, indicating that QMC
improves the spatial resolution of classical imaging by approximately
a factor of 2. The LSFs at different axial
z
coordinates are shown
in Fig.
3
e.
QMC demonstrates a two-fold enhancement in spatial resolution
over classical imaging due to the fact that the equivalent wavelength of
the biphoton is half the wavelength of the SPDC photon. As shown in
Fig.
3
a,
r
0,
s
,
r
1,
s
,and
r
2,
s
are the coordinates of the source Fourier plane,
the object plane, and the detection plane in the signal arm, respec-
tively.
r
0,
i
,
r
1,
i
,and
r
2,
i
are the corresponding coordinates in the idler
arm. The quantized
fi
eld operators
^
E
+
ðÞ
s
and
^
E
+
ðÞ
i
for the signal and idler
arms are shown in Supplementary Note 1. The intensity correlation
between the signal and idler photons for a given pixel pair is given by
the second-order correlation function:
G
ð
2
Þ
QMC
=0
j
^
E
+
ðÞ
s
^
E
+
ðÞ
i
j
ξ
DE






2
:
ð
6
Þ
where
ξ

is the wavefunction of a photon pair emitted from the source
Fourier plane at
r
0,
s
and
r
0,
i
:
ξ



=
X
k
0,
s
A
k
0,
s

e

j
k
0,
s

r
0,
s
e

j
k
0,
i

r
0,
i
1
k
0,
s
,1
k
0,
i
E
:
ð
7
Þ
k
0,
s
and
k
0,
i
are the entangled wavevectors of the signal and idler
photons from the source Fourier plane. Denoting
r
p
and
k
p
the
BBO
z
=
40
μm
30
μm
20
μm
10
μm
0
μm
-10
μm
-20
μm
-30
μm
-40
μm
b
d
Classical
Classical
Quantum
1
0
1
0
Quantum
c
a
e
Fig. 3 | Spatial resolution of QMC. a
Simple schematic of QMC. BBO,
β
-barium
borate crystal. EMCCD, electron multiplying charge-coupled device camera.
r
0
,
r
1
,
and
r
2
are the coordinates of the source Fourier plane, the object plane, and the
detection plane, respectively.
r
0,
s
,
r
1,
s
,and
r
2,
s
are the corresponding coordinates in
the signal arm, and
r
0,
i
,
r
1,
i
,and
r
2,
i
are the coordinates in the idler arm.
h
r
0,
s
,
r
1,
s

and
h
r
1,
s
,
r
2,
s

are the PSFs from
r
0,
s
to
r
1,
s
and from
r
1,
s
to
r
2,
s
.
h
r
0,
i
,
r
1,
i

and
h
r
1,
i
,
r
2,
i

are the PSFs from
r
0,
i
to
r
1,
i
and from
r
1,
i
to
r
2,
i
.
t
is the amplitude
transmission coef
fi
cient of the object. Classical (
b
)andQMC(
c
) images of group 7
(2.76 ~ 3.91
μ
m) of a USAF 1951 resolution target. Scale bars, 20
μ
m. All the images
are normalized by their maximum and minimum intensities (see
Methods
).
d
Spatial resolution of classical imaging and QMC versus the axial
z
coordinate from
the classical focal point. The highest spatial resolutions for classical imaging and
QMC are 2.9
μ
mand1.4
μ
m, respectively. Data are plotted as means ± standard
errors of the means (
n
=14).
e
Normalized lateral LSFs of classical imaging and QMC
versus the lateral coordinate at different
z
positions.
Article
https://doi.org/10.1038/s41467-023-38191-4
Nature Communications
| (2023) 14:2441
4
position and wavevector of the pump light, Eq. (
7
)demonstratesa
spatially entangled state with
r
0,
s
+
r
0,
i

