Teleportation Systems Towards a Quantum Internet
Raju Valivarthi,
1, 2
Samantha Davis,
1, 2
Cristi ́an Pe ̃na,
1, 2, 3
Si Xie,
1, 2
Nikolai Lauk,
1, 2
Lautaro Narv ́aez,
1, 2
Jason P. Allmaras,
4
Andrew D. Beyer,
4
Yewon Gim,
2, 5
Meraj Hussein,
2
George Iskander,
1
Hyunseong Linus
Kim,
1, 2
Boris Korzh,
4
Andrew Mueller,
1
Mandy Rominsky,
3
Matthew Shaw,
4
Dawn Tang,
1, 2
Emma E.
Wollman,
4
Christoph Simon,
6
Panagiotis Spentzouris,
3
Neil Sinclair,
1, 2, 7
Daniel Oblak,
6
and Maria Spiropulu
1, 2
1
Division of Physics, Mathematics and Astronomy,
California Institute of Technology, Pasadena, CA 91125, USA
2
Alliance for Quantum Technologies (AQT), California Institute of Technology, Pasadena, CA 91125, USA
3
Fermi National Accelerator Laboratory, Batavia, IL 60510, USA
4
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
5
AT&T Foundry, Palo Alto, CA 94301, USA
6
Institute for Quantum Science and Technology, and Department of Physics & Astronomy,
University of Calgary, Calgary, AB T2N 1N4, Canada
7
John A. Paulson School of Engineering and Applied Sciences,
Harvard University, Cambridge, MA 02138, USA
(Dated: July 29, 2020)
Quantum teleportation is essential for many quantum information technologies including long-
distance quantum networks. Using fiber-coupled devices, including state-of-the-art low-noise super-
conducting nanowire single photon detectors and off-the-shelf optics, we achieve quantum teleporta-
tion of time-bin qubits at the telecommunication wavelength of 1536.5 nm. We measure teleportation
fidelities of
≥
90% that are consistent with an analytical model of our system, which includes realis-
tic imperfections. To demonstrate the compatibility of our setup with deployed quantum networks,
we teleport qubits over 22 km of single-mode fiber while transmitting qubits over an additional 22
km of fiber. Our systems, which are compatible with emerging solid-state quantum devices, provide
a realistic foundation for a high-fidelity quantum internet with practical devices.
I. INTRODUCTION
Quantum teleportation [1], one of the most captivat-
ing predictions of quantum theory, has been widely in-
vestigated since its seminal demonstrations over 20 years
ago [2–4]. This is due to its connections to fundamental
physics [5–14], and its central role in the realization of
quantum information technology such as quantum com-
puters and networks [15–19]. The goal of a quantum
network is to distribute qubits between different loca-
tions, a key task for quantum cryptography, distributed
quantum computing and sensing. A quantum network
is expected to form part of a future quantum internet
[20–22]: a globally distributed set of quantum proces-
sors, sensors, or users there-of that are mutually con-
nected over a network capable of allocating quantum re-
sources (e.g. qubits and entangled states) between loca-
tions. Many architectures for quantum networks require
quantum teleportation, such as star-type networks that
distribute entanglement from a central location or quan-
tum repeaters that overcome the rate-loss trade-off of
direct transmission of qubits [19, 23–26].
Quantum teleportation of a qubit can be achieved by
performing a Bell-state measurement (BSM) between the
qubit and another that forms one member of an entan-
gled Bell state [1, 18, 27]. The quality of the teleporta-
tion is often characterized by the fidelity
F
=
〈
ψ
|
ρ
|
ψ
〉
of the teleported state
ρ
with respect to the state
|
ψ
〉
accomplished by ideal generation and teleportation [15].
This metric is becoming increasingly important as quan-
tum networks move beyond specific applications, such as
quantum key distribution, and towards the quantum in-
ternet.
Qubits encoded by the time-of-arrival of individual
photons, i.e. time-bin qubits [28], are useful for net-
works due to their simplicity of generation, interfacing
with quantum devices, as well as independence of dy-
namic transformations of real-world fibers. Individual
telecom-band photons (around 1.5
μ
m wavelength) are
ideal carriers of qubits in networks due to their ability
to rapidly travel over long distances in deployed optical
fibers [17, 29–31] or atmospheric channels [32], among
other properties. Moreover, the improvement and grow-
ing availability of sources and detectors of individual
telecom-band photons has accelerated progress towards
workable quantum networks and associated technologies,
such as quantum memories [33], transducers [34, 35], or
quantum non-destructive measurement devices [36].
Teleportation of telecom-band photonic time-bin
qubits has been performed inside and outside the labora-
tory with impressive results [29–31, 37–42]. Despite this,
there has been little work to increase
F
beyond
∼
90% for
these qubits, in particular using practical devices that al-
low straightforward replication and deployment of quan-
tum networks (e.g. using fiber-coupled and commercially
available devices). Moreover, it is desirable to develop
teleportation systems that are forward-compatible with
emerging quantum devices for the quantum internet.
In the context of Caltech’s multi-disciplinary multi-
institutional collaborative public-private research pro-
gram on Intelligent Quantum Networks and Technologies
(IN-Q-NET) founded with AT&T as well as Fermi Na-
arXiv:2007.11157v2 [quant-ph] 28 Jul 2020
2
tional Accelerator Laboratory and Jet Propulsion Labo-
ratory in 2017, we designed, built, commissioned and de-
ployed two quantum teleportation systems: one at Fer-
milab, the Fermilab Quantum Network (FQNET), and
one at Caltech’s Lauritsen Laboratory for High Energy
Physics, the Caltech Quantum Network (CQNET). The
CQNET system serves as an R&D, prototyping, and
commissioning system, while FQNET serves as an ex-
pandable system, for scaling up to long distances and is
used in multiple projects funded currently by DOE’s Of-
fice of High Energy Physics (HEP) and Advanced Scien-
tific Research Computing (ASCR). Material and devices
level R&D in both systems is facilitated and funded by
the Office of Basic Energy Sciences (BES). Both systems
are accessible to quantum researchers for R&D purposes
as well as testing and integration of various novel de-
vices, such as for example on-chip integrated nanopho-
tonic devices and quantum memories, needed to up-
grade such systems towards a realistic quantum inter-
net.Importantly both systems are also used for improve-
ments of the entanglement quality and distribution with
emphasis on implementation of protocols with complex
entangled states towards advanced and complex quan-
tum communications channels. These will assist in stud-
ies of systems that implement new teleportation proto-
cols whose gravitational duals correspond to wormholes
[43], error correlation properties of wormhole teleporta-
tion, on-chip codes as well as possible implementation of
protocols on quantum optics communication platforms.
Hence the systems serve both fundamental quantum in-
formation science as well as quantum technologies.
Here we perform quantum teleportation of time-bin
qubits at a wavelength of 1536.5 nm with an average
F
≥
90%. This is accomplished using a compact setup
of fiber-coupled devices, including low-dark-count sin-
gle photon detectors and off-the-shelf optics, allowing
straight-forward reproduction for multi-node networks.
