## Introduction

Since the observation of double–slit interference by Young in 1807, optical interference phenomena have provided multiple demonstrations of the wave nature of light. After that pioneering experiment, many studies on interferences have been performed to reveal the deeper nature of light, for example, the wave–particle duality of photons1,2,3 and their high-order correlations4,5. To date, interference phenomena have been observed not only in the light intensity, but also in other degrees of freedom of light6, including the frequency7, polarisation8, and orbital angular momentum9, and have thus played an important role in various structured light generation applications10. Fringe patterns are a common feature of most interference phenomena and these fringes form the basis of interferometers, which have proven to be powerful practical tools in numerous fields, e.g., in gravitational-wave detection11, optical coherence tomography12, Fourier transform infrared spectroscopy13, and applications of fibre optic gyroscopes14.

For light intensity interference, the existence of constructive and destructive interference is dependent on a stable phase difference between two or more light beams. In traditional interferometers, the stable phase difference is determined by the optical path difference (OPD). For example, in equal–inclination interference15 (Fig. 1a), the OPD between the two reflecting surfaces changes with incident angle, and therefore, light with the same incident angle finally superposes to form a bright or dark fringe. Features of the interference fringe patterns are also dependent on the properties of the light source. Most past studies and applications of interference have used lasers or thermal light sources. In recent years, a new light source based on spontaneous parametric down-conversion (SPDC)16,17 in nonlinear crystals has been attracting much attention. The SPDC is a second-order nonlinear process, in which a higher-energy pump photon splits into a pair of lower-energy photons, one designated a signal photon and the other an idler photon, emerging with a certain probability from a nonlinear crystal. This special source of light has helped in finding many novel interference phenomena4,18,19,20 and applications21,22,23,24,25,26,27,28,29,30 that are quite different from those using lasers or thermal light sources31,32,33. If the entanglement properties are ignored, each arm (subsystem) of an SPDC source can usually be regarded as an incoherent mix of photons with all possible spatial modes and frequencies. Unlike lasers or thermal light sources, in which the spatial modes and frequency components can be treated independently, photons from an SPDC source have a structured frequency-angular spectrum (FAS) caused by the phase-matching conditions. The emission angles outside the nonlinear crystal are dependent on the emitted photon frequencies. For a long crystal, this dependence relation is approximately a one-to-one mapping that is governed by a tuning curve31, which can be approximated as a parabola.

In this work, we have observed a distinctive two-beam interference phenomenon in an amplitude division interferometer using photons from one arm of an SPDC source (Fig. 1b); we refer to it as angular-spectrum-dependent (ASD) interference because it is caused by a combination of interference patterns of different angular components. The principle and phenomenon of the ASD interference are very similar to those of the traditional equal-inclination interference: they both have ring-like fringes, the phase difference inducing bright or dark rings is dependent on the angle, and the number of rings is dependent on the distance d. However, ASD interference is fundamentally different from traditional equal-inclination interference. The creation and properties of ASD interference are closely related to the frequency-angular one-to-one mapping relation of the SPDC process. To illustrate the properties of ASD interference (Fig. 1b) and distinguish it from the traditional equal-inclination interference (Fig. 1a), we compare them in terms of the following five aspects. First, the two light sources have different radiation properties: the point source shown in Fig. 1a radiates spherical waves that are isotropic, but the SPDC process shown in Fig. 1b radiates photons over a very wide spectrum, where the photon frequencies are related to the emission angle θ(ω), which is shown using Eq. (1). Second, with regard to their principles of interference, the phase differences for the bright or dark fringes are caused by the angular-dependent OPDs Δ(θ) of the light in Fig. 1a, whereas the phase differences are caused by the specific photon frequencies ωn in Fig. 1b. Third, in Fig. 1a, the photons in each of the fringes are coherent and have the same spectrum and the interference visibility is thus dependent on the width of the spectrum; in Fig. 1b, however, the photons in the different fringes have different frequencies and the fringe visibility is dependent on the width of the FAS. Fourth, in the optical setups, the lens in Fig. 1a allows observation of the far-field of the fringes that are created, while the lens shown in Fig. 1b is used for collimation. Finally, the interference patterns of the two phenomena are both ring-like fringes, but with increasing distance d between the two reflecting surfaces, the fringes of the ASD interference vary much more quickly than those in the traditional interference pattern; in other words, much shorter distance d are required for the ASD interference to obtain the same interference patterns. In stressing this last point, we say that the equivalent wavelength of this ASD interference is much shorter than the actual wavelength. The physical meaning of the equivalent wavelength here is that the ASD interference fringes are the same as those from a traditional equal-inclination interferometer in which the wavelength of the photons has this value. In the following, the equivalent wavelength is defined so that the expression for the phase difference has the same form as that for the traditional interference.