=
2=
r
p
and
k
0,
s
+
k
0,
i
=
k
p
.
A
k
0,
s

denotes the probability amplitude of the state
1
k
0,
s
,1
k
0,
i
i
.The
momentum correlation width of the entangled photons is demon-
strated in Supplementary Fig. 8.
As derived in Supplementary Note 1, the QMC image can be
described by
G
2
ðÞ
QMC
:
G
2
ðÞ
QMC
ρ
ðÞ
=
t
ρ
ðÞ
2
Γ
QMC
λ
2
;
ρ

h
λ
2
;
ρ
,
M
ρ









2
:
ð
8
Þ
where
t
(
ρ
) is the amplitude transmission coef
fi
cient of the object, and
ρ
is the 2D coordinates on the object plane.
Γ
QMC
λ
2
;
ρ

is the dis-
tribution of squared intensity with a wavelength of
λ
/2 on the object
plane.
h
(
λ
;
ρ
,
M
ρ
) is the point spread function (PSF) from
ρ
on the
object plane (P
obj
)to
M
ρ
on the detection plane (P
det
) for the light with
a wavelength of
λ
/2.
M
is the magni
fi
cation ratio from the object to the
detector. Similarly, the classical counterpart is given by
G
ð
1
Þ
CI
ρ
ðÞ
=
t
ρ
ðÞ
2
γ
CI
λ
;
ρ
ðÞ
h
λ
;
ρ
,
M
ρ
ðÞ
2
:
ð
9
Þ
where
γ
CI
λ
;
ρ
ðÞ
is the intensity distribution of wide-
fi
eld illumination
with a wavelength of
λ
on the object plane.
h
λ
;
ρ
,
M
ρ
ðÞ
denotes the
point spread function (PSF) from
ρ
on the object plane (P
obj
)to
M
ρ
on
thedetectionplane(P
det
) for the light with a wavelength of
λ
.
In contrast to linear classical imaging, QMC is based on a pure
quantum effect to achieve the Heisenberg limit. Unlike the quantum
super-resolution methods requiring both signal and idler photons to
pass through the object
30
, the idler photons in our experiment do not
traverse the object. Indicated by Eqs. (S5) and (S6), while calculating
the QMC image, the point spread functions
h
r
1,
s
,
r
2,
s

and
h
r
1,
i
,
r
2,
i

in
Fig.
3
a are multiplied for each photon pair instead of being multiplied
classically as
h

h
=
h
2
. This concept has been theoretically proven for
quantum imaging based on a simpli
fi
ed model
35
,which,however,
cannot be applied to the complex setup in this work (see Fig.
3
a).
For example, as shown in Fig.
3
b, c, the spatial distributions of the
wide-
fi
eld illumination for the classical imaging and QMC are different,
which was not considered in ref.
35
but can be explained by
different wide-
fi
eld illumination functions
Γ
QMC
λ
=
2
;
ρ