To illustrate network compatibility, teleportation is per-
formed with up to 44 km of single-mode fiber between
the qubit generation and the measurement of the tele-
ported qubit, and is facilitated using semi-autonomous
control, monitoring, and synchronization systems, with
results collected using scalable acquisition hardware. Our
systems, which operates at a clock rate of 90 MHz, can
be run remotely for several days without interruption and
yield teleportation rates of a few Hz using the full length
of fiber. Our qubits are also compatible with erbium-
doped crystals, e.g. Er:Y
2
SiO
5
, that are used to develop
quantum network devices like memories and transduc-
ers [44–46]. Finally, we develop an analytical model of
our system, which includes experimental imperfections,
predicting that the fidelity can be improved further to-
wards unity by well-understood methods (such as im-
provement in photon indistinguishability). Our demon-
strations provide a step towards a workable quantum net-
work with practical and replicable nodes, such as the
ambitious U.S. Department of Energy quantum research
network envisioned to link the U.S. National Laborato-
ries.
In the following we describe the components of our sys-
tems as well as characterization measurements that sup-
port our teleportation results, including the fidelity of our
entangled Bell state and Hong-Ou-Mandel (HOM) inter-
ference [47] that underpins the success of the BSM. We
then present our teleportation results using both quan-
tum state tomography (QST) [48] and projection mea-
surements based on a decoy state method [49], followed
by a discussion of our model. We conclude by consid-
ering improvements towards near-unit fidelity and GHz
level teleportation rates.
II. SETUP
Our fiber-based experimental system is summarized
in the diagram of Fig. 1. It allow us to demonstrate
a quantum teleportation protocol in which a photonic
qubit (provided by Alice) is interfered with one member
of an entangled photon-pair (from Bob) and projected
(by Charlie) onto a Bell-state whereby the state of Al-
ice’s qubit can be transferred to the remaining member
of Bob’s entangled photon pair. Up to 22 (11) km of
single mode fiber is introduced between Alice and Char-
lie (Bob and Charlie), as well as up to another 11 km
at Bob, depending on the experiment (see Sec. III). All
qubits are generated at the clock rate, with all of their
measurements collected using a data acquisition (DAQ)
system. Each of the Alice, Bob, Charlie subsystems are
further detailed in the following subsections, with the
DAQ subsystem described in Appendix A 1.
A. Alice: single-qubit generation
To generate the time-bin qubit that Alice will teleport
to Bob, light from a fiber-coupled 1536.5 nm continuous
wave (CW) laser is input into a lithium niobate intensity
modulator (IM). We drive the IM with one pulse, or two
pulses separated by 2 ns. Each pulse is of
∼
65 ps full
width at half maximum (FWHM) duration. The pulses
are produced by an arbitrary waveform generator (AWG)
and amplified by a 27 dB-gain high-bandwidth amplifier
to generate optical pulses that have an extinction ratio
of up to 22 dB. We note that this method of creating
time-bin qubits offers us flexibility not only in terms of
choosing a suitable time-bin separation, but also for syn-
chronizing qubits originating from different nodes in a
network. A 90/10 polarization-maintaining fiber beam
splitter combined with a power monitor (PWM) is used
to apply feedback to the DC-bias port of the IM so as
to maintain a constant 22 dB extinction ratio [50]. In
order to successfully execute the quantum teleportation
protocol, photons from Alice and Bob must be indistin-
guishable in all degrees of freedom (see Sec. III B). Hence,
the optical pulses at the output of the IM are band-pass
filtered using a 2 GHz-bandwidth (FWHM) fiber Bragg
3
Charlie
DAQ
IM
Alice
CIR
VOA
POC
AMP
Bob
PWM
BS
90|10
1
TDC
Data Analysis
and Storage
Clock
FBG
FIS
2
3
4
LAS
FIS
CIR
CIR
SPDC
SHG
φ
MZI
EDFA
IM
PWM
AMP
Cryostat
PBS
50|50
BPF
FBG
1536 nm
signal
idler
POC
POC
FIS
AWG
Clock
BS
90|10
PWM = Powermeter
PBS = Polarizing
Beam Splitter
Controller
POC = Polarization
φ
MZI = Mach-Zehnder
Interferometer
LAS = Laser
IM = Intensity Modulator
HPF = High Pass Filter
EDFA = Erbium Doped
Fiber Amplifier
FIS = Fiber Spool
3
4
BS
10
90
|
SPDC = Spontaneous
Parametric Down Conversion
SNSPD = Superconducting
Nanowire Single Photon Detector
VOA = Variable Optical
Attenuator
SHG = Second Harmonic
Generation
TDC = Time-To-Digital
Converter
FBG
1536 nm
1510 nm
1510 nm
768 nm
1536 nm
1536 nm
AMP = Amplifier
AWG = Arbitrary
Waveform Generator
BS = Beam Splitter
CIR = Circulator
FBG = Fiber Bragg Grating
BPF = Band Pass Filter
Bandwidth: 20 nm
Cryostat
BS
50|50
PBS
PBS
1
2
HPF
HPF
HPF
1510 nm
HPF
1510 nm
FIG. 1. Schematic diagram of the quantum teleportation system consisting of Alice, Bob, Charlie, and the data acquisition
(DAQ) subsystems. See the main text for descriptions of each subsystem. One cryostat is used to house all SNSPDs, it is
drawn as two for ease of explanation. Detection signals generated by each of the SNSPDs are labelled 1-4 and collected at
the TDC, with 3 and 4 being time-multiplexed. All individual components are labeled in the legend, with single-mode optical
fibers (electronic cables) in grey (green), and with uni- and bi-chromatic (i.e. unfiltered) optical pulses indicated.
grating (FBG) centered at 1536.5 nm to match the spec-
trum of the photons from the entangled pair-source (de-
scribed in Sec. II B). Furthermore, the polarization of
Alice’s photons is determined by a manual polarization
controller (POC) in conjunction with a polarizing beam
splitter (PBS) at Charlie. Finally, the optical pulses from
Alice are attenuated to the single photon level by a vari-
able optical attenuator (VOA), to approximate photonic
time-bin qubits of the form
|
A
〉
=
γ
|
e
〉
A
+
√
1
−
γ
2
|
l
〉
A
,
where the late state
|
l
〉
A
arrives 2 ns after the early state
|
e
〉
A
,
γ
is real and set to be either 1, 0, or 1
/
√
2 to
generate
|
e
〉
A
,
|
l
〉
A
, or
|
+
〉
A
= (
|
e
〉
A
+
|
l
〉
A
)
/
√
2, respec-
tively, depending on the experiment. The complex rel-
ative phase is absorbed into the definition of
|
l
〉
A
. The
duration of each time bin is 800 ps.
B. Bob: entangled qubit generation and
teleported-qubit measurement
Similar to Alice, one (two) optical pulse(s) with a
FWHM of
∼
65 ps is (and separated by 2 ns are) cre-
ated using a 1536.5 nm CW laser in conjunction with a
lithium niobate IM driven by an AWG, while the 90/10
beam splitter and PWM are used to maintain an extinc-
tion ratio of at least 20 dB. An Erbium-Doped Fiber
Amplifier (EDFA) is used after the IM to boost the pulse
power and thus maintain a high output rate of photon
pairs.
