Photonics Research, Volume. 13, Issue 8, 2291(2025)

Optical footprint of ghost and leaky hyperbolic polaritons

Mark Cunningham1、*, Adam L. Lafferty1, Mario González-Jiménez2, and Rair Macêdo1
Author Affiliations
  • 1James Watt School of Engineering, Electronics & Nanoscale Engineering Division, University of Glasgow, Glasgow G12 8QQ, UK
  • 2School of Chemistry, University of Glasgow, Glasgow G12 8QQ, UK
  • show less

    Manipulating hyperbolic polaritons at infrared frequencies has recently garnered interest as it promises to deliver new functionality for next-generation optical and photonic devices. This study investigates the impact of the crystal’s anisotropy orientation on the attenuated total reflection (ATR) spectra, more specifically, revealing the optical footprint of elliptical, ghost (GHP), and leaky (LHP) hyperbolic polaritons. Our findings reveal that the ATR spectra of GHPs exhibit a distinct hyperbolic behavior that is similar to that recently observed using s-SNOM techniques. Similarly, the ATR spectra of LHPs show its clear lenticular behavior; however, here we are able to discern the effects of large asymmetry due to cross polarization conversion when the crystal anisotropy is tilted away from the surface. Furthermore, we demonstrate that by controlling the anisotropy orientation of hyperbolic media it is possible to significantly alter the optical response of these polaritons. Thus, our results provide a foundation for the design of direction-dependent optical devices.

    1. INTRODUCTION

    Hyperbolic materials have attracted significant interest for controlling light at the nanoscale [13], due to their intrinsic hyperbolic dispersion and strong electromagnetic field confinement [4]. They have been shown to support surface polaritons [513], with long-range and low-loss propagation of subwavelength information [8,11], guided waves [1417], and negative refraction [4,5,1820]. In these materials, hyperbolic dispersion results from the principal elements of the permeability or permittivity tensor possessing opposite signs [4,5,8,11,16,2124]. This is typically a consequence of anisotropy due to elementary resonances in matter and can emerge across a vast range of frequencies depending on the mechanism (e.g., phonon resonances in the infrared [15,2527] or magnetic resonances [2832] in the GHz and THz frequency range). The role of anisotropy orientation with respect to the interface has recently received attention for creating direction-dependent optical devices [5,22,3344] and has, more recently, led to the discovery of peculiar entities, namely ghost hyperbolic polaritons (GHPs) [8] and leaky hyperbolic polaritons (LHPs) [11].

    GHPs come from the phenomenon of a “ghost wave” first theorized by Naraminov as an extension of the Dyakonov surface polariton [45]. Dyakonov surface polaritons are polaritons that propagate along the interface of transparent anisotropic media with its anisotropy axis aligned with the surface, or at the interface between two identical anisotropic crystals with different orientations [4548]; they are highly directional, and confined to very narrow angular orientations of the anisotropy axis [49]. These ghost waves combine the properties of propagating and evanescent fields within anisotropic media. Coupling to these ghost waves in a hyperbolic material (i.e., the GHP) was first proposed in a metamaterial [50] with a tilted anisotropy axis and experimentally observed in tilted calcite [8], a natural hyperbolic material. GHPs have been characterized as virtual surface phonon-polariton modes [51,52], devoid of an electrostatic limit (with damped propagation even in the absence of material loss [53]) with characteristic high-resolution, ray-like propagation at the material surface over distances up to 20 μm [8]. These are a consequence of the anisotropy axis being neither parallel nor perpendicular to the sample surface; this, in turn, gives rise to phase wavefronts slanted away from the surface of the crystal, Poynting vectors parallel to the surface, and exponential decay away from the surface. Since their emergence, spatiotemporal ultrafast dynamics of GHP nanolight pulse propagation has also been studied [2] as well as planar junctions and anisotropic metasurfaces that can support “ghost line waves” that propagate unattenuated along the line interface, with phase oscillations combined with evanescent decay away from the interface [54]. In the visible light range, ghost modes have been observed in the bulk plasmonic material MoOCL2 [53]. Remarkably though, they do not require an interface or a tilted anisotropy axis away from the surface.

    LHPs, on the other hand, are hybridizations of propagating ordinary bulk modes and extraordinary surface waves [11]. They originate from the physics of leaky waves, studied since the 1940s, which are guided modes that propagate along open wave-guiding structures [55,56]. Unlike conventional surface waves, leaky waves possess complex propagation constants, allowing energy radiation into free space as they travel [5759]. Leaky wave antennas have utilized plasmonic metamaterials with epsilon-near-zero (ENZ) dielectric constants to enhance directionality [60]. Anisotropic ENZ materials with tunable transverse dielectric responses and low magnetic permeability materials with strong tangential magnetic fields have also been employed to control emission and directivity [61]. Hyperbolic materials are ideal candidates for supporting leaky waves, particularly around longitudinal optic phonon frequencies where dielectric tensor components are small [4]. These materials offer advantages over plasma layers, which only support leaky waves above their plasma frequency. Additionally, LHPs have been shown to exhibit tilted wavefronts into the bulk and Poynting vectors canted away from the interface [11].