and
γ
CI
λ
;
ρ
ðÞ
in
Eqs. (
8
,
9
).
The classical resolution in our experiment is limited by the
effective NA of the objectives, which may be lower than the nominal
NA of the objectives (NA = 0.4) due to under
fi
lling.
Imaging cells by QMC
In Fig.
4
, we demonstrate classical (Fig.
4
a) and QMC (Fig.
4
b) imaging
of cancer cells. Figure
4
c shows the normalized intensities between the
arrows in Fig.
4
a, b. QMC clearly distinguishes the cell structures that
cannot be resolved in its classical counterpart. Note that the lumpy
features in both images are due to imperfect sample preparation.
Whereas the images in Fig.
4
were averaged over 2 × 10
6
frames (10 ms
per frame) to achieve a high CNR, the images of the cells shown in
Supplementary Fig. 9 were acquired using fewer (10
5
)frames.
Discussion
The balanced pathlengths require symmetry in the optical paths of the
signal and idler photons from the source Fourier plane to the detection
planes, such that the paired photons are correlated in positions and
momentums concurrently, and the phases of the paired photons can
be combined. This requirement, however, cannot be satis
fi
ed through
classical sources because two unentangled photons can only be cor-
related in either position or momentum in accordance with the
uncertainty principle
36
. As a consequence of the path symmetry, all
entangled photon pairs should appear at positions symmetric about
the same center within the source Fourier plane, the object plane, and
the detection plane. We mirrored the signal arm setup onto the
idler arm to maintain the path symmetry as precisely as possible.
In particular, the photon pairs on the symmetric positions on
the source Fourier plane propagate symmetrically due to the SPDC
phase matching, and they propagate through the identical pairs of free-
space 4
f
systems to reach the object plane and the reference plane,
respectively. The sign
al photon on the object plane can be scattered by
the object, leading to different wavevectors between the signal and idler
photons. In Fig.
3
a, in the paraxial approximation, photons traversing
the same position on the object plane would arrive at the same position
on the detection plane, indicating
identical optical pathlengths
according to Fermat
s principle. Though the scattering effect appears to
disrupt the path symmetry, the pathlength symmetry is maintained
because the conjugation between the object and detection planes bal-
ances the optical pathlengths of a scattered signal photon and the
related idler photon. Therefore, we can utilize the con
fi
guration of the
balanced pathlengths to describe t
he biphoton propagation from the
sourceFourierplanetothedetectionplane(seeEq.(S5)).
We have attempted to provide the most practical setup and
algorithm for quantum bioimaging with a spatial resolution down to
1.4
μ
m. However, the current implementation of QMC is not intended
to compete with state-of-the-art classical microscopy techniques in
termsofCNRsbecauseofthelowSPDCef
fi
ciency of the BBO crystal.
For example, to achieve a CNR of 3, QMC requires the acquisition of
about 10
5
frames over 17 min, whereas classical imaging may only need
a single frame captured in less than a second. With more powerful
quantum sources in the future
37
, QMC could demonstrate quantum
advantages over state-of-the-art classical imaging. Furthermore, com-
pared with classical methods, such as SHG microscopy
38
, that reject
background noise through spectral
fi
ltering, QMC eliminates both
temporally and spatially uncorrelated background noise through
coincidence detection.
In conclusion, we have demonstrated quantum microscopy of
cancer cells at the Heisenberg limit. QMC is advantageous over exist-
ing wide-
fi
eld quantum imaging methods due to the 1.4
μ
m resolution,
a
c
b
Classical
Quantum
1
0
1
0
Fig. 4 | Imaging of cancer cells with QMC.
Classical (
a
)andQMC(
b
)imagesoftwo
HeLa cells. Scale bars, 20
μ
m.
c
Normalized classical and QMC intensities between
the arrows in (
a
)and(
b
).
Article
https://doi.org/10.1038/s41467-023-38191-4
Nature Communications
| (2023) 14:2441
5
up to 5 times higher speed, 2.6 times higher CNR, and 10 times more
robustness to stray light. With low-intensity illumination, we have
demonstrated that QMC is suitable for nondestructive bioimaging at a
cellular level, revealing details that cannot be resolved by its classical
counterpart. Finally, while the resolution of classical imaging can be
improved in various ways
39
,
40
,thecon
fi