The output of the EDFA is sent to a Type-0 period-
ically poled lithium niobate (PPLN) waveguide for sec-
ond harmonic generation (SHG), upconverting the pulses
to 768.25 nm. The residual light at 1536.5 nm is re-
moved by a 768 nm band-pass filter with an extinction
ratio
≥
80 dB. These pulses undergo spontaneous para-
4
metric down-conversion (SPDC) using a Type-II PPLN
waveguide coupled to a polarization-maintaining fiber
(PMF), approximately producing either a photon pair
|
pair
〉
B
=
|
ee
〉
B
, or the time-bin entangled state
|
φ
+
〉
B
=
(
|
ee
〉
B
+
|
ll
〉
B
)
/
√
2, if one or two pulses, respectively, are
used to drive the IM.
The ordering of the states refers to so-called signal and
idler modes of the pair of which the former has parallel,
and the latter orthogonal, polarization with respect to
the axis of the PMF. As before, the relative phase is
absorbed into the definition of
|
ll
〉
B
. Each photon is sep-
arated into different fibers using a PBS and spectrally
filtered with FBGs akin to that at Alice. Note the band-
width of the FBG is chosen as a trade-off between spec-
tral purity and generation rate of Bob’s photons [51].
The photon in the idler mode is sent to Charlie for
teleportation or HOM measurements (see Sec. III B), or
to the MZI (see below) for characterizations of the en-
tangled state (see Sec. III A), with its polarization de-
termined using a POC.The photon in the signal mode
is sent to a Mach Zehnder interferometer (MZI) by way
of a POC (and an additional 11 km of single-mode fiber
for some measurements), and is detected by supercon-
ducting nanowire single photon detectors (SNSPDs) [52]
after high-pass filtering (HPF) to reject any remaining
768.25 nm light. The MZI and detectors are used for
projection measurements of the teleported state, charac-
terization of the time-bin entangled state, or measuring
HOM interference at Charlie. The time-of-arrival of the
photons is recorded by the DAQ subsystem using a time-
to-digital converter (TDC) referenced to the clock signal
from the AWG.
All SNSPDs are installed in a compact sorption fridge
cryostat [53], which operates at a temperature of 0.8 K
for typically 24 h before a required 2 h downtime. Our
SNSPDs are developed at the Jet Propulsion Laboratory
and have detection efficiencies between 76 and 85%, with
low dark count rates of 2-3 Hz. The FWHM temporal
resolution of all detectors is between 60 and 90 ps while
their recovery time is
∼
50 ns. A detailed description
of the SNSPDs and associated setup is provided in Ap-
pendix A 2.
The MZI has a path length difference of 2 ns and is
used to perform projection measurements of
|
e
〉
B
,
|
l
〉
B
,
and (
|
e
〉
B
+
e
iφ
|
l
〉
B
)
/
√
2, by detecting photons at three
distinct arrival times in one of the outputs, and varying
the relative phase
φ
[28]. Detection at the other out-
put yields the same measurements except with a relative
phase of
φ
+
π
. Using a custom temperature-feedback
system, we slowly vary
φ
for up to 15 hour time intervals
to collect all measurements, which is within the cryostat
hold time. Further details of the MZI setup is described
in Appendix A 3.
C. Charlie: Bell-state measurement
Charlie consists of a 50/50 polarization-maintaining
fiber beam splitter (BS), with relevant photons from the
Alice and Bob subsystems directed to each of its inputs
via a PBSs and optical fiber. The photons are detected
at each output with an SNSPD after HPFs, with their
arrival times recorded using the DAQ as was done at
Bob. Teleportation is facilitated by measurement of the
|
Ψ
−
〉
AB
= (
|
el
〉
AB
−|
le
〉
AB
)
/
√
2 Bell state, which cor-
responds to the detection of a photon in
|
e
〉
at one de-
tector followed by the detection of a photon in
|
l
〉
at the
other detector after Alice and Bob’s (indistinguishable)
qubits arrive at the BS [54]. Projection on the
|
Ψ
−
〉
AB
state corresponds to teleportation of
|
A
〉
up to a known
local unitary transformation, i.e. our system produces
−
iσ
y
|
A
〉
, with
σ
y
being the Pauli
y
-matrix.
III. EXPERIMENTAL RESULTS
Prior to performing quantum teleportation, we mea-
sure some key parameters of our system that underpin
the teleportation fidelity. Specifically, we determine the
fidelity of the entangled state produced by Bob by mea-
suring the entanglement visibility
V
ent
[55], and also de-
termine to what extent Alice and Bob’s photons are in-
distinguishable at Charlie’s BS using the HOM effect [47].
A. Entanglement visibility
The state
|
pair
〉
B
(and hence the entangled state
|
φ
+
〉
B
) described in Sec.
II B is idealized.
In real-
ity, the state produced by Bob is better approximated
by a two-mode squeezed vacuum state
|
TMSV
〉
B
=
√
1
−
p
∑
∞
n
=0
√
p
n
|
nn
〉
B
after the FBG filter and neglect-
ing loss [56]. Here,
n
is the number of photons per tem-
poral mode (or qubit),
p
is the emission probability of
a single pair per mode (or qubit), with state ordering
referring to signal and idler modes. However,
|
TMSV
〉
B
approximates a photon pair for
p <<
1, with
p
≈
μ
B
mean number of pairs per mode (or qubit), conditioned
on measurement of a pair such that the
n
= 0 term is
eliminated. As a compromise between the pair-creation
rate
∝
p
and the quality of entanglement, here and hence-
forth we set the mean photon number of our pair source
to be
μ
B
= (8
.
0
±
0
.
4)
×
10
−
3
per time bin, which is fea-
sible because of the exceptionally low dark counts of our
SNSPDs. Measurement of
μ
B
is outlined in Appendix B.
We generate
|
φ
+
〉
B
and measure
V
ent
by directing the
idler photon to the second input port of the MZI, slightly
modifying the setup of Fig. 1. The idler photon is de-
layed compared to the signal, allowing unambiguous mea-
surement of each qubit. We vary
φ
and project each qubit
of the entangled state onto phase-varied superpositions of
|
e
〉
and
|
l
〉
by accumulating coincidence events of photons
at both the outputs of the interferometer [55].
5
The results shown in Fig. 2 are fit proportional to
1+
V
ent
sin (
ωT
+ Φ), where
V
ent
= (
R
x
−
R
n
)
/
(
R
x
+
R
n
),
with
R
x
(
n
)
denoting the maximum (minimum) rate of
coincidence events [55],
ω
and Φ are unconstrained con-
stants, and
T
is the temperature of the MZI, finding
V
ent
= 96
.
4
±
0
.
3%.
The deviation from unit visibility is mainly due to non-
zero multi photon emissions [57], which is supported by
an analytical model that includes experimental imperfec-
tions [58]. Nonetheless, this visibility is far beyond the
1
/
3 required for non-separability of a Werner state [59]
and the locality bound of 1
/
√
2 [55, 60]. Furthermore, it
predicts a fidelity
F
ent
= (3
V
ent
+ 1)
/
4 = 97
.