    These novel polariton modes have been, very recently, studied in-depth using s-SNOM and further supported by spectroscopy. Here, we demonstrate how GHPs and LHPs manifest through attenuated total reflection (ATR) spectroscopy in bulk hyperbolic crystals, specifically investigating their direction-dependent optical footprint across the crystal’s surface. By investigating how these polaritons appear in the far-field using more widely available infrared spectroscopy, we use ATR to investigate the conditions under which LHPs and GHPs may be supported in bulk hyperbolic media, using crystal quartz as the example material. This should provide valuable insight for integrating these materials into, as well as exploiting these properties for, novel optical devices.

    We employ ATR in the Otto configuration [37,62,63], as shown in Fig. 1(a), where reflection occurs at the boundary between a prism and the crystal supporting surface polaritons. In turn, the prism with a high dielectric constant, εp, generates a high in-plane momentum with wavevector kx=k0εpsinθ, where k0=ω/c and θ is the incident angle of the infrared waves with angular frequency ω that couple to polariton modes. Note that if an air gap d is included between the prism and the crystal and radiation is incident at an angle higher than the critical angle of the prism/air interface, total internal reflection occurs and only evanescent modes travel across the air gap.

    (a) Experimental setup geometry, where a polarizer is used to generate a TM-polarized beam, which is incident at the surface of crystal quartz at an incident angle of θ=45° from a dielectric prism (εp=5.5). (b) Real part of the principal components of the dielectric function of quartz in the frequency range 410–610 cm−1. (c) Theoretical (dashed line) and experimental (solid line) reflectance spectra [using the setup shown in (a)] for a crystal quartz sample whose anisotropy lies along the z axis and an air gap of d=2.0 μm.

    Figure 1.(a) Experimental setup geometry, where a polarizer is used to generate a TM-polarized beam, which is incident at the surface of crystal quartz at an incident angle of θ=45° from a dielectric prism (εp=5.5). (b) Real part of the principal components of the dielectric function of quartz in the frequency range 410610  cm1. (c) Theoretical (dashed line) and experimental (solid line) reflectance spectra [using the setup shown in (a)] for a crystal quartz sample whose anisotropy lies along the z axis and an air gap of d=2.0  μm.

    The natural hyperbolic material used here, crystal quartz, supports hyperbolic polaritons due to infrared-active phonon resonances. This makes the crystal anisotropic with a diagonal dielectric tensor. For instance, in the frequency range between 410 and 610  cm1, corresponding to free-space wavelengths between 16 and 25 μm, there are two regions where the principal components of the dielectric tensor possess opposite signs, as shown in Fig. 1(b). All parameters used for calculating the dielectric tensor components were taken from Ref. [25] as detailed in Section 5. Therefore, hyperbolic behavior is observed: a Type I region, i.e., the extraordinary component ε of the dielectric tensor is negative while the ordinary component ε is positive, between 510 and 550  cm1, and a Type II region, ε>0 and ε<0, between 450 and 480  cm1.

    To build context, let us look at the case where ε is perpendicular to the surface of the crystal (along z) and the crystal axes are aligned with the laboratory axes. SPhPs typically propagate along the crystal’s surface with an exponential decay of amplitude away from the surface. In the case shown in Fig. 1(a), SPhPs couple with TM-polarized infrared radiation. Assuming propagation along x and decay along z, given by the parameters α0 (air) and α (hyperbolic material), plane wave solutions take the following form in air: H(x,z,t)=y^Hei(kxxωt)eα0z,and in the hyperbolic material: H(x,z,t)=y^Hei(kxxωt)eαz.Using Maxwell’s equations, similarly to Ref. [28], and matching its solutions inside and outside the hyperbolic material, the boundary conditions allow us to find the following dispersion relation for the surface polaritons: 0=α0+αεxx.Since α0 and α are positive (to ensure decay away from the surface) and the anisotropy axis is oriented along z such that εxx=ε, Eq. (3) can only be satisfied when ε<0. The corresponding ATR response is shown in Fig. 1(c) where a distinct minimum in the reflection is observed between hyperbolic regions, corresponding to where the condition set out above is met. In this case, evanescent waves in air, generated by the total internal reflection in the prism, couple to SPhPs in the hyperbolic material. Here, we used a coupling prism with dielectric constant εp=5.5 and an air gap of d=1.5  μm at a fixed incident angle of θ=45°, corresponding to an in-plane momentum of kx/k0=1.66 to induce total internal reflection.

    While the behavior of SPhPs detailed above is well known, it can be drastically modified by controlling the orientation of the anisotropy. One way to achieve this is by tilting the anisotropy axis by an angle φ away from the z axis, as shown in Fig. 2(a), so that ε is neither perpendicular nor parallel to the interface. When discussing this angle, a few special configurations are worth noting, namely, φ=0° and φ=90°, which correspond to ε aligning perpendicular and parallel to the surface, respectively. Altering φ will effectively rotate the hyperbolic dispersion [5], introducing off-diagonal components to the dielectric tensor [5,34]. Another way to modify the behavior of SPhPs is by introducing an azimuthal rotation around the z axis by an angle β with respect to the incidence plane (here taken as xz) as shown in Fig. 2(b), which mimics the effect of an in-plane wavevector ky. Therefore, a special case includes φ=90° and β=90° making ε and ε aligned along the x and y axes, respectively. Another special case is when φ=0°. In this case, the components on the dielectric tensor aligned with x and y are both equal to ε, as shown in Fig. 2(b). Therefore, there is no azimuthal dependence of the spectrum shown in Fig. 1(c).

