True on-demand high-repetition-rate single-photon sources are highly sought after for quantum information processing applications. However, any coherently driven two-level quantum system suffers from a finite re-excitation probability under pulsed excitation, causing undesirable multi-photon emission. Here, we present a solid-state source of on-demand single photons yielding a raw second-order coherence of g(2)(0)=(7.5±1.6)×105 without any background subtraction or data processing. To this date, this is the lowest value of g(2)(0) reported for any single-photon source even compared to the previously reported best background subtracted values. We achieve this result on GaAs/AlGaAs quantum dots embedded in a low-Q planar cavity by employing (i) a two-photon excitation process and (ii) a filtering and detection setup featuring two superconducting single-photon detectors with ultralow dark-count rates of (0.0056±0.0007) s−1 and (0.017±0.001) s−1, respectively. Re-excitation processes are dramatically suppressed by (i), while (ii) removes false coincidences resulting in a negligibly low noise floor.

Recently, scientific and industrial interest in quantum simulation, computation, and communication applications has considerably increased.1 In the field of quantum information processing and communication,2 single photons have emerged as ideal candidates for quantum information carriers (flying qubits) due to their small interaction cross-section. Applications with particularly stringent requirements on the second-order coherence are current protocols in cluster-state computation and the realization of an all-optical quantum repeater.3 Like fiber amplifiers in classical optical long-distance communication, quantum repeaters have to be employed to increase the range over which a quantum channel can reliably function. A lower multi-photon emission rate allows for a higher number of consecutive repeater nodes without negatively affecting the secret-key rate, therefore allowing longer distance communication.4,5 Current single-photon sources include trapped atoms, heralded spontaneous parametric down conversion sources, color centers and the emerging field of 2D materials, as well as semiconductor quantum dots (QDs).3 Spontaneous parametric down conversion sources offer room temperature operation but suffer from intrinsic multi-photon emission scaling with the emission rate.6 The lowest second-order coherence at time delay zero demonstrated with natural atoms is g(2)(0)=(3±1.5)×104 with background subtraction.7 However, these systems typically suffer from a low repetition rate, limited by their intrinsically long lifetime. Compared to natural atoms and ions, optically active semiconductor quantum dots are scalable, nano-fabricated, high repetition rate single-photon sources with tailorable optical properties.8 QDs under direct resonant excitation have only shown g(2)(0)=(2.8±1.2)×103 with background subtraction.9 The reason for this is that a residual multi-photon emission probability cannot be fully suppressed under direct resonant pulsed excitation of the excited state [exciton (X) or charged exciton].10–12 This holds true for all quantum mechanical two-level systems. Addressing a QD via a third level should result in an even lower multi-photon emission probability due to suppressed re-excitation processes. However, this has only been demonstrated using temporal post-selection of coincidence events, yielding g(2)(0)=(4.4±0.2)×104.13 In this work, we employ two-photon resonant excitation of the biexciton (XX) state,14,15 strongly suppressing multi-photon emission of our quantum dot and thereby reaching an unprecedented second-order coherence of g(2)(0)=(7.5±1.6)×105.