The FAS of the SPDC has been reported previously31,34. Shih calculated the tuning curve required for type-I and type-II angle phase-matching31. Burlakov et al.34 calculated the intensity distribution of the FAS near the degenerate phase-matching condition and presented a photograph of this distribution; they implemented the second-order and fourth-order interference using photons from two nonlinear interaction regions, however, only single-frequency interference was observed in their experiment. Nevertheless, the ring-like fringes created by interference using photons with the structured FAS remain unexplored, along with the properties of these fringes, and these fringes thus form the main topic of our study. We also quantify the distribution of the fringes and their differences from the fringes obtained through traditional equal-inclination interference. In the following, we first introduce briefly the experimental setup (details are presented in Methods), describe the FAS of the SPDC obtained from our experiment and present the expression for the tuning curve used for nondegenerate type-0 quasi-phase-matching. Next, we explain how the interference fringes are generated and define the equivalent wavelength and parameter γ, which is the ratio of the real centre wavelength to the equivalent wavelength, to show the difference between ASD and equal-inclination interference. Finally, we discuss the potential applications of this ASD interference phenomenon.

## Results

In our experiment (Fig. 2), we use a periodically poled potassium titanyl phosphate (PPKTP) crystal as our SPDC source, which makes use of nondegenerate type-0 quasi-phase-matching35. The photons generated in SPDC and used for the interference are referred to as signal photons (with wavelengths of approximately 797 nm); the idler photons (~1540 nm) are discarded. The FAS of the signal photon (Fig. 2a) is described by a binary function that reflects the radiation properties of the SPDC process. Its shape is parabolic with a width having a sinc2 functional shape. The unique distribution of FAS is simulated based on the phase-matching condition (see Section 1 of Supplementary Information for details). The function values of the FAS reflect the relative probability of photon detection for a particular outside angle (emission angle outside the crystal) and a particular frequency. If the phase-matching condition is well satisfied, the value is relatively large. In other words, the smaller the phase mismatch is, the larger the value is, and vice versa.

We assume photons with a FAS of Fig. 2a enter a Michelson interferometer having an arm difference d. Because each frequency component has a distinct interference result expressed by factor[1 + cos(2s/c)]/2, the FAS after the interferometer becomes that shown in Fig. 2b (here, d = 100 μm as an example). If the photons then pass through a lens that is used as a Fourier translator, each of their angular components maps into a ring in the spatial domain. Therefore, a ring-like interference pattern is formed when the photons are observed. The setup of the Michelson interferometer in our experiment (Fig. 2) comprises two lenses (L1 and L2) that form a 4-f imaging system and two mirrors (M1 and M2) located at the focal points. Another lens (L3) is used as a Fourier translator, which maps the spatial frequency components to the spatial rings on the detection plane. The interference patterns, shown in Fig. 3a, are recorded by a photon-counting intensified charge-coupled device (ICCD) camera. The simulations of the interference patterns from calculating the phase mismatch are shown in Fig. 3b (the simulation is based on equations (S3) and (S6) in Section 2 of Supplementary Information, in which a small-angle approximation is used).

The interference pattern may also be established from analytical methods. Here, we ignore the width of the FAS (Fig. 2a), and we are only interested in parabola-like tuning curves that show how the outside angle of the signal photons changes as a function of frequency or wavelength. The tuning curve is approximately described by the expressions (detailed derivations may be found in Section 3 of Supplementary)

$$\theta _{{{{\mathrm{s - out}}}}}^2 = b_1\Delta \omega$$
(1)
$$b_1 = \frac{{2n_{i0}n_{{{{\mathrm{s}}}}0}\omega _{{{{\mathrm{i}}}}0}\left( {\beta _{{{\mathrm{s}}}}\omega _{{{{\mathrm{s}}}}0} + n_{{{{\mathrm{s}}}}0} - \beta _{{{\mathrm{i}}}}\omega _{{{{\mathrm{i}}}}0} - n_{{{{\mathrm{i}}}}0}} \right)}}{{\omega _{{{{\mathrm{s}}}}0}\left( {\omega _{{{{\mathrm{s}}}}0}n_{{{{\mathrm{s}}}}0} + \omega _{{{{\mathrm{i}}}}0}n_{{{{\mathrm{i}}}}0}} \right)}}$$
(2)