    (a) Geometry of the dielectric components with respect to the laboratory axis when introducing the angle φ. (b) Geometry of the dielectric components with respect to the laboratory axis when introducing the angle β.

    Figure 2.(a) Geometry of the dielectric components with respect to the laboratory axis when introducing the angle φ. (b) Geometry of the dielectric components with respect to the laboratory axis when introducing the angle β.

    On the other hand, an azimuthal rotation will introduce significant change to this spectrum if φ0 as shown in Fig. 3 where both theoretical and experimental results for φ=45° [Fig. 3(a)] and φ=90° [Fig. 3(b)] are given. Clear agreement is shown between theory and experiment and, in both cases, we can see a sharp dip in reflectivity between the two hyperbolic regions, corresponding to the existence of a surface polariton. When φ=45° as shown in Fig. 3(a), the surface wave displays a sinusoidal azimuthal dependence. The excitation frequency reaches its maximum value of ω/2πc=500  cm1 at azimuthal angles β=0° and 180°, while the minimum value of ω/2πc=480  cm1 occurs at β=90° and 270°. We note that the surface wave exists entirely within a region where bulk propagation is not allowed, shown by the rectangular shape of high reflectivity around the surface wave.

    The dependence of ATR in crystal quartz on the azimuthal angle β. (a) φ=45°, (b) φ=90°, with kxk0=1.66. εp=5.5 and d=2 μm. (c) ATR of quartz at ω/2πc=490 cm−1 when φ=90°, with the radius corresponding to kx where εp=5.5, and the azimuthal angle corresponding to the angle β, with d=2 μm.

    Figure 3.The dependence of ATR in crystal quartz on the azimuthal angle β. (a) φ=45°, (b) φ=90°, with kxk0=1.66. εp=5.5 and d=2  μm. (c) ATR of quartz at ω/2πc=490  cm1 when φ=90°, with the radius corresponding to kx where εp=5.5, and the azimuthal angle corresponding to the angle β, with d=2  μm.

    When we rotate the anisotropy further (φ=90°), as shown in Fig. 3(b), the dependence on azimuthal orientation now takes a rectified sinusoidal shape. This frequency reaches its maximum value of ω/2πc=505  cm1 at azimuthal angles β=0° and 180°, while the minimum value of 475  cm1 occurs at β=90° and 270°.

    So far, we have focused on the azimuthal dependence of the ATR spectra at a fixed kx/k0 value for a range of frequencies; we will now turn to the case of a fixed frequency between the two hyperbolic regions where the surface polariton exists. This is shown in Fig. 3(c), in which the behavior of varying kx/k0 is given for φ=90° and at 490  cm1. We can see that the surface polariton displays an elliptical profile with respect to the azimuthal angle β, which is to be expected where all dielectric tensor components are negative [23,64]. We can see that a smaller kx/k0 is needed when β=0°, and a larger value is needed towards β=90°. This is because ε has a much larger negative value than ε, so less in-plane momentum is required to couple with the surface polariton when the anisotropy is aligned with the x axis.

    Now that we have shown how the orientation of the anisotropy axis can greatly impact the existence of surface polaritons in crystal quartz, we can redirect our analysis towards the reflective traits of GHPs and LHPs.

    2. GHOST POLARITONS

    We have seen how surface waves behave in anisotropic materials, namely, their elliptical behavior with respect to β (or in-plane wavevector). Now, let us change the frequency region of interest; instead of looking at regions where no propagation is allowed, and thus surface waves can emerge, we turn to hyperbolic regions where propagation is allowed, beginning with the Type II hyperbolic region. In Type II hyperbolic regions we again focus on two main scenarios: (i) the anisotropy perpendicular to the crystal surface (here along z), and (ii) the case when the anisotropy aligns with the crystal’s surface, i.e., a geometry that allows for hyperbolic Dyakonov polaritons [49]. The first case would be similar to the classic surface polariton, which we have discussed in detail, as both components of the dielectric tensor along the surface are negative and despite εzz being positive, the condition in Eq. (3) could still be met for any β. The second case, on the other hand, is far more complex. For instance, when φ=90° and β=0° (ε lies along x and ε is along y), Eq. (3) can thus only be satisfied if β=90°, resulting in ε aligning with y and ε along x. In this orientation, and considering the incidence plane to be the xz plane, crystal quartz behaves entirely like a metal (εxx=εzz=ε).