The QD sample was grown by molecular beam epitaxy at Johannes Kepler University Linz. The QD layer is obtained by Al-droplet etching16,17 on Al0.4Ga0.6As followed by deposition of 2 nm GaAs. This technique allows the fabrication of highly symmetric QDs with measured entanglement fidelities of up to 94%.18 The QD layer is placed at the center of a λ-cavity made of a λ/2-thick (123 nm) layer of Al0.4Ga0.6As sandwiched between two λ/4-thick (59.8 nm) Al0.2Ga0.8As layers. The cavity sits on top of a distributed Bragg reflector made of 9 pairs of λ/4-thick Al0.95Ga0.05As (68.9 nm) and Al0.2Ga0.8As layers and below two pairs of the same material combination. A 4 nm-thick GaAs protective layer completes the structure. The QD emission is centered around ∼790 nm, and a gradient in the mode position (Q factor of about 50) is obtained by stopping the substrate rotation during the deposition of the top Al0.2Ga0.8As cavity-layer. This simple cavity design enhances the extraction efficiency by ∼15 times compared to an unstructured sample. As illustrated in Fig. 1(a), the sample is cooled to about 4 K in a closed-cycle cryostat. Inside the cryostat, we use an aspheric lens with a working distance of 4.93 mm to focus the excitation laser under a slight angle through a solid immersion lens in the Weierstraß geometry and onto the QD under investigation. 90% of the confocally collected photoluminescence then passes the non-polarizing beam splitter we use to couple in the pulse-stretched excitation laser with a repetition rate of 80.028 MHz. As shown in Fig. 1(b), we tune a pulsed laser to an energy corresponding to half the energy difference between the ground state and the biexciton state in order to resonantly address the biexciton state of the QD with a two-photon process.19,20 In the case of the quantum dot under investigation, this corresponds to a laser wavelength of 793.8 nm. Using a pulse shaper, we create a laser pulse with a spectral width of 260 μeV, measured with a spectrum analyzer and a pulse length of 7 ps, measured with an auto-correlator assuming a Gaussian pulse shape. The peak power density of a π-pulse is 96 kW cm−2, and the scattered laser light is subsequently filtered. Since, in the case of two-photon resonant excitation [see Fig. 1(b), bottom], the excitation energy is detuned from the emission energies of both XX and X, we can suppress the laser spectrally. After the beam splitter, we use tunable notch filters (FWHM = 0.4 nm; extinction ratio ∼30 dB) mounted on stepper motors to selectively block laser light before we couple into an optical fiber. The fiber core with a diameter of 4.4 μm acts as a spatial filter. In addition, we employ polarization suppression by cross-polarizing excitation and detection photons.21 Furthermore, a transmission spectrometer with a bandwidth of 22 pm and an end-to-end efficiency of 60% suppresses the remaining light at all wavelengths, except for the XX photons. Specifically, the laser, spectrally detuned by 0.9 nm with respect to the XX wavelength, is suppressed by 86 dB. We then use a fiber based 50:50 beam splitter to send the photons onto two superconducting single-photon detectors (SSPDs), with a FWHM timing jitter of 20 ps and 30 ps and dark count rates of (0.0056 ± 0.0007) s−1 and (0.017±0.001) s−1, to perform a start–stop measurement. At these settings and for the biexciton wavelength of ∼795 nm, our detectors still perform with detection efficiencies of 50% and 64%, respectively.

FIG. 1.

(a) Confocal micro-photoluminescence spectroscopy setup with pulse-slicer, closed-cycle cryostat, polarization suppression, transmission spectrometer, and superconducting single-photon detectors (SSPDs). Additional optical components: reflection grating (RG), polarizer (Pol), beamsplitter (BS), quarter waveplate (QWP), aspheric lens (AL), solid immersion lens (SIL), notch filter (NF), transmission grating (TG), and fiber beamsplitter (FBS). (b) Two-photon excitation scheme to resonantly excite the biexciton state with two laser photons (orange). Top: Three level energy scheme of the biexciton–exciton cascade. Bottom: Visualization of the two-photon excitation spectrum.

FIG. 1.

(a) Confocal micro-photoluminescence spectroscopy setup with pulse-slicer, closed-cycle cryostat, polarization suppression, transmission spectrometer, and superconducting single-photon detectors (SSPDs). Additional optical components: reflection grating (RG), polarizer (Pol), beamsplitter (BS), quarter waveplate (QWP), aspheric lens (AL), solid immersion lens (SIL), notch filter (NF), transmission grating (TG), and fiber beamsplitter (FBS). (b) Two-photon excitation scheme to resonantly excite the biexciton state with two laser photons (orange). Top: Three level energy scheme of the biexciton–exciton cascade. Bottom: Visualization of the two-photon excitation spectrum.

Close modal

In order to verify that we are addressing our quantum system coherently via two-photon excitation, we investigate the power dependence of the photoluminescence. Figure 2 is a color plot showing spectra of the QD including both the X and XX emission for different excitation pulse areas. Blue corresponds to low intensity, whereas red corresponds to high intensity. The observed Rabi-oscillations of the intensity reflect an oscillation in the population of the excited state (XX) and indicate that the system is coherently driven by the excitation light field without the need for any additional off-resonant light field.22 To the left (right) of the color plot, we show the integrated intensity of the exciton (biexciton) transition as a function of the excitation pulse area. The quadratic power dependence of the state population reflects the two-photon nature of the excitation process, clearly visible in the initial rise. Below the color plot, we show an exemplary spectrum excited with a pulse area corresponding to the maximum population inversion probability (π-pulse) indicated by the horizontal dashed white line in the color plot. The small peak next to the biexciton has a linear dependence on the laser pulse area and could not be attributed to a specific quantum dot transition.

FIG. 2.