3
±
.
2% with
respect to
|
φ
+
〉
[59], and hence is sufficient for quantum
teleportation.
24.4
24.5
24.6
24.7
24.8
24.9
Interferometer Temperature (°C)
0
10000
20000
30000
40000
50000
60000
Coincidences / (30 min)
CQNET/FQNET Preliminary 2020
V
ent
: 96.4 ± 0.3%
FIG. 2. Entanglement visibility. The temperature of the in-
terferometer is varied to reveal the expected sinusoidal vari-
ations in the rate of coincidence events. A fit reveals the
entanglement visibility
V
ent
= 96
.
4
±
0
.
3%, see main text for
details. Uncertainties here and in all measurements are cal-
culated assuming Poisson statistics.
B. HOM interference visibility
The BSM relies on quantum interference of photons
from Alice and Bob. This is ensured by the BS at Charlie,
precise control of the arrival time of photons with IMs,
identical FBG filters, and POCs (with PBSs) to provide
the required indistinguishabiliy. The degree of interfer-
ence is quantified by way of the HOM interference visibil-
ity
V
HOM
= (
R
d
−
R
i
)
/R
d
, with
R
d
(
i
)
denoting the rate of
coincident detections of photons after the BS when the
photons are rendered as distinguishable (indistinguish-
able) as possible [47]. Completely indistinguishable sin-
gle photons from Alice and Bob may yield
V
HOM
= 1.
However in our system, Alice’s qubit is approximated
from a coherent state
|
α
〉
A
= e
−|
α
|
2
/
2
∑
∞
n
=0
α
n
√
n
!
|
n
〉
A
with
α <<
1, akin to how Bob’s pair is approximated
from
|
TMSV
〉
B
(see Sec. III A), with
μ
A
=
|
α
|
2
being
Alice’s mean photon number per mode (or qubit) [56].
Therefore, the contribution of undesired photons from
Alice and Bob lowers the maximum achievable
V
HOM
below unity, with a further reduction if the interfering
photons are not completely indistinguishable. The de-
pendence of
V
HOM
with varied
μ
A
and
μ
B
, including
effects of losses or distinguishable photons in our system
is analytically modelled in Ref. [58], and briefly discussed
in Sec. IV.
We measure
V
HOM
by slightly modifying the setup of
Fig. 1: We prepare
|
A
〉
=
|
e
〉
A
with
μ
A
= 2
.
6
×
10
−
3
and
Bob as
|
pair
〉
B
and direct Alice’s photon and Bob’s idler
to Charlie, with Bob’s signal bypassing the MZI to be di-
rectly measured by an SNSPD. Alice’s IM is used to intro-
duce distinguishability by way of a relative difference in
arrival time ∆
t
AB
of Alice and Bob’s photons at Charlie’s
BS. Using Charlie’s SNSPDs and the third detector at
Bob, a three-fold coincidence detection rate is measured
for varying ∆
t
AB
, with results shown in Fig. 3a. Since
the temporal profiles of our photons are approximately
Gaussian, we fit our results to
A
[1
−
V
HOM
exp(
−
∆
t
2
AB
2
σ
2
)],
where A is the maximum coincidence rate when the pho-
tons are completely distinguishable and
σ
= 300 ps is the
1
/e
temporal duration of the optical pulses [47, 61], find-
ing
V
HOM
= 70
.
9
±
1
.
9%. The maximum
V
HOM
for this
experiment is 83
.
5% if the photons were completely in-
distinguishable [58], with the difference ascribed to slight
distinguishability between our photons as supported by
the further measurements and analytical modelling in
Sec. IV. Improvements to our system to remove this
distinguishability is discussed in Sec. V.
To test our system for quantum teleportation over long
distances, we introduce the aforementioned 22, 11, and
11 km lengths of single-mode fiber between Alice and
Charlie, Bob and Charlie, and in the path of Bob’s signal
photon, respectively, repeat our measurement of
V
HOM
and fit the results as before (see Fig. 3b). We find
V
HOM
= 63
.
4
±
5
.
9%, which is consistent with the maxi-
mum
V
HOM
we expect when including the impact of the
additional 5.92 (2.56) dB loss between Charlie and Alice
(Bob) as well as the effect of photon distinguishability
(analyzed in Sec. IV). This suggests that the additional
fiber importantly does not introduce any further distin-
guishability (that we cannot account for), thereby sup-
porting our system’s use in quantum networking. Over-
all, the presence of clear HOM interference suggests our
system (with or without the additional fiber) introduces
relatively little imperfections that can negatively impact
the BSM and hence the fidelity of quantum teleportation.
C. Quantum teleportation
We now perform quantum teleportation of the time-
bin qubit basis states
|
e
〉
,
|
l
〉
and
|
+
〉
, so as to mea-
sure the teleportation fidelities,
F
e
,
F
l
, an
F
+
, respec-
tively, of the teleported states with respect to their ideal
counterparts, up to the local unitary introduced by the
6
600
400
200
0
200
400
600
t
AB
(ps)
50
100
150
200
250
300
Three-fold coincidences / (10 min)
a)
CQNET/FQNET Preliminary 2020
V
HOM
: 70.9 ± 1.9%
600
400
200
0
200
400
600
t
AB
(ps)
10
20
30
40
50
Three-fold coincidences / (10 min)
b)
V
HOM
: 63.4 ± 5.9%
FIG. 3. Hong-Ou-Mandel (HOM) interference. A relative dif-
ference in arrival time is introduced between photons from Al-
ice and Bob at Charlie’s BS. HOM interference produces a re-
duction of the three-fold coincidence detection rate of photons
as measured with SNSPDs after Charlie’s BS and at Bob. A
fit reveals a)
V
HOM
= 70
.
9
±
1
.
9% and b)
V
HOM
= 63
.
4
±
5
.
9%
when lengths of fiber are added, see main text for details.
BSM (see Sec. II C). Since measurement of
|
+
〉
in our
setup by symmetry is equivalent to any state of the
form (
|
e
〉
+
e
iφ
|
l
〉
)
/
√
2 (and in particular the remaining
three basis states (
|
e
〉−|
l
〉
)
/
√
2 and (
|
e
〉±
i
|
l
〉
)
/
√
2), we
may determine the average teleportation fidelity
F
avg
=
(
F
e
+
F
l
+ 4
F
+
)
/
6 of any time-bin qubit.
First, we prepare
|
e
〉
A
and
|
l
〉
A
with
μ
A
= 3
.
53
×
10
−
2
,
with Bob’s idler bypassing the MZI to be detected by
a single SNSPD. We measure
F
e
= 95
±
1% and
F
l
=
96
±
1%, conditioned on a successful measurement of
|
Ψ
−
〉
AB
at Charlie, with fidelity limited by multipho-
ton events in Alice and Bob’s qubits and dark counts
of the SNSPDs [58]. We then repeat the measurement
with
μ
A
= 9
.