    To illustrate this we calculate the ATR behavior at ω/2πc=460  cm1, shown in Fig. 4. First we look at the case where φ=90° but no air gap (d=0  μm). This is shown in Fig. 4(a), where we can see the clear bulk hyperbolic dispersion traced by propagating radiation (i.e., continuous dips in reflectance). Propagation is mostly supported when β=0° or 180°, reducing in intensity for higher kx values. On the other hand, propagation is completely forbidden when β=90° due to the quartz behaving entirely like a metal. In Fig. 4(b), we show the ATR when an air gap of d=0.1  μm is present so that evanescent waves can couple to surface waves. We observe a hyperbola-shaped drop in reflectivity, indicative of Dyakonov surface waves, in the region where bulk propagation is forbidden (i.e., upper region of the plot). As expected, it requires smaller kx values where β=90°, requiring more in-plane momentum when azimuthal rotation is introduced, until the surface wave is no longer supported at β=45° and β=135° where the bulk hyperbolic band exists. This highly angular dispersion mirrors that found in the original s-SNOM results of the original GHP discovery [8].

    ATR spectra for crystal quartz at ω/2πc=460 cm−1, with the radius corresponding to kx where εp=50, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) there is no air gap (d=0 μm) and φ=90°. In (b) the anisotropy orientation is unchanged (φ=90°) and an air gap is introduced to study the GHP, with d=0.1 μm. In (c), the air gap is removed (d=0 μm) and the anisotropy is rotated to φ=60° to alter the hyperbolic dispersion. In (d), the anisotropy orientation is unchanged (φ=60°) and an air gap is introduced again to study the GHP, with d=0.1 μm.

    Figure 4.ATR spectra for crystal quartz at ω/2πc=460  cm1, with the radius corresponding to kx where εp=50, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) there is no air gap (d=0  μm) and φ=90°. In (b) the anisotropy orientation is unchanged (φ=90°) and an air gap is introduced to study the GHP, with d=0.1  μm. In (c), the air gap is removed (d=0  μm) and the anisotropy is rotated to φ=60° to alter the hyperbolic dispersion. In (d), the anisotropy orientation is unchanged (φ=60°) and an air gap is introduced again to study the GHP, with d=0.1  μm.

    Earlier, we have also seen how combining a tilted anisotropy axis (with respect to the surface) with in-plane wavevectors can yield an extra degree of control of the surface polariton behavior. Since tilting the anisotropy in such a way has been used as a route to introducing GHPs [8], we now look at the effect of tilting the anisotropy away from the surface with φ=60°, shown in Figs. 4(c) and 4(d), again at ω/2πc=460  cm1. For the first case, in Fig. 4(c) we again look at no air gap (d=0  μm). The propagating behavior tracing the hyperbolic dispersion is very similar to Fig. 4(a), except that the reflectivity dip occurs at a slightly larger range of azimuthal angles. Introducing an air gap of d=0.1  μm, shown in Fig. 4(d), clearly displays the impact of rotating the anisotropy in the form of a GHP. Qualitatively, the shape of the ATR spectra is very similar to the untilted case. However, the surface wave component is now supported by a narrower range of azimuthal angles, centered at β=90°. The drop in reflectivity is less intense, showing the GHP moving away from the bulk hyperbolic dispersion. Moreover, tilting the anisotropy away from the surface means that the positive extraordinary dielectric tensor component will now provide propagation characteristics to the polariton (instead of a “true” surface polariton). This has been previously explained as tilted wavefronts into the bulk of the material and as long-distance propagation along the surface [8]. This anisotropy tilting introduces more pronounced optical effects associated with large anisotropy such as asymmetric cross polarization conversion [34], where details are shown in Appendix D.

    In order to obtain the results above we needed to modify a few parameters, namely, increase the prism dielectric constant compared to the experimental case shown in earlier sections. This is necessary to be able to generate high enough in-plane momentum to probe a large portion of the hyperbolic dispersion. As a consequence of the larger in-plane momentum, we also needed to reduce the air gap thickness to support critical coupling (see Appendix E for details on the effect of varying d). While we illustrate this behavior at a single frequency, in order to address behavior observed in s-SNOM, the frequency-dependent behavior is also vastly different to what we previously showed for true surface polaritons. For more information on the ATR response at specific frequencies, see Appendix F. In Fig. 5 we show the ATR spectra over the frequency range 430500  cm1 at a fixed kx/k0=5. For φ=90°, in Fig. 5(a), the elliptical surface polariton examined previously splits into segments at 490  cm1, positioned above the bulk propagation linked with Type II hyperbolic dispersion. A distinct hyperbolic Dyakonov surface polariton emerges between 450 and 470  cm1, peaking around β=90°, 270°, where ε aligns on both x and z axes. The polariton’s frequency-β relationship resembles an upward arrow, segregating bulk-propagation zones in the Type II hyperbolic region. At φ=60°, shown in Fig. 5(b), the GHP’s intensity reduces. The elliptical surface wave, rather than being separated, now connects via a slight reflectivity dip at 485  cm1 near β=90°, 270°, also increasing the range of β angles for which there is propagation within the Type II region. Increasing the range of angles for which there is propagation inside the Type II regions seems to also alter the GHP, decreasing its reflectance intensity, consistent with true surface waves being more pronounced where bulk propagation is absent [5].

    The dependence of ATR in quartz on the azimuthal angle β, with kxk0=5 and εp=50. An air gap is included (d=0.1 μm) to probe the GHP. In (a), the anisotropy is aligned with the interface (φ=90°). In (b), the anisotropy is rotated below the interface where φ=60°.