Color-coded photoluminescence spectra of the biexciton–exciton cascade under resonant two-photon excitation as a function of the excitation pulse area. Integrated peak intensity of the X (XX) emission is shown to the left (right) of the color map, undergoing Rabi-oscillations. The spectrum shown in the bottom is excited with a pulse area corresponding to a π-pulse and is indicated by the horizontal dashed line.

FIG. 2.

Color-coded photoluminescence spectra of the biexciton–exciton cascade under resonant two-photon excitation as a function of the excitation pulse area. Integrated peak intensity of the X (XX) emission is shown to the left (right) of the color map, undergoing Rabi-oscillations. The spectrum shown in the bottom is excited with a pulse area corresponding to a π-pulse and is indicated by the horizontal dashed line.

Close modal

To investigate the multi-photon emission probability of our source, we record coincidences of XX photons between both output ports of a 50:50 beam splitter binned in time windows of 16 ps. In Fig. 3(a), we show the resulting histogram approximating a pulsed second-order intensity autocorrelation g(2)(τ)-function. The distance between the side peaks is 12.496 ns corresponding to the laser repetition rate. In order to analyze our multi-photon emission probability, we compare the amount of coincidences from consecutive excitation pulses with the amount of coincidences within the same pulse. We choose a time window of 5 ns, ∼40 times longer than the XX lifetime of 125 ps (where the accuracy is limited by the detector time jitter of 20 ps) to avoid temporal post-selection. In this time window, we sum up the coincidences to find an average of 279171 ± 187 events per side peak in a sample of 8 side peaks after integrating for 10 h. The error is propagated quadratically from the square root of the counts in each individual side peak, assuming Poissonian counting statistics. In Fig. 3(b), we show a 5 ns window centered around τ = 0 with only 21 ± 5 coincidence events, where the error is the square root of the coincidences, leading to a value of g(2)(0)=(7.5±1.6)×105. The error is based on the statistical error and was calculated using quadratic error propagation. Given our low g(2)(0) value together with a detected single-photon count rate of (60 ± 5) kcts/s, we were able to experimentally verify the quantum non-Gaussian character23,24 of the single photons emitted from our semiconductor quantum dot. We find a non-Gaussian depth of 5.2 ± 1.5 dB using the expressions of Ref. 25.

FIG. 3.

(a) Measured second-order autocorrelation function of the biexciton under π-pulse two-photon excitation. An average side peak contains 279 171 ± 187 coincidences. (b) 5 ns wide zoom-in around τ = 0, showing a total of 21 ± 5 coincidences. We use this time window for the calculation of the g(2)(0) value.

FIG. 3.

(a) Measured second-order autocorrelation function of the biexciton under π-pulse two-photon excitation. An average side peak contains 279 171 ± 187 coincidences. (b) 5 ns wide zoom-in around τ = 0, showing a total of 21 ± 5 coincidences. We use this time window for the calculation of the g(2)(0) value.

Close modal

We would like to note that cross-polarization of the emission and detection photons helps to lower the measured second-order coherence function at time delay zero from g(2)(0)=(4.6±0.5)×104 to the stated record value. This is due to finite laser intensity at the XX energy and spatial position of the fiber core. The main reason for the low multi-photon emission probability is the previously described two-photon excitation technique directly addressing the transition from the ground state to the XX state. Unlike with resonant excitation of the X state, where re-excitation can directly occur after the initial emission of the single photon, re-excitation is strongly suppressed in the case of two-photon excitation. Re-excitation can only occur once the system has returned to the ground state - a condition that is delayed by the X state's lifetime of ∼210 ps. By the time the system has completed its cascaded decay, the intensity of the excitation laser pulse is much lower than it would be after only a single decay. A theoretical model of this re-excitation suppression has now been developed during the editorial process of our work.26 In addition, a lowered excitation laser intensity corresponds to a quadratically lowered re-excitation probability, due to the two-photon nature of the excitation.27 

In summary, we have shown a single-photon source with unprecedentedly low multi-photon emission. Measuring g(2)(0)=(7.5±1.6)×105 without any background subtraction or temporal post-selection was possible due to two key factors: a low dark coincidence count rate of our SSPDs (0 events in 48 h) and a suppressed re-excitation probability during the lifetime of the X made possible by two-photon resonant excitation of the XX state. This highlights semiconductor quantum dots resonantly excited with a two-photon process as ideal candidates for all-optical quantum repeaters, cluster state computation, and other applications where low multi-photon emission is of crucial importance.