guration used in QMC can
further improve the resolution by halving the wavelength, thus push-
ing the boundary of classical super-resolution imaging techniques with
quantum enhancement.
Methods
Experimental setup
In the QMC system, a
β
-barium borate (BBO) crystal (5 × 5 × 0.5 mm
3
,
PABBO5050-266(I)-HA3, Newlight Photonics) was cut for type-I SPDC
at 266 nm wavelength. The pump was a 266 nm continuous-wave laser
(FQCW266-10-C, CryLaS) with an output power of 10 mW. A UV-coated
Glan-Laser polarizer (GLB10-UV, Thorlabs) and a half-wave plate
(WPH05M-266, Thorlabs) were used to adjust the polarization angle of
the pump laser beam. For imaging, the pump beam was adjusted to be
vertically polarized. The pump laser beam then passed through the
BBO crystal and generated a ring of SPDC photons with a half-opening
angle of 3°. A bandpass
fi
lter with a center wavelength of 532 nm and a
bandwidth of 2 nm (64-252, Edmund Optics) was used to block the
pump beam. The generated SPDC photon pairs propagated through an
f
0
=50mmlenstotheFourierplane,i.e.,thesourceFourierplane(P
0
),
and were spatially separated using a knife-edge right-angle prism
mirror (MRAK25-P01, Thorlabs). The separated signal and idler pho-
tons propagated to the object plane (P
obj
) and the reference plane
(P
ref
), respectively, by two identical 4
f
imaging systems comprising
of an
f
1
= 180 mm lens and an
f
2
= 9 mm objective (LI-20X, 0.4 NA,
Newport). The sample was placed on the object plane. The object
plane, the reference planes, and the intermediate plane were conjugate
through the other two identical 4
f
imaging systems, which consist of
an identical set of
f
2
= 9 mm objectives and
f
1
= 180 mm lenses and
another right-angle prism mirror. Each objective was followed by an
HWP mounted on a motorized precision rotation mount (PRM1Z8,
Thorlabs). The intermediate plane and the detection plane (P
det
)ofan
EMCCD camera (iXon Ultra 888, Andor) were conjugated through a 4
f
system consisting of
f
3
= 300 mm and
f
4
= 200 mm lenses. Another BPF
was placed in front of the EMCCD camera to block unwanted stray
light. The EMCCD was operated at
65 °C, with a horizontal pixel shift
readout rate of 10 MHz, a vertical pixel shift speed of 1.13
μ
s, and an
electron multiplier (EM) gain of 1000. The whole setup was covered by
a light-shielding box.
Sample preparation
A2
×2
(5.08 × 5.08 cm) positive 1951 USAF resolution target (58-
198, Edmund Optics) was used to quantify the spatial resolution and
DOF of our system. The carbon
fi
ber sample was prepared by ran-
domly distributing carbon
fi
bers with a diameter of 6
μ
m on top of a
glass slide. The
fi
bers were mixed with UV-curing optical adhesive
(NOA61, Thorlabs) and sealed with a cover glass. The optical adhesive
was then cured by illumination of UV light from a light-emitting diode
(LED). HeLa cells were placed on sterile glass slides and cultured in
DMEM supplemented with 10% fetal bovine serum and a penicillin-
streptomycin mixture (all from Invitrogen/Life Technologies) at
37 °C in a 5% CO
2
air atmosphere. When cells were 70% con
fl
uent on
the glass slides, we
fi
xed them with an ice-cold mixture of ethanol and
methanol (1:1 volume ratio). The glass slides placed in a 10-cm petri-
dish were covered by the organic solvents and then incubated in a
freezer (
20 °C) for 5
7 min. The organic solvents preserved the
cells by removing lipids, dehydrating tissue, and denaturing and
precipitating the proteins in the cells. After
fi
xation, the glass slides
were gently rinsed with phosphate-buffered saline to remove any
fi
xation agent.
Data acquisition and processing
A custom-written LabVIEW (National Instruments) program utilizing
the library from the Andor software development kit (SDK) was used to
control the EMCCD for data acquisition. The imaging data were saved
as 16-bit Flexible Image Transport System (FITS)
fi
les with each
fi
le
containing 1000 frames. The FITS
fi
les were imported into MATLAB
(MathWorks) and processed with custom-written scripts. The EMCCD
frames were extracted from the
fi
les and were used to calculate the
coincidence intensity using our QMC algorithm. The reconstructed
images were then interpolated based on a cubic spline using not-a-knot
end conditions for better visualization. The maximum pixel number of
the EMCCD camera is 1024 × 1024. We utilized an area of 100 × 50
pixels after binning of 2.
Image normalization
Denoting
I
as the image intensity, the normalized intensity is calcu-
lated by
I
norm
=
I