where $$\Delta \omega = \omega _{{{\mathrm{s}}}} - \omega _{{{{\mathrm{s}}}}0} = \omega _{{{{\mathrm{i}}}}0} - \omega _{{{\mathrm{i}}}}$$, and $$\beta _{{{\mathrm{s}}}} = \left( {\frac{{dn}}{{d\omega _{{{\mathrm{s}}}}}}} \right)_{\omega _{{{{\mathrm{s}}}}0}},\;\beta _{{{\mathrm{i}}}} = \left( {\frac{{dn}}{{d\omega _{{{\mathrm{i}}}}}}} \right)_{\omega _{{{{\mathrm{i}}}}0}}$$ are the coefficients of first-order dispersion at the centre frequency of the signal and idler photons. The subscript 0 indicates a corresponding value at the centre frequency of the wavelength; for example, ωs0,ωi0,ns0,ni0 are the centre frequency and the corresponding refractive index of the signal and idler photons. Equations (1) and (2) were obtained by applying approximate conditions in which Δω is small and the length of the crystal is long enough so that the width of the FAS may be ignored.

The relationship between radius ρ of the abovementioned ring and the outside angle of signal photons is approximately given by ρθs_outf3, for which f3 is the focal length of L3. By substituting Eq. (1) into the general interference factor [1 + cos(2s/c)]/2, the count recorded by the ICCD may be expressed as:

$$C\left( \rho \right) \propto 1 + \cos \left( {\frac{{2d\omega _{s0}}}{c} + \frac{{2d}}{{f_3^2b_1c}}\rho ^2} \right)$$
(3)

The interference patterns predicted by Eq. (3) are presented in Fig. 3c. The difference between Fig. 3b, c is that the simulations in Fig. 3c do not take the interference visibility into account because the width of the sinc2 function is ignored. In other words, the complete interference expression should have the form [1 + V(d)cos(2s/c)]/2, where the function V(d) represents the interference visibility and V(d) is assumed to have a constant value of 1 in Eq. (3). The interference visibility and the coherence length are described by Eq. (S22) and (S23) in Section 4 of Supplementary Information, respectively.

In the experiment, we fixed M2 on the displacement platform and M1 on the piezoelectric transducer (PZT). We varied the arm difference by moving M2, then finely adjusted the PZT to ensure the centres of the interference patterns are bright spots. Fig. 3a shows the experimental results with different arm differences. The numbers at the top indicate approximate arm differences, specifically, from the reading of the displacement platform. The numbers at the bottom of Fig. 3c show the actual arm differences set in the simulation. In comparison, the experimental results agree well with our theoretical calculation.

In Fig. 3a–c, more interference rings appear with increasing arm difference d. We next show the radial distribution of the rings as a function of the arm difference. Assuming the radius of the n-th ring is ρn, (n being the constructive interference order), then from Eq. (3) we obtain a quadratic relation

$$a\rho _n^2{{{\mathrm{ + }}}}\phi _0 = n$$
(4)

where $$a = d/\pi f_3^2b_1c$$ and ϕ0 = s0/πc. Equation (4) describes the distribution of fringes where the coefficient a determines the radius of the fringes for each order. For a specific order n, a greater value of a indicates a smaller value of the radius ρn and thus indicates a higher fringe density. In the experiments, a is obtained by fitting the experimental data (ρn,n). By comparing the coefficient ae = d/f2λ for the far-field equal-inclination interference36, ($$a_{{{\mathrm{e}}}} = d/f_3^2\lambda _{{{{\mathrm{s}}}}0}$$ for our experimental condition), we define an equivalent wavelength λeq = πb1c to cause the coefficient a to have the general form $$a = d/f_3^2\lambda _{{{{\mathrm{eq}}}}}$$. In the experiment, this equivalent wavelength is obtained by fitting the dependence of a to d. Fig. 3d shows the experimentally obtained pairs (ρn,n) for different values of d. The coefficient a may be evaluated using a second-order polynomial fit to the data. In Fig. 3e, the obtained values of a are plotted for different d. The red line shows the fitted result, from which one obtains the equivalent wavelength 29.38 nm, which agrees well with the predicted value of 29.86 nm. For comparison, we also show the ae-d relation (dashed line) of a traditional equal-inclination interference; the ratio of the slopes of the two lines is denoted γ = a/ae = λs0/λeq. Except for the centre wavelength, γ is also dependent on the key parameter b1, the value of which depends on properties of the crystal material. From a qualitative analysis using Eq. (2), the determining factor for b1 includes the refractive index and crystal dispersion, the degree of degeneracy, and the type of quasi-phase-matching. The value of γ can be larger if the experimental parameters are carefully selected.