5
×
10
−
3
after inserting the aforementioned
44 km length of fiber as before to emulate Alice, Charlie
and parts of Bob being separated by long distances. This
gives
F
e
= 98
±
1% and
F
l
= 98
±
2%, with no reduc-
tion from the additional fiber loss owing to our low noise
SNSPDs.
Next, we prepare
|
+
〉
A
with
μ
A
= 9
.
38
×
10
−
3
, in-
sert the MZI and, conditioned on the BSM, we measure
F
+
= (1 +
V
+
)
/
2 = 84
.
9
±
0
.
5% by varying
φ
. Here,
V
+
= 69
.
7
±
0
.
9% is the average visibility obtained by
fits to the resultant interference measured at each out-
put of the MZI, as shown in Fig. 4a. The reduction in
fidelity from unity is due to multiphoton events and dis-
tinguishability, consistent with that inferred from HOM
interference, as supported by further measurements and
analytical modelling in Sec. IV.
The measurement is repeated with the additional long
fiber, giving
V
+
= 58
.
6
±
5
.
7% and
F
+
= 79
.
3
±
2
.
9% with
results and corresponding fit shown in Fig. 4b. The re-
duced fidelity is likely due to aforementioned polarization
variations over the long fibers, consistent with the reduc-
tion in HOM interference visibility, and exacerbated here
owing to the less than ideal visibility of the MZI over long
measurement times (see Sec. A 3).
The results yield
F
avg
= 89
±
1% (86
±
3%) without
(with) the additional fiber, which is significantly above
the classical bound of 2
/
3, implying strong evidence of
quantum teleportation [62], and limited from unity by
multiphotons events, distinguishability, and polarization
variations, as mentioned [58].
To glean more information about our teleportation sys-
tem beyond the fidelity, we reconstruct the density matri-
ces of the teleported states using a maximum-likelihood
QST [48] described in Appendix C. The results of the
QST with and without the additional fiber lengths are
summarized in Figs. 8 and 9, respectively. As can be
seen, the diagonal elements for
|
+
〉
are very close to the
expected value indicating the preservation of probabili-
ties for the basis states of
|
e
〉
and
|
l
〉
after teleportation,
while the deviation of the off-diagonal elements indicate
the deterioration of coherence between the basis states.
The decoherence is attributed to multiphoton emissions
from our entangled pair source and distinguishability,
consistent with the aforementioned teleportation fideli-
ties of
|
+
〉
A
, and further discussed in Sec. IV. Finally,
we do also extract the teleportation fidelity from these
density matrices, finding the results shown in Fig. 5,
and
F
avg
= 89
±
1% (88
±
3%) without (with) the fiber
spools, which are consistent with previous measurements
given the similar
μ
A
used for QST.
We point out that the 2
/
3 classical bound may only be
applied if Alice prepares her qubits using genuine single
photons, i.e.
|
n
= 1
〉
, rather than using
|
α <<
1
〉
as we
do in this work [63]. As a way to account for the photon
statistics of Alice’s qubits we turn to an analysis using
decoy states.
1. Teleportation fidelity using decoy states
To determine the minimum teleportation fidelity of
qubits prepared using single photons, we use a decoy
7
24.2
24.4
24.6
24.8
25.0
Interferometer Temperature (°C)
0
100
200
300
400
Three-fold coincidences / (12 min)
CQNET/FQNET Preliminary 2020
a)
V
+, 1
: 69.9 ± 1.2%
0
100
200
300
400
V
+, 2
: 69.5 ± 1.2%
24.0
24.2
24.4
24.6
24.8
Interferometer Temperature (°C)
0
5
10
15
20
25
Three-fold coincidences / (40 min)
b)
V
+, 1
: 63.2 ± 9.6%
0
5
10
15
20
25
30
35
40
V
+, 2
: 54.1 ± 6.3%
FIG. 4. Quantum teleportation of
|
+
〉
. Teleportation is per-
formed b) with and a) without an additional 44 km of single-
mode fiber inserted into the system. The temperature of the
inteferometer is varied to yield a sinusoidal variation of the
three-fold coincidence rate at each output of the MZI (blue
and red points). A fit of the visibilities (see Sec. III A) mea-
sured at each output (
V
+
,
1
,
V
+
,
2
) of the MZI gives an average
visibility
V
+
= (
V
+
,
1
+
V
+
,
2
)
/
2 of a) 69
.
7
±
0
.
91% without the
additional fiber and b) 58
.
6
±
5
.
7% with the additional fiber.
state method [49] and follow the approach of Refs.
[29, 64].
Decoy states, which are traditionally used
in quantum key distribution to defend against photon-
number splitting attacks, are qubits encoded into co-
herent states
|
α
〉
with varying mean photon number
μ
A
=
|
α
|
2
. Measuring fidelities of the teleported qubits
for different
μ
A
, the decoy-state method allows us to cal-
culate a lower bound
F
d
A
on the teleportation fidelity if
Alice had encoded her qubits using
|
n
= 1
〉
.
We prepare decoy states
|
e
〉
A
,
|
l
〉
A
, and
|
+
〉
A
with vary-
ing
μ
A
, as listed in Table I, and perform quantum telepor-
tation both with and without the added fiber, with tele-
portation fidelities shown in Table I. From these results
we calculate
F
d
A
as shown in Fig. 5, with
F
d
avg
≥
93
±
4%
(
F
d
avg
≥
89
±
2%) without (with) the added fiber, which
significantly violate the classical bound and the bound
of 5
/
6 given by an optimal symmetric universal cloner
[65, 66], clearly demonstrating the capability of our sys-
|
e
|
l
| +
Average
0.0
0.2
0.4
0.6
0.8
1.0
1.2
Fidelity
99.2±0.6%
97.9±1.3%
90.3±5.9%
93.0±3.9%
95.2±1.2%
95.9±1.3%
85.0±1.6%
88.5±1.1%
a)
CQNET/FQNET Preliminary 2020
Single-photon fidelity from DSM
Fidelity from QST
|
e
|
l
| +
Average
0.0
0.2
0.4
0.6
0.8
1.0
1.2
Fidelity
98.6±0.9%
98.4±0.9%
84.5±3.3%
89.2±2.2%
98.6±0.6%
96.2±1.9%
83.1±5.0%
87.9±3.3%
b)
Single-photon fidelity from DSM
Fidelity from QST
FIG. 5. Quantum teleportation fidelities for
|
e
〉
A
,
|
l
〉
A
, and
|
+
〉
A
, including the average fidelity. The dashed line rep-
resents the classical bound. Fidelities using quantum state
tomography (QST) are shown using blue bars while the min-
imum fidelities for qubits prepared using
|
n
= 1
〉
,
F
d
e
,
F
d
l
,
and
F
d
+
, including the associated average fidelity
F
d
avg
, respec-
tively, using a decoy state method (DSM) is shown in grey.
Panels a) and b) depicts the results without and with addi-
tional fiber, respectively. Uncertainties are calculated using
Monte-Carlo simulations with Poissonian statistics.
tem for high-fidelity teleportation. As depicted in Fig.