K.D.J. acknowledges funding from the MARIE SKŁODOWSKA-CURIE Individual Fellowship under REA Grant Agreement No. 661416 (SiPhoN). K.D.Z. gratefully acknowledges funding by the Dr. Isolde Dietrich Foundation. This work was financially supported by the European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme (SPQRel, Grant Agreement No. 679183 and NaQuOp, Grant Agreement No. 307687), the Swedish Research Council under Grant Agreement No. 638-2013-7152, the Austrian Science Fund (FWF): P29603, and the Linnaeus Center in Advanced Optics and Photonics (Adopt). The JKU group acknowledges V. Volobuev, Y. Huo, P. Atkinson, G. Weihs, and B. Pressl for fruitful discussions. The Quantum Nano Photonics group at KTH acknowledges the continuous support by the companies APE Angewandte Physik und Elektronik GmbH on their picoEmerald system and Single Quantum BV on their SSPDs.

1.
M. F.
Riedel
,
D.
Binosi
,
R.
Thew
, and
T.
Calarco
,
Quantum Sci. Technol.
2
,
030501
(
2017
).
2.
P.
Zoller
,
T.
Beth
,
D.
Binosi
,
R.
Blatt
,
H.
Briegel
,
D.
Bruss
,
T.
Calarco
,
J. I.
Cirac
,
D.
Deutsch
,
J.
Eisert
,
A.
Ekert
,
C.
Fabre
,
N.
Gisin
,
P.
Grangiere
,
M.
Grassl
,
S.
Haroche
,
A.
Imamoglu
,
A.
Karlson
,
J.
Kempe
,
L.
Kouwenhoven
,
S.
Kröll
,
G.
Leuchs
,
M.
Lewenstein
,
D.
Loss
,
N.
Lütkenhaus
,
S.
Massar
,
J. E.
Mooij
,
M. B.
Plenio
,
E.
Polzik
,
S.
Popescu
,
G.
Rempe
,
A.
Sergienko
,
D.
Suter
,
J.
Twamley
,
G.
Wendin
,
R.
Werner
,
A.
Winter
,
J.
Wrachtrup
, and
A.
Zeilinger
,
Eur. Phys. J. D
36
,
203
(
2005
).
3.
I.
Aharonovich
,
D.
Englund
, and
M.
Toth
,
Nat. Photonics
10
,
631
(
2016
).
4.
S.
Guha
,
H.
Krovi
,
C. A.
Fuchs
,
Z.
Dutton
,
J. A.
Slater
,
C.
Simon
, and
W.
Tittel
,
Phys. Rev. A
92
,
022357
(
2015
).
5.
A.
Khalique
and
B. C.
Sanders
,
J. Opt. Soc. Am. B
32
,
2382
(
2015
).
6.
E.
Waks
,
E.
Diamanti
, and
Y.
Yamamoto
,
New J. Phys.
8
,
4
(
2006
).
7.
D. B.
Higginbottom
,
L.
Slodička
,
G.
Araneda
,
L.
Lachman
,
R.
Filip
,
M.
Hennrich
, and
R.
Blatt
,
New J. Phys.
18
,
093038
(
2016
).
8.
Quantum Dots for Quantum Information Technologies
, edited by
P.
Michler
(
Springer
,
2017
).
9.
N.
Somaschi
,
V.
Giesz
,
L. D.
Santis
,
J. C.
Loredo
,
M. P.
Almeida
,
G.
Hornecker
,
S. L.
Portalupi
,
T.
Grange
,
C.
Antón
,
J.
Demory
,
C.
Gómez
,
I.
Sagnes
,
N. D.
Lanzillotti-Kimura
,
A.
Lemaítre
,
A.
Auffeves
,
A. G.
White
,
L.
Lanco
, and
P.
Senellart
,
Nat. Photonics
10
,
340
(
2016
).
10.
A. C.
Dada
,
T. S.
Santana
,
R. N. E.
Malein
,
A.
Koutroumanis
,
Y.
Ma
,
J. M.
Zajac
,
J. Y.
Lim
,