I
min
I
max

I
min
:
ð
10
Þ
where
I
max
and
I
min
are the maximum and minimum values of
I
.
Contrast-to-noise ratio estimation
Denoting
I
1
and
I
2
as the intensities of the object of interest and the
background, respectively, the contrast-to-noise ratio (CNR) is calcu-
lated by
CNR =

I
1


I
2




ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
σ
2
1
+
σ
2
2
q
:
ð
11
Þ
where

I
1
and

I
2
are the mean values;
σ
1
and
σ
2
are the standard devia-
tions of
I
1
and
I
2
.
Measurements of resolution and depth of
fi
eld
To measure the resolution of our system, the line pro
fi
le
perpendicular to an edge in the USAF resolution target was extracted
and
fi
tted to an edge spread function (ESF) centered at
x
0
, i.e.,
ESF
x
ðÞ
=
a
erf
ð
x

x
0
Þ
=
w

+
b
,where
a
and
b
are coef
fi
cients, and
w
is
the radius of the beam. A Gaussian line spread function (LSF) was
obtained by taking the derivative of the ESF, i.e., LSF
x
ðÞ
=
d
ESF
ð
x
Þ
=
dx
=
2
a
exp
ð
x

x
0

2
=
w
2
Þ
=
w
ffiffiffiffi
π
p

. The resolution was estimated by the
FWHM of the LSF, i.e.,
R
=2
ffiffiffiffiffiffiffi
ln2
p
w
.
Imaging with stray light
A 532 nm continuous-wave laser (MLL-III-532, CNI) was used to
introduce stray light to the detection plane. Transmitting through
a ground glass diffuser (DG20-1500, Thorlabs), the 532 nm laser
created speckle patterns on the detection plane, leading to sig-
ni
fi
cantly reduced CNR in the raw EMCCD images. To evaluate how
robust the classical imaging and QMC were against the stray light, we
acquired images under different stray light intensities and calculated
their CNRs.
Statistics and reproducibility
Statistical analysis was performed using MATLAB (R2021a). Data are
presented as means ± standard errors of the means in all
fi
gure parts in
which error bars are shown. No statistical method was used to pre-
determine sample sizes. We determined sample sizes based on our
preliminary studies and on the criteria in the
fi
eld to experimentally
demonstrate the imaging system. All experiments except for that
shown in Fig.
4
were replicated at least twice. All attempts at replica-
tion were successful. Cell imaging in Fig.
4
with 2 × 10
6
frames was not
replicated because we repeated the measurement under the same
Article
https://doi.org/10.1038/s41467-023-38191-4
Nature Communications
| (2023) 14:2441
6
condition with 10
5
frames (Supplementary Fig. 9). Besides, we have
repeated experiments on other samples under the same condition
with 2 × 10
6
frames.
Reporting summary
Further information on research design is available in the Nature
Portfolio Reporting Summary linked to this article.
Data availability
Imaging data for the cell images generated in Fig.
4
are available in the
Github online at
http://github.com/ZheHE2022/Quantum-Microscopy-
of-Cells-at-the-Heisenberg-Limit
. All data used in this study are available
from the corresponding auth
or upon reasonable request.
Code availability
The code for the covariance algorithm is provided in the Supplemen-
tary Software and Github online at
http://github.com/ZheHE2022/
Quantum-Microscopy-of-Cells-at-the-Heisenberg-Limit
. All custom
codes used in this study are available from the corresponding author
upon reasonable request.
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Acknowledgements
We thank Dr. Qiyuan Song and Samuel A. Solomon for their assistance
with the experiment. We also thank Dr. Kelvin Titimbo Chaparro and
Siddik Suleyman Kahraman for the discussion. This project has been
made possible in part by grant number 2020-225832 from the Chan
Zuckerberg Initiative DAF, an advised fund of Silicon Valley Community
Foundation, and National Institutes of Health grants R35 CA220436
(Outstanding Investigator Award) and R01 EB028277.
Author contributions
Z.H., Y.Z., and X.T. built the imaging system, performed the experiments,
and analyzed the data. Z.H. developed the quantum imaging theory. Y.Z.
Article
https://doi.org/10.1038/s41467-023-38191-4
Nature Communications
| (2023) 14:2441
7
developed the data acquisition program. L.L. prepared the biological
samples. L.V.W. conceived the concept and supervised the project.
All authors contributed to writing the manuscript.
Competing interests
The authors declare no competing interests.
Additional information
Supplementary information
The online version contains
supplementary material available at
https://doi.org/10.1038/s41467-023-38191-4
.
Correspondence
and requests for materials should be addressed to
Lihong V. Wang.
Peer review information
Nature Communications
thanks the anon-
ymous reviewers for their contribution to the peer review of this work.
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