    Figure 5.The dependence of ATR in quartz on the azimuthal angle β, with kxk0=5 and εp=50. An air gap is included (d=0.1  μm) to probe the GHP. In (a), the anisotropy is aligned with the interface (φ=90°). In (b), the anisotropy is rotated below the interface where φ=60°.

    3. LEAKY POLARITONS

    Similar to GHPs, leaky polaritons have recently been studied using s-SNOM where the direction of the anistropy with respect to the crystal surface has been shown to play a crucial role [11]. To understand how LHPs manifest in ATR spectra, we now shift our focus to Type I hyperbolic regions where these waves have been shown to emerge in calcite [11]. To allow radiation leakage in an ATR setup, an air gap must be introduced to include the coupling of evanescent waves with the leaky wave. Leaky waves experience an exponential increase in air [58], which in the past has led them to be known as “mathematically improper” [65], meaning that quite a large air gap (as used here) will be necessary to allow coupling. As leaky waves appear at low wavevectors, we only observe surface wave-like to be supported slightly beyond the critical angle, close to kx/k0=1. Figure 6 shows the ATR behavior of leaky polaritons at 545  cm1 in crystal quartz.

    ATR spectra for crystal quartz at ω/2πc=545 cm−1, with the radius corresponding to kx where εp=2.2, and the azimuthal angle corresponding to the angle β. In (a) there is no air gap (d=0 μm) and φ=90°. In (b) the anisotropy orientation is unchanged (φ=90°) and an air gap is introduced to study the LHP, with d=10 μm. In (c), the air gap is removed (d=0 μm) and the anisotropy is rotated to φ=70° to alter the hyperbolic dispersion. In (d), the anisotropy orientation is unchanged (φ=70°) and an air gap is introduced again to study the LHP, with d=10 μm. The white, solid lines denote the light line (i.e., kx/k0=ky/k0=1.0).

    Figure 6.ATR spectra for crystal quartz at ω/2πc=545  cm1, with the radius corresponding to kx where εp=2.2, and the azimuthal angle corresponding to the angle β. In (a) there is no air gap (d=0  μm) and φ=90°. In (b) the anisotropy orientation is unchanged (φ=90°) and an air gap is introduced to study the LHP, with d=10  μm. In (c), the air gap is removed (d=0  μm) and the anisotropy is rotated to φ=70° to alter the hyperbolic dispersion. In (d), the anisotropy orientation is unchanged (φ=70°) and an air gap is introduced again to study the LHP, with d=10  μm. The white, solid lines denote the light line (i.e., kx/k0=ky/k0=1.0).

    In Fig. 6(a), where φ=90° and d=0  μm, we can see that the ATR spectra trace the hyperbolic dispersion (left- and right-hand side) due to the in-plane anisotropy, with two extraordinary cones on either side of the bulk ordinary cone. Outside of the ordinary cone, propagation is mostly supported when β=0° or 180°, reducing in intensity for higher kx values. In Fig. 6(b), we introduce an air gap d=10  μm, which induces the emergence of leaky polaritons. We observe a lenticular-shaped drop in reflectivity, indicative of the leaky polariton [11]. What is interesting is that this drop in reflectivity is only at a small kx interval larger than the critical angle, but it is within the bulk ordinary circle bounds of Fig. 6(a). The leaky polariton is supported mostly when β=0°, where metallic contribution from the negative dielectric tensor component is at its maximum. At β=90°, only non-metallic (positive) dielectric tensor components contribute; therefore no surface-like wave phenomena are supported.

    The effect of tilting the anisotropy away from the surface (φ=70°) is shown in Figs. 6(c) and 6(d) for both no air gap and d=10  μm. When probing bulk waves (no air gap) we can see that rotating the anisotropy causes the extraordinary cones to move inward, overlapping with the bulk ordinary cone, facilitating radiation leakage [11]. Notable asymmetry is observed due to cross polarization conversion, which has been studied previously, albeit not using ATR [34]. On the other hand, introducing an air gap causes the lenticular shape of the leaky polariton to move inwards too. The reflectivity drop is still shown slightly beyond the critical angle, so that evanescent coupling is still occurring, but within the bulk ordinary cone. We also note the stark asymmetry within the critical angle due to much larger cross polarization conversion than what was observed with no air gap (see Appendix G for details on cross polarization conversion due to LHPs).

    In Fig. 7(a), we see the azimuthal dependence of leaky polaritons in crystal quartz when the anisotropy is aligned with the surface, and an incident angle of θ=26.6° (corresponding to kx/k0=1.05 for a prism of εp=5.5). The reflectivity dip takes a downward-arrow shape, centered at azimuthal angles of β=0° and 180°, which correspond to the anisotropy aligning with the x axis and separating into two branches that widen as the frequency increases. This behavior is directly linked to the isofrequency contours of dispersion with lenticular shape observed in near-field imaging of LHPs in calcite [11]; namely, at the bottom of the downward-arrow shape, the lenticular shape is connected at β=0° and thus waves at the surface propagate along x (and all) directions, whereas at higher frequencies, the splitting into two branches indicates that waves at the surface of the crystal will only propagate in some directions. Notably, this is consistent with our understanding that larger negative extraordinary permittivity components reduce the directionality associated with ENZ ordinary components (see details of this in Appendix H, in the form of polar plots showing how the LHPs’ lenticular shape changes with frequency).