J. D.
Song
, and
B. D.
Gerardot
,
Optica
3
,
493
(
2016
).
11.
K. A.
Fischer
,
K.
Müller
,
K. G.
Lagoudakis
, and
J.
Vučković
,
New J. Phys.
18
,
113053
(
2016
).
12.
K. A.
Fischer
,
L.
Hanschke
,
J.
Wierzbowski
,
T.
Simmet
,
C.
Dory
,
J. J.
Finley
,
J.
Vučković
, and
K.
Müller
,
Nat. Phys.
13
,
649
(
2017
).
13.
T.
Miyazawa
,
K.
Takemoto
,
Y.
Nambu
,
S.
Miki
,
T.
Yamashita
,
H.
Terai
,
M.
Fujiwara
,
M.
Sasaki
,
Y.
Sakuma
,
M.
Takatsu
,
T.
Yamamoto
, and
Y.
Arakawa
,
Appl. Phys. Lett.
109
,
132106
(
2016
).
14.
H.
Jayakumar
,
A.
Predojević
,
T.
Huber
,
T.
Kauten
,
G. S.
Solomon
, and
G.
Weihs
,
Phys. Rev. Lett.
110
,
135505
(
2013
).
15.
M.
Müller
,
S.
Bounouar
,
K. D.
Jöns
,
M.
Glässl
, and
P.
Michler
,
Nat. Photonics
8
,
224
(
2014
).
16.
C.
Heyn
,
A.
Stemmann
,
T.
Köppen
,
C.
Strelow
,
T.
Kipp
,
M.
Grave
,
S.
Mendach
, and
W.
Hansen
,
Appl. Phys. Lett.
94
,
183113
(
2009
).
17.
Y. H.
Huo
,
B. J.
Witek
,
S.
Kumar
,
J. R.
Cardenas
,
J. X.
Zhang
,
N.
Akopian
,
R.
Singh
,
E.
Zallo
,
R.
Grifone
,
D.
Kriegner
,
R.
Trotta
,
F.
Ding
,
J.
Stangl
,
V.
Zwiller
,
G.
Bester
,
A.
Rastelli
, and
O. G.
Schmidt
,
Nat. Phys.
10
,
46
(
2014
).
18.
D.
Huber
,
M.
Reindl
,
Y.
Huo
,
H.
Huang
,
J. S.
Wildmann
,
O. G.
Schmidt
,
A.
Rastelli
, and
R.
Trotta
,
Nat. Commun.
8
,
15506
(
2017
).
19.
K.
Brunner
,
G.
Abstreiter
,
G.
Böhm
,
G.
Tränkle
, and
G.
Weimann
,
Phys. Rev. Lett.
73
,
1138
(
1994
).
20.
S.
Stufler
,
P.
Machnikowski
,
P.
Ester
,
M.
Bichler
,
V. M.
Axt
,
T.
Kuhn
, and
A.
Zrenner
,
Phys. Rev. B
73
,
125304
(
2006
).
21.
A. V.
Kuhlmann
,
J.
Houel
,
D.
Brunner
,
A.
Ludwig
,
D.
Reuter
,
A. D.
Wieck
, and
R. J.
Warburton
,
Rev. Sci. Instrum.
84
,
073905
(
2013
).
22.
M.
Reindl
,
K. D.
Jöns
,
D.
Huber
,
C.
Schimpf
,
Y.
Huo
,
V.
Zwiller
,
A.
Rastelli
, and
R.
Trotta
,
Nano Lett.
17
,
4090
(
2017
).
23.
R.
Filip
and
L.
Mišta
,
Phys. Rev. Lett.
106
,
200401
(
2011
).
24.
M.
Ježek
,
I.
Straka
,
M.
Mičuda
,
M.
Dušek
,
J.
Fiurášek
, and
R.
Filip
,
Phys. Rev. Lett.
107
,
213602
(
2011
).
25.
I.
Straka
,
A.
Predojević
,
T.
Huber
,
L.
Lachman
,
L.
Butschek
,
M.
Miková
,
M.
Mičuda
,
G. S.
Solomon
,
G.
Weihs
,
M.
Ježek
, and
R.
Filip
,
Phys. Rev. Lett.
113
,
223603
(
2014
).
26.
L.
Hanschke
,
K. A.
Fischer
,
S.
Appel
,
D.
Lukin
,
J.
Wierzbowski
,
S.
Sun
,
R.
Trivedi
,
J.
Vučković
,
J. J.
Finley
, and
K.
Müller
, preprint arXiv:1801.01672 [quant-ph] (
2018
).
27.
R.
Kolesov
,
K.
Xia
,
R.
Reuter
,
R.
Stöhr
,
A.
Zappe
,
J.
Meijer
,
P. R.
Hemmer
, and
J.
Wrachtrup
,
Nat. Commun.
3
,
1029
(
2012
).