5 these fidelities nearly match the results we obtained
without decoy states within statistical uncertainty. This
is due to the suitable
μ
A
, as well as low
μ
B
and SNSPD
dark counts in our previous measurements [58].
IV. ANALYTICAL MODEL AND SIMULATION
As our measurements have suggested, multi-photon
components in, and distinguishability between, Alice and
Bob’s qubits reduce the values of key metrics includ-
ing HOM interference visibility and, consequently, quan-
tum teleportation fidelity. To capture these effects in
our model, we employ a Gaussian-state characteristic-
function method developed in Ref. [58], which was en-
8
qubit
without long fiber
with long fiber
μ
A
(
×
10
−
3
)
F
d
A
(%)
μ
A
(
×
10
−
3
)
F
d
A
(%)
|
e
〉
A
3.53
95.2
±
1
26.6
95.7
±
1.5
1.24
86.7
±
2
9.01
98.4
±
1.1
0
52.8
±
3.4
-
-
|
l
〉
A
3.53
95.9
±
1
32.9
98.6
±
0.7
1.24
90.5
±
2
9.49
98.4
±
1.6
0
52.8
±
3.4
-
-
|
+
〉
A
9.38
84.7
±
1.1
29.7
73.6
±
3.0
2.01
83.2
±
3.6
10.6
82.21
±
3.9
0
52.8
±
3.4
-
-
TABLE I. Teleportation fidelities with (right column) and
without (center column) the 44 km-length of fiber for Alice’s
qubit states prepared with varying
μ
A
. Mean photon numbers
and fidelities for vacuum states with fiber are assumed to be
zero and 50%, respectively.
abled by work in Ref. [67]. This approach is well-suited
to analyze our system because the quantum states, oper-
ations, and imperfections (including losses, dark counts,
etc.) of the experiment can be fully described using
Gaussian operators, see e.g. Ref. [68]. We now briefly
outline the model of Ref. [58], and employ it to estimate
the amount of indistinguishability
ζ
between Alice and
Bob’s qubits in our measurements of HOM interference
and quantum teleportation.
Distinguishability in any degree-of-freedom may be
modelled by introducing a virtual beam splitter of trans-
mittance
ζ
into the paths of Alice and Bob’s relevant pho-
tons. As shown in Fig. 6, indistinguishable components
of incoming photon modes are directed towards Charlie’s
BS where they interfere, whereas distinguishable compo-
nents are mixed with vacuum at the BS and do not con-
tribute to interference. Here
ζ
= 1 (
ζ
= 0) corresponds
to the case when both incoming photons are perfectly
indistinguishable (distinguishable). Now we may calcu-
late the probability of a three-fold coincidence detection
event
P
3
f
between
D
1
,
D
2
(Charlies’ detectors), and
D
3
FIG. 6. Schematic depiction of distingushability between Al-
ice and Bob’s photons at Charlie’s BS. Distinguishability is
modeled by means of a virtual beam splitter with a transmit-
tance
ζ
. Indistinguishable photons contribute to interference
at the Charlie’s BS while distinguishable photons are mixed
with vacuum, leading to a reduction of HOM visibility and
teleportation fidelity. See main text for further details.
(detects Bob’s signal photon) for a given qubit state
ρ
AB
from Alice and Bob:
P
3
f
= Tr
{
ρ
AB
(
I
−
(
|
0
〉〈
0
|
)
⊗
3
ˆ
a
1
,
ˆ
a
2
,
ˆ
a
3
)
⊗
(
I
−
(
|
0
〉〈
0
|
)
⊗
3
ˆ
b
1
,
ˆ
b
2
,
ˆ
b
3
)
⊗
(
I
−
(
|
0
〉〈
0
|
)
ˆ
c
)
}
,
(1)
where the ˆ
a
and
ˆ
b
operators refer to modes, which origi-
nate from Alice and Bob’s virtual beam splitters and are
directed to
D
1
and
D
2
, respectively, and ˆ
c
corresponds
to Bob’s idler mode, which is directed to
D
3
, see Fig. 6.
This allows the derivation of an expression for the HOM
interference visibility
V
HOM
(
ζ
) = [
P
3
f
(0)
−
P
3
f
(
ζ
)]
/P
3
f
(0)
,
(2)
consistent with that introduced in Sec.
III B. Since
Alice and Bob ideally produce
ρ
AB
= (
|
α
〉〈
α
|
)
⊗
(
|
TMSV
〉〈
TMSV
|
), and recognizing that all operators in
P
3
f
are Gaussian, we analytically derive
P
3
f
(
ζ
) = 1
−
2
exp(
−
μ
A
/
2[1+(1
−
ζ
2
)
η
i
μ
B
/
2]
1+
η
i
μ
B
/
2
)
1 +
η
i
μ
B
/
2
−
1
1 +
η
s
μ
B
+
exp(
−
μ
A
)
1 +
η
i
μ
B
−
exp(
−
μ
A
)
1 + (1
−
η
s
)
η
i
μ
B
+
η
s
μ
B
+ 2
exp(
−
μ
A
/
2[1+(1
−
ζ
2
)(1
−
η
s
)
η
i
μ
B
/
2+
η
s
μ
B
]
1+(1
−
η
s
)
η
i
μ
B
/
2+
η
s
μ
B
)
1 + (1
−
η
s
)
η
i
μ
B
/
2 +
η
s
μ
B
,
(3)
for varied
ζ
, where
η
i
and
η
s
are the transmission ef-
ficiencies of the signal and idler photons, including de-
tector efficiencies. We similarly calculate the impact of
distinguishability on the teleportation fidelity of
|
+
〉
:
F
(
ζ
) =
P
3
f
(
ζ,φ
max
)
/
[
P
3
f
(
ζ,φ
max
) +
P
3
f
(
ζ,φ
min
)]
,
(4)
where
φ
max
(
φ
min
) is the phase of the MZI added into
the path of the signal photon, corresponding to maximum
9
(minimum) three-fold detection rates.
To compare the model to our measurements, we use the
experimental mean photon numbers for the photon-pair
source
η
i
= 1
.
2
×
10
−
2
and
η
s
= 4
.
5
×
10
−
3
as deter-
mined by the method described in Appendix B. We then
measure the teleportation fidelity of
|
+
〉
and HOM inter-
ference visibility (keeping the MZI in the system to en-
sure
η
s
remains unchanged) for different values
μ
A
. The
results are plotted in Fig. 7. The data is then fitted to
the expressions
V
HOM
(
ζ
) and
F
(
ζ
) derived in our model
and graphed in Fig. 7. The fitted curves are in very good
agreement with our experimental values and consistently
yield a value of
ζ
= 90% for both measurements types.
This implies that we have only a small amount of resid-
ual distinguishability between Alice and Bob’s photons.
Potential effects leading to this distinguishability are dis-
cussed in Sec. V.
Overall, our analytic model is consistent with our ex-
perimental data [58] in the regime of
μ
A
<<
1, which
is the parameter space most often used in quantum net-
working protocols (e.g. key distribution). Our model,
thus, offers a practical way to determine any underlying
distinguishability in a deployed network where a full char-
acterization of the properties of Alice and Bob’s photons
may not be possible.