    The dependence of ATR in quartz on the azimuthal angle β, with kx/k0=1.05 and εp=5.5. An air gap is included (d=10 μm) to probe the LHP. In (a), the anisotropy is aligned with the interface (φ=90°). In (b), the anisotropy is rotated below the interface such that φ=70°.

    Figure 7.The dependence of ATR in quartz on the azimuthal angle β, with kx/k0=1.05 and εp=5.5. An air gap is included (d=10  μm) to probe the LHP. In (a), the anisotropy is aligned with the interface (φ=90°). In (b), the anisotropy is rotated below the interface such that φ=70°.

    When we tilt the anisotropy into the bulk at an angle φ=70° in Fig. 7(b), The intensity of the leaky polariton decreases slightly, and its minimum supporting frequency shifts above 540  cm1. This shift is accompanied by an increase in bulk hyperbolic dispersion below 540  cm1, illustrating the sensitive dependence of leaky polaritons on the orientation of the crystal’s anisotropy.

    4. DISCUSSION

    Our investigation of elliptical surface polaritons, GHPs, and LHPs in hyperbolic media using ATR spectroscopy reveals several key insights into their optical behavior. We have demonstrated that anisotropy orientation significantly influences the optical properties of hyperbolic polaritons, namely, their ATR spectra.

    As such, crystallographic orientation could be of significant importance in designing nanophotonic devices utilizing these phenomena, and it offers a new degree of freedom for manipulating light at the nanoscale.

    The ATR spectra of GHPs clearly trace the hyperbolic dispersion, outside of the bulk bands, when the anisotropy aligns with the surface, but reflectance reduces in intensity when the anisotropy is tilted with respect to the surface, due to an increase in cross polarization conversion. This strong direction-dependent behavior could be used in the directional control of electromagnetic waves. Moreover, GHPs respond to very high in-plane momenta, which could be utilized in receiving signals from a wide field of view. On the other hand, we find that LHPs are limited to a smaller range of kx values. However, the large asymmetry due to cross polarization conversion when the anisotropy is oriented away from the surface could be used in novel devices, such as potentially enabling one way communications. In this work, we investigate the LHP in the Type I region, and the GHP in Type II dispersion to more deeply understand the original experimental observation. However, ghost modes were observed in the visible range in the material MoOCL2 [53], which featured Type I hyperbolic dispersion. We note that, when investigating Type I hyperbolic dispersion, we could not obtain a reflective footprint similar to the GHP behavior observed in Type II regions in quartz and calcite. Therefore, more work is needed to understand how individual dielectric tensor elements, including off-diagonals, real components, and imaginary components, affect ghost-like features manifesting in the material.

    Finally, similar methods to what we explored here could be directly translated to investigating other unusual hyperbolic behavior such as the newly studied hyperbolic shear polariton in materials with larger asymmetry in their crystal structure [3,21,23,66,67]. In addition, this could also be a way to investigate the impact of twisted-layer structures [42,6773] on these phenomena, particularly as this could be a way to introduce further control over optical behavior.

    5. METHODS

    To calculate the reflectivity coefficients, the 4×4 transfer matrix method was used [36,37,7478] with full details given in Appendices A and B.

    The parameters used to model the optical behavior of crystal quartz were obtained from the parameters given by Estevam et al. [25], built on the work of Gervais and Piraeus [79]. These parameters include the high-frequency permittivity ε, frequencies of the transverse optical (TO) phonons and of the longitudinal optical (LO) phonons, and the appropriate damping parameters responsible for absorption around the phonon frequencies.

    A method for calculating the wavevector solutions to be calculated using the dielectric tensor is also included in Appendix A. These solutions then allow for the fields at the interface to be calculated, which can then be matched with that of the air gap (and other layers) and ultimately trace the frequency of specific polariton modes, taking into account all layers. For understanding these mathematical solutions (for both the GHP and the LHP), similar to our context building within Eq. (3), we refer the reader to the supplementary material in Ref. [11], along with Refs. [5052].

    The experimental data was collected via reflectance measurements using Fourier-transform infrared spectroscopy with a Bruker Vertex 70 spectrometer. The spectra featured a resolution of 4  cm1, and each spectrum was averaged 15 times.

    A KRS-5 polarizer was placed in the path of the incident beam to obtain spectra for p-polarized light.

    To obtain ATR spectra, a diamond coupling prism was used with a dielectric constant εp=5.5 and at a fixed incident angle of 45°. To introduce an appropriate air gap, 1.5 μm silica spacers were thinly coated over the ATR stage. Throughout the azimuthal rotation, the silica spacers were partially moved, so extra care was taken in order to maintain a consistent air gap thickness. There is significant margin for error, but results show clear agreement with theory despite this. Experimental results align with a theoretical air gap distance of 2 μm, with variation between 1.5 and 3 μm (see Appendix C for details of the error associated with the air gap and its effect on reflectance).