## Discussion

In summary, we report and study an interference phenomenon known as ASD interference using photons from one arm of an SPDC source. In this type of interference, the fringes distribution in Eq. (4) is the same as that in equal-inclination interference, however, it varies more rapidly with the increasing interferometer arm difference than those obtained from traditional equal-inclination interference. We defined two parameters to quantitatively compare the difference between the ASD interference and the traditional equal-inclination interference: the equivalent wavelength λeq and the ratio γ. Under our experimental conditions, γ has an approximate value of 27; this means that the fringe density is improved by 27-fold for a specific arm difference d, in other words, the fringes of this interference vary 27 times more rapidly than the traditional equal-inclination interference with increasing arm difference. An advantage of the ASD interference is that the sensitivity can be increased γ-fold when we use this interferometer to measure small displacements or refractive index changes by recording variations of fringes, because in these cases, greater variation in the fringes indicates better sensitivity for OPD.

Another advantage of ASD interference with large value of γ is that the point at which the zero OPD occurs can be determined more accurately and thus the optical path measurement accuracy can be improved. As shown in Fig. 3a–c, the first completely dark fringe occurs when d = ±20 μm; this means that the position with the equivalent path can be determined with an error of ±20 μm; in the supplementary, we show that the error can be reduced to ±0.54 μm by fitting our experimental data. Furthermore, Eq. (3) indicates that the accuracy may be improved further by expanding the field of view ρmax or reducing either the focal length of L3 or the equivalent wavelength λeq. Because the SPDC source itself is a currently available nondegenerate two-photon source, the potential applications of ASD interference can also be generalised to the nonlinear interferometers based on SPDC34,37,38.

The ASD interference fringes not only have a ring-like structure in intensity but also have a structure in frequency of photons, where the photons in the different fringes have different frequencies. Considering the frequency structure, this interference phenomenon also holds promise in spectral-shaping a photon source based on SPDC. Because the rings in the interference patterns map different wavelength components, a cosine-modulated frequency spectrum is obtained if the interference patterns are collected into multimode fibres.

The interference phenomenon can be used in a reverse manner to measure the tuning curve of the SPDC process. By fitting the equivalent wavelength, the parameter b1 of the tuning curve can then be obtained. Overall, the novel phenomenon reported here not only enriches the existing knowledge with regard to interference and SPDC but also has promise for use in interferometry applications.

## Materials and methods

### Pump laser

The 525.2-nm light beam of the CW pump laser is generated in single-pass sum-frequency generation (SFG) with a 10-mm type-0 periodically poled potassium titanyl phosphate (PPKTP) crystal (the SFG source is omitted in Fig. 2). In the SFG source, the wavelengths of the two pump beams are 1540 nm and 797 nm, and all three beams are vertically polarised. The SFG laser beam is collected into a single-mode fibre and exits through a fibre collimator (the FC in Fig. 2). The idealised plane-wave pump in the SPDC leads to strict transverse momentum correlations. Therefore, the pump beam is collimated by a lens group (the lens group is omitted in Fig. 2); its width is of order 400 μm and the pump power is 50 mW. The waveplates (Fig. 2) are used to transform the pump beam from the collimator into a vertically polarised beam.

### Crystals

Two PPKTP crystals are used in the experiment, one for SFG and the other for SPDC. The two crystals have the same parameter values: their dimensions are 1 mm × 2 mm × 10 mm, and their grating periods are 9.34 μm. The temperature of the crystal used during SFG is set at 24 °C, which is an optimum temperature for SFG. The temperature of the crystal used for SPDC is set at 29 °C. This temperature is determined by performing difference-frequency generation between the 525.2-nm and 1540-nm laser beams. The two temperatures are different because the widths of the beams in the two crystals are different.

### Optical setup

Because the SPDC is the inverse of SFG, the central wavelength of the idler and signal photons are approximately 1540 nm and 797 nm. The signal and idler photons are split through a long-pass dichroic mirror (DM), where the idler photons pass through the DM (discarded) and the signal photons are reflected. The pump beam is filtered by a 750-nm long-pass filter that is omitted in Fig. 2. The experiment was performed in a dark environment, and the light path in front of the camera was carefully shaded by a sealed box to block external light.

### Data acquisition

The interference patterns (Fig. 3a) were recorded by our ICCD camera (Andor iStar DH334T) with a 10 s exposure time. The working temperature of the ICCD is cooled at −25 °C. The background is taken before the data acquisition and is subtracted by the ICCD camera automatically when signals are taken. The average counts of each pixel of the background are around 9000. The normalised grey values of the images in Fig. 3a from 0 to 1 represent the counts from 0 to 10000.