V. DISCUSSION AND OUTLOOK
We have demonstrated quantum teleportation systems
for photonic time-bin qubits at a quantum channel- and
device-compatible wavelength of 1536.5 nm using a fiber-
based setup comprising state-of-the-art SNSPDs and off-
the-shelf components. We measure an average fidelity
above 90% using QST and a decoy state analysis with up
to 44 km of single mode fiber in our setup. Our results
are further supported by an analytical model in conjunc-
tion with measurements of the entanglement and HOM
interference visibilities.
The decoy state analysis indicates that the maximum
teleportation fidelity is currently restricted by that of
the teleported qubits prepared in superposition states,
for which a 10% distinguishability between the qubits
undergoing BSM and the contribution of multiple pho-
ton pairs play the largest role. Our model predicts that
the average fidelity will increase to 95% with completely
indistinguishable photons, while fidelities close to unity
can be achieved with lowered mean number of photon
pairs. Alternatively, we may replace our SNSPDs with
efficient photon-number resolving (PNR) SNSPDs [69] to
allow postselection of multiphoton events at the MZI or
BSM [70]. Both approaches must be accompanied by
increased coupling efficiencies of the pair source beyond
the current
∼
1% either to maintain realistic teleporta-
tion rates (above the system noise and current rate of
phase drift of the MZI), or to derive any advantage from
PNR capability.
As suggested by the width of our HOM interference
FIG. 7. Evaluation of photon indistinguishability using an
analytical model. Panel a) depicts the quantum teleportation
fidelity of
|
+
〉
while panel b) shows the HOM interference vis-
ibility, each with varied mean photon number
μ
A
of Alice’s
qubits. Fits of analytical models the data reveal
ζ
= 90% in-
distinguishability between Alice and Bob’s photons at Char-
lie’s BS. Bob produces
μ
B
photon pairs on average,
η
i
and
η
s
are the probabilities for an individual idler (signal) photon
to arrive at Charlie’s BS and be detected at Bob’s detector,
respectively.
fringe – which predicts an average photon bandwidth of
0
.
44
/σ
∼
1.5 GHz (see Sec. III B), i.e. less than the
2 GHz bandwidth of our FBGs – the indistinguishabil-
ity in our system could be limited by the large differ-
ence in the bandwidth between the photons originating
from the SPDC (
>
100 GHz) and those generated at Al-
ice by the IM (15 GHz), leading to nonidentical filtering
by the FBG. This can be improved by narrower FBGs
or by using a more broadband pump at Alice (e.g. us-
ing a mode locked laser or a higher bandwidth IM, e.g
>
50 GHz, which is commercially available). Alternatively,
pure photon pairs may be generated by engineered phase
matching, see e.g. Ref. [71]. Distinguishability owing to
nonlinear modulation during the SHG process could also
play a role [72]. The origin of distinguishability in our
system, whether due to imperfect filtering or other device
imperfections (e.g. PBS or BS) will be studied in future
work. Coupling loss can be minimized to less than a
few dB overall by improved fiber-to-chip coupling, lower-
loss components of the FBGs (e.g. the required isolator),
spliced fiber connections, and reduced losses within our
MZI. Note that our current coupling efficiency is equiva-
lent to
∼
50 km of single mode fiber, suggesting that our
system is well-suited for quantum networks provided loss
10
is reduced.
While the fidelities we demonstrate are sufficient for
several applications, the current
∼
Hz teleportation rates
with the 44 km length of fiber are still low. Higher repe-
tition rates (e.g. using high-bandwidth modulators with
wide-band wavelength division multiplexed filters and
low-jitter SNSPDs [73]), improvements to coupling and
detector efficiencies, enhanced BSM efficiency with fast-
recovery SNSPDs [74], or multiplexing in frequency [64]
will all yield substantial increases in teleportation rate.
Note that increased repetition rates permits a reduction
in time bin separation which will allow constructing the
MZI on chip, providing exceptional phase stability and
hence, achievable fidelity. Importantly, the aforemen-
tioned increases in repetition rate and efficiency are af-
forded by improvements in SNSPD technology that are
currently being pursued with our JPL, NIST and other
academic partners.
Upcoming system-level improvements we plan to in-
vestigate and implement include further automation by
the implementation of free-running temporal and polar-
ization feedback schemes to render the photons indistin-
guishable at the BSM [29, 30]. Furthermore, several elec-
trical components can be miniaturized, scaled, and made
more cost effective (e.g. field-programmable gate arrays
can replace the AWG).We note that our setup prototype
will be easily extended to independent lasers at different
locations, also with appropriate feedback mechanisms for
spectral overlap [75, 76]. These planned improvements
are compatible with the data acquisition and control sys-
tems that were built for the systems and experiments at
FQNET and CQNET presented in this work.
Overall, our high-fidelity teleportation systems achiev-
ing state-of-the-art teleporation fidelities of time-bin
qubits serve as a blueprint for the construction of quan-
tum network test-beds and eventually global quantum
networks towards the quantum internet. In this work,
we present a complete analytical model of the telepora-
tion system that includes imperfections, and compare it
with our measurements. Our implementation, using ap-
proaches from High Energy Physics experimental systems
and real-world quantum networking, features near fully-
automated data acquisition, monitoring, and real-time
data analysis. In this regard our Fermilab and Caltech
Quantum Networks serve as R& D laboratories and pro-
totypes towards real-world quantum networks. The high
fidelities achieved in our experiments using practical and
replicable devices are essential when expanding a quan-
tum network to many nodes, and enable the realization
of more advanced protocols, e.g. [18, 77, 78].
ACKNOWLEDGEMENTS
R.V., N.L., L.N., C.P., N.S., M.S. and S.X. acknowl-
edge partial and S.D. full support from the Alliance
for Quantum Technologies (AQT) Intelligent Quantum
Networks and Technologies (IN-Q-NET) research pro-
gram.
