Figure 1
Frequency down-conversion of nonclassical light emitted by a single QD. (a) Experimental setup. The confocal microscope consists of a liquid helium (LHe) continuous flow cryostat containing the QD sample at a temperature of 12 K. A bias-voltage of 3.20–3.47 V is applied to the QDs which are additionally optically excited using an average power of 160 nW at 590 nm from a pulsed fs optical parametric oscillator (OPO) with 80 MHz repetition rate [
35]. Optical excitation and collection of photoluminescence (PL) emitted by a QD are performed using a
microscope objective with numerical aperture
. We collect up to
into a single-mode fiber (SMF600). A silica etalon can be inserted optionally for narrow-band filtering of the PL. Two long-pass filters prevent residual excitation light from entering the fiber. For frequency down-conversion, the visible photons are coupled into the Zn:PPLN ridge waveguide together with a strong pump beam at 1550 nm provided by a continuous-wave OPO (see the Supplemental Material [
27]). The converted photons are spatially separated from the strong pump light and from residual visible photons by a prism and a pinhole and are coupled into a standard telecom fiber (SMF28). To suppress residual pump light and noise background around the target wavelength
, we additionally use a spectral filtering setup composed of a fiber-optic circulator, a fiber Bragg grating (FBG) centered at 1312.714 nm (
reflection bandwidth: 0.755 nm) and two
wavelength division multiplexers (WDM1 and WDM2). SMF: single mode fiber, PC: polarization control, HWP: half-wave plate, PBS: polarizing beam splitter, BC: beam combiner, AL: aspheric lens. (b) Total efficiency and SNR of the frequency conversion setup calculated from measured data using single photon input from a QD. (c) Spectral acceptance bandwidth of the DFG process measured for 2 mW input power around 710.74 nm from a tunable cw Ti:sapphire laser. For further details, see the Supplemental Material [
27].
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