    The crystal quartz samples used were provided by Boston Piezo Optics Inc. The anisotropy orientation was determined with respect to the crystal’s surface using single-crystal X-ray diffraction, with the crystal mounted on a goniometer for precise positioning at selected orientations. These samples were then cut into flat slabs of chemically polished faces of 20 mm in diameter and 10 mm in thickness. The faces were cut at specific angles with respect to the anisotropy; one of our samples had anisotropy set at φ=45° and another at φ=90°. Figure 3(a) contains experimental results for the φ=45° sample and Fig. 3(b) contains experimental results for the φ=90° sample.

    Acknowledgment

    Acknowledgment. M.C.C. acknowledges funding from the EPSRC. We thank N. Parry, C. A. McEleney, M. Smith, A. Joseph, K. Stevens, A. MacGruer, and S. Mekhail for useful insights, discussion, and helpful comments on the manuscript.

    APPENDIX A: DIELECTRIC TENSOR AND TWISTED ANISOTROPY ORIENTATION

    In a uniaxial material like crystal quartz, and when the crystal axes are aligned with the laboratory axes, the dielectric tensor can be written as follows: ε=[ε000ε000ε],where ε denotes the anisotropy axis (in this case along z), and ε denotes the axes perpendicular to the anisotropy (in our case along x and y).

    Throughout this paper, we have described the rotation of the anisotropy axis by two angles: φ, which is the angle between the anisotropy and the crystal’s surface, and β, which represents a rotation of the incidence plane with respect to the plane where the anisotropy axis lies (here xz). Mathematically, these angles correspond to matrix transformations about the y axis and z axis, respectively. The rotation of the anisotropy axis by the angle φ as described in this work is represented by a matrix transformation around the y axis done by Tφ=[cosφ0sinφ010sinφ0cosφ],and conversely, the rotation β corresponds to a rotation around the z axis given by Tβ=[cosβsinβ0sinβcosβ0001].The overall rotation matrix is thus given by T=TβTφ,and the overall rotated permittivity matrix is given by ε=TεT1.This results in a 3×3 tensor of an arbitrarily oriented anisotropic material, ready to be used in the transfer matrix method: ε=[εxxεxyεxzεyxεyyεyzεzxεzyεzz].With this dielectric tensor, the source-free Maxwell equations are as follows for a plane wave solution ei(krωt) [11,75,77]: (εxxk02kz2εxyk02εxzk02+kxkzεxyk02εyyk02kz2kx2εyzk02εzxk02+kzkxεzyk02εzzk02kx2)(ExEyEz)=0.To obtain solutions for kz, the determinant of the matrix in this equation must vanish [77]. This then gives a quartic equation that gives four roots (either complex or real) of kz, which are in conjugate pairs. The two pairs are equivalent to forward and backward propagating waves, and each pair contains an ordinary solution and an extraordinary solution. We will go on to show how kz values can be obtained using the transfer matrix method.

    APPENDIX B: TRANSFER MATRIX METHOD

    The Berreman 4×4 transfer matrix method, introduced in 1971 [74] and later optimized [36,75,78] for more straightforward implementation, calculates eigenvalues for four wave components inside a randomly oriented anisotropic medium, with associated eigenvectors providing boundary conditions. The method can be easily expanded for multiple layers, making it highly useful for ATR simulations. Reflection and transmission coefficients can be computed for all polarizations (Rpp,Rps,Rsp,Rss), enabling accurate modeling of anisotropic multilayer systems with different anisotropy axis orientations [22]. Here, we summarize this method that was used throughout the main paper to obtain the theoretical ATR spectra and begin with the definition of a plane wave: E=E0ei(krωt)and H=H0ei(krωt).

    Since we are interested in multiple rotations (as outlined in Appendix A), we consider an arbitrary anisotropic material, with fully anisotropic dielectric permittivity and magnetic permeability tensors: εr=[εxxεxyεxzεyxεyyεyzεzxεzyεzz]and μr=[μxxμxyμxzμyxμyyμyzμzxμzyμzz].We can then employ Maxwell’s equations and the electromagnetic constitutive relations, which in CGS units take the following form: Δ×E=1cμrHtand Δ×H=1cεrEt.By solving the partial derivatives [using Eqs. (B1) and (B2)] as well as making ω/c=k0 we get Δ×E=ik0μrHand Δ×H=ik0εrE.We can also say that xikx and yiky and since there is no contribution from the y-component of the wavevector, y0. We will not extend this to the z-component, as the sample will not be homogenous in z. Therefore we will keep z the way it is. From this point on, we will normalize our spatial components by a factor of k0 whereby Kxkxk0,which is known as the reduced wavevector, and zk0zso that z1k0z.This leaves us with Δ×E=iμrHand Δ×H=iεrE.

    Following from Eq. (B12) we get |ijkiKx0zExEyEz|=i[μxxμxyμxzμyxμyyμyzμzxμzyμzz][HxHyHz],which gives us three linear equations: zEy=i(μxxHx+μxyHy+μxzHz),zExiKxEz=i(μyxHx+μyyHy+μyzHz),and iKxEy=i(μzxHx+μzyHy+μzzHz).These equations can then be rearranged as 1izEy=(μxxHx+μxyHy+μxzHz),1izEx=KxEz+μyxHx+μyyHy+μyzHz,and Hz=1μzz(KxEyμzxHxμzyHy).