R.V., N.L., L.N., C.P., N.S., M.S. S.X. and
A.M. acknowledge partial support from the U.S. De-
partment of Energy, Office of Science, High Energy
Physics, QuantISED program grant, under award num-
ber de-sc0019219. A.M. is supported in part by the
JPL President and Directors Research and Develop-
ment Fund (PDRDF). C.P. further acknowledges par-
tial support from the Fermilab’s Lederman Fellowship
and LDRD. D.O. and N.S. acknowledge partial sup-
port from the Natural Sciences and Research Council of
Canada (NSERC). D.O. further acknowledges the Cana-
dian Foundation for Innovation, Alberta Innovates, and
Alberta Economic Development, Trade and Tourisms
Major Innovation Fund. J.A. acknowledges support by
a NASA Space Technology Research Fellowship. Part
of the research was carried out at the Jet Propulsion
Laboratory, California Institute of Technology, under a
contract with the National Aeronautics and Space Ad-
ministration (80NM0018D0004). We thank Jason Trevor
(Caltech Lauritsen Laboratory for High Energy Physics),
Nigel Lockyer and Joseph Lykken (Fermilab), Vikas
Anant (PhotonSpot), Aaron Miller (Quantum Opus), In-
der Monga and his ESNET group at LBNL, the groups of
Wolfgang Tittel and Christoph Simon at the University
of Calgary, the groups of Nick Hutzler, Oskar Painter,
Andrei Faraon, Manuel Enders and Alireza Marandi
at Caltech, Marko Loncar’s group at Harvard, Ar-
tur Apresyan and the HL-LHC USCMS-MTD Fermilab
group; Marco Colangelo (MIT); Tian Zhong (Chicago);
AT&T’s Soren Telfer, Rishi Pravahan, Igal Elbaz, Andre
Feutch and John Donovan. We acknowledge the enthusi-
astic support of the Kavli Foundation on funding QIS&T
workshops and events and the Brinson Foundation sup-
port especially for students working at FQNET and
CQNET. M.S. is especially grateful to Norm Augustine
(Lockheed Martin), Carl Williams (NIST) and Joe Broz
(SRI, QED-C); Hartmut Neven (Google Venice); Amir
Yacoby and Misha Lukin (Harvard); Ned Allen (Lock-
heed Martin); Larry James and Ed Chow (JPL); the
QCCFP wormhole teleportation team especially Daniel
Jafferis (Harvard) and Alex Zlokapa (Caltech), Mark Ka-
sevich (Stanford), Ronald Walsworth (Maryland), Jun
Yeh and Sae Woo Nam (NIST); Irfan Siddiqi (Berkeley);
Prem Kumar (Northwestern), Saikat Guha (Arizona),
Paul Kwiat (UIUC), Mark Saffman (Wisconcin), Jelena
Vuckovic (Stanford) Jack Hidary (X), and the quantum
networking teams at ORNL, ANL, and BNL, for produc-
tive discussions and interactions on quantum networks
and communications.
Appendix A: Detailed description of experimental
components
1. Control systems and data acquisition
Our system is built with a vision towards future repli-
cability, with particular emphasis on systems integra-
11
tion. Each of the Alice, Bob and Charlie subsystems
is equipped with monitoring and active feedback stabi-
lization systems (e.g. for IM extinction ratio), or has ca-
pability for remote control of critical network parameters
(e.g. varying the qubit generation time). Each subsystem
has a central classical processing unit with the following
functions: oversight of automated functions and work-
flows within the subsystem, data acquisition and man-
agement, and handling of input and output synchroniza-
tion streams. As the quantum information is encoded
in the time domain the correct operation of the classical
processing unit depends critically on the recorded time-
of-arrival of the photons at the SNSPDs. Thus signifi-
cant effort was dedicated to build a robust DAQ subsys-
tem capable of recording and processing large volumes of
time-tagged signals from the SNSPDs and recorded by
our TDCs at a high rate. The DAQ is designed to en-
able both real-time data analysis for prompt data quality
monitoring as well as post-processing data analysis that
allows to achieve the best understanding of the data.
The DAQ system is built on top of the standalone
Linux library of our commercial TDC. It records time
tags whenever a signal is detected in any channel in co-
incidence with the reference 90 MHz clock. Time tags
are streamed to a PC where they are processed in real-
time and stored to disk for future analysis. A graphical
user interface has been developed, capable of real-time
visualization and monitoring of photons detected while
executing teleportation. It also allows for easy control of
the time-intervals used for each channel and to configure
relevant coincidences between different photon detection
events across all TDC channels. We expect our DAQ sub-
system to serve as the foundation for future real-world
time-bin quantum networking experiments (see Sec. V).
2. Superconducting nanowire single photon
detectors
We employ amorphous tungsten silicide SNSPDs man-
ufactured in the JPL Microdevices Laboratory for all
measurements at the single photon level (see Sec. II B)
[52]. The entire detection system is customized for opti-
mum autonomous operation in a quantum network. The
SNSPDs are operated at 0.8 K in a closed-cycle sorption
fridge [53]. The detectors have nanowire widths between
140 to 160 nm and are biased at a current current of 8
to 9
μ
A. The full-width at half maximum (FWHM) tim-
ing jitter (i.e. temporal resolution) for all detectors is
between 60 and 90 ps (measured using a Becker & Hickl
SPC-150NXX time-tagging module). The system detec-
tion efficiencies (as measured from the fiber bulkhead of
the cryostat) are between 76 and 85 %. The SNSPDs fea-
ture low dark count rates between 2 and 3 Hz, achieved by
short-pass filtering of background black-body radiation
through coiling of optical fiber to a 3 cm diameter within
the 40 K cryogenic environment, and an additional band-
pass filter coating deposited on the detector fiber pigtails
(by Andover Corporation). Biasing of the SNSPDs is fa-
cilitated by cryogenic bias-Ts with inductive shunts to
prevent latching, thus enabling uninterrupted operation.
The detection signals are amplified using Mini-Circuits
ZX60-P103LN+ and ZFL-1000LN+ amplifiers at room
temperature, achieving a total noise figure of 0.61 dB
and gain of 39 dB at 1 GHz, which enables the low sys-
tem jitter. Note that FWHM jitter as low as 45 ps is
achievable with the system, by biasing the detectors at
approximately 10
μ
A, at the cost of an elevated DCR on
the order of 30 cps. Using commercially available com-
ponents, the system is readily scalable to as many as 64
channels per cryostat, ideal for star-type quantum net-
works, with uninterrupted 24/7 operation. The bulkiest
component of the current system is an external helium
compressor, however, compact rack-mountable versions
are readily available [53].
3. Interferometer and phase stabilization
We use a commercial Kylia 04906-MINT MZI, which
is constructed of free-space devices (e.g mirrors, beam
spliters) with small form-factor that fits into a hand-held
box. Light is coupled into and out of the MZI using
polarization maintaining fiber with loss of
∼
2.5 dB. The
interferometer features an average visibility of 98.5% that
was determined by directing
|
+
〉
with
μ
A
= 0
.
07 into one
of the input ports, measuring the fringe visibility on each
of the outputs using an SNSPD. The relative phase
φ
is
controlled by a voltage-driven heater that introduces a
small change in refractive index in one arm of the MZI.
However, this built-in heater did not permit phase stabil-
ity sufficient to measure high-fidelity teleportation, with
the relative phase following the slowly-varying ambient
temperature of the room. To mitigate this instability,
we built another casing, thermally isolating the MZI en-
closure from the laboratory environment and controlled
the temperature via a closed-loop feedback control sys-
tem based on a commercial thermoelectric cooler and a
LTC1923 PID-controller. The temperature feedback is
provided by a 10 kΩ NTC thermistor while the set-point
is applied with a programmable power supply. This con-
trol system permits us to measure visbilities by slowly
varying
φ
over up to 15 hour timescales. We remark
that no additional methods of phase control were used
beyond that of temperature.
Appendix B: Estimation of mean number of photon
pairs and transmission efficiencies of signal and idler
photons
Using a method described in Ref. [55], we measure
the mean number of photon pairs produced by Bob
μ
B
as a function of laser excitation power before the PPLN
waveguide used for SHG. To this end, we modify the
setup of Fig. 1 and direct each of Bob’s signal and idler