The inefficient single photon detection of Al-SNSPDs for infrared photons can be attributed to the relatively large diffusion coefficient (
De) of normal state electrons in Al films. Generally, 2D Al films exhibit a
De (∼5 cm
2/s) that is one order of magnitude higher than that of disordered NbN films or amorphous WSi films (∼0.5 cm
2/s) [
36], [
37], [
38]. Consequently, the quasiparticles or hot electrons within the hotspot are not sufficiently heated, resulting in a relatively low “temperature” within the hotspot. In Al SNSPDs, since the devices are prone to latch into a resistive state, we may then estimate that the hotspot relaxation time is comparable with the kinetic induce limited recovery time, ∼ 33.2 ns. If we even estimate the hotspot relaxation as 1 ns, with a
De of ∼ 5 cm
2/s, the hotspot size can then be estimated to be around
$ 2 \sqrt{D_{e} \tau_{\text {hotspot }}} \approx 1400$. As a result, the dissipated photon energy within the hotspot may be significantly suppressed, leading to a relatively “cold” hotspot. This may partially explain the relatively small hotspot resistance observed in our Al nanostrips. As a result, the hotspot is unable to effectively expel the bias current into the readout, thus limiting the IDE of the devices. Apart from the large
De, another contributing factor that further diminishes the IDE of Al-SNSPDs is the relatively long coherence length (
$\xi$). Due to its ultra-low upper critical field, the
$\xi$ of bulk clean Al can reach up to 1.5 μm [
39]. Even for our disordered Al films, the
$\xi$ can still be more than 60 nm [
40], which is significantly larger than the
$\xi$ of other commonly used thin films in SNSPD fabrication. Finally, it is also interesting to note that as a type-I superconductor, the quantized vortices is absent in Al-SNSPD. As a result, the vortex-assisted photon detection event (either by single vortex crossing or breakup of vortex-antivortex pairs) is therefore not present in Al nanowires, which in turn further hampers the superconducting to normal transition within the Al nanowire cross section. Consequently, to completely collapse superconductivity of Al-nanostrips, it would necessitate more telecom wavelength photons to generate a detection event. Specifically, on one hand, due to the relatively long coherence length in Al-nanostrips, cooper pairs may tunnel through the small hotspot. On the other hand, due to the relatively “cold” hotspot, it would need more photon energy to “over heat” the hotspot to completely transit the nanowire from superconducting to normal state.
Fig. 4 (b) and
(c) illustrate the photon count rates under different incident laser power at wavelengths of 785 nm and 1550 nm, respectively, for varying bias currents. By fitting the photon count rate dependency in a log–log scale, the slopes indicate that the probability of detecting a 785-nm photon increases linearly with the mean number of photons (
Fig. 4 (b)), demonstrating the operation of the detector in the single-photon region [
38]. Additionally,
Fig. 4 (c) indicates that two or three 1550-nm photons are required to trigger a detection event when
$I_{b}<0.8 I_{S W}$. Even in the higher bias range (
$I_{b}>0.8 I_{S W}$), the fitted slope remains greater than 1, suggesting the occurrence of multi-photon detection events. Typically, such cases of multi-photon detection significantly increase the timing jitter of the device, as indicated by a measured value of 644 ps for 1550-nm photons, obtained from the full width at half maximum of the time correlated photon count histogram.