    Repeating this process for Eq. (B13) yields 1izHy=εxxHx+εxyHy+εxzEz,1izHx=KxHzεyxExεyyEyεyzEz,and Ez=1εzz(KxHy+εzxEx+εzyEy).With this, we now have expressions for Ez and Hz in terms of Ex, Ey, Hx, and Hy, along with four equations for the partial derivatives of Ex, Ey, Hx, and Hy with respect to z in terms of Ez and Hz.

    Now we can substitute Ez and Hz into Eqs. (B18), (B19), (B21), and (B22). We begin with Eq. (B19): 1izEx=Kx[1εzz(KxHy+εzxEx+εzyEy)]+μyxHx+μyyHy+μyz[1μzz(KxEyμzxHxμzyHy)],which after substantial rearranging yields 1izEx=Ex[Kx(εzxεzz)]+Ey[Kx(μyzμzzεzyεzz)]+Hx(μyxμyzμzxμzz)+Hy(μyyμyzμzyμzzKxεzyεzz).Equation (B18) becomes 1izEy=μxxHxμxyHyμxzμzz(KxEyμzxHxμzyHy),which after rearranging yields 1izEy=Ey(Kxμxzμzz)+Hx(μxzμzxμzzμxx)+Hy(μxzμzyμzzμxy).Equation (B22) now is 1izHx=Kx[1μzz(KxEyμzxHxμzyHy)]εyxExεyyEyεyz[1εzz(KxHy+εzxEx+εzyEy)],which after rearranging takes the form 1izHx=Ex(εyzεzxεzzεyx)+Ey(Kx2μzz+εyzεzyεzzεyy)+Hx(Kxμzxμzz)+Hy[Kx(εyzεzzμzyμzz)].Finally, Eq. (B21) can be written as 1izHy=εxxHx+εxyHy+εxz[1εzz(KxHy+εzxEx+εzyEy)],and after rearranging it becomes 1izHy=Ex(εxxεxzεzxεzz)+Ey(εxyεxzεzyεzz)+Hy(Kxεxzεzz).

    With Eqs. (B25), (B27), (B29), and (B31), we have four linearly independent equations in terms of the partial z derivative for each component of an incident wave of arbitrary polarization. These four equations can be written in the form z[ExEyHxHy]=iΔ[ExEyHxHy],where Δ is a 4×4 matrix: Δ[Kx(εzxεzz)Kx(μyzμzzεzyεzz)μyxμyzμzxμzzμyyμyzμzyμzzKxεzyεzz0KxμxzμzzμxzμzxμzzμxxμxzμzyμzzμxyεyzεzxεzzεyxKx2μzz+εyzεzyεzzεyyKxμzxμzzKx(εyzεzzμzyμzz)εxxεxzεzxεzzεxyεxzεzyεzz0Kxεxzεzz].

    The overall partial transfer matrix T for a given material of arbitrary thickness d is then given by T=exp(ik0Δd).As our wavenumber ω is measured in cm1, the thickness d is given in cm for the purpose of our analysis. When taking the exponential of the 4×4 matrix, it would be too computationally intensive to calculate the exponential of every element. Instead, we can find the eigenvalues and corresponding column eigenvectors to apply the exponential function exp(Δ)=VeλV1,where V is the matrix of eigenvectors and λ is the diagonal matrix of eigenvalues. The eigenvalues will be four values, with the eigenvectors in a 4×4 matrix, where each nth column is the column eigenvector for the nth eigenvalue.

    Therefore, the transfer matrix for a given material is given by T=Vexp(iλk0d)V1,where the eigenvectors V correspond to the boundary conditions at the entry interface of the medium. The eigenvalues λ tell us the propagation properties of each mode inside the medium. The inverses of the eigenvectors V1 correspond to the boundary conditions at the exit interface of the medium.

    By repeating this method for all the films in a system, an overall transfer matrix can be found by multiplying each partial transfer matrix in the corresponding order of each medium. A full transfer matrix can be made by projecting the fields into the ambient and substrate media, given by T¯=Li1TLt,where Li1=[011ncosθi0011ncosθi01cosθi001n1cosθi001n]and Lt=[00AA1100AnsA0000nsns],where A=cosθt [78].

    When we wish to model our final layer as semi-infinite, we do not extend our transfer matrix in the same way as we do with an isotropic substrate, as there is no singular refractive index value that we can use. To refresh, the fields in our system can be expressed as follows: [AsBsApBp]=T[CsDsCpDp],where s and p denote polarizations, A denotes positive traveling waves in the initial medium, and B denotes backward waves in the initial medium, with C and D denoting the respective counterparts in the exit medium. When calculating the 4×4 transfer matrix, the column eigenvectors are the boundary conditions of the layer for each mode of propagation, represented by each eigenvalue. For a semi-infinite layer, we assume that there are no backward-traveling waves, which means that Ds=Dp=0. To achieve this, we need to examine the four eigenvalues of the matrix. Two eigenvalues correspond to forward waves, and the other two correspond to backward waves. We must sort these eigenvalues by their imaginary components, so that evanescent waves are decaying exponentially from the interface, to satisfy the conservation of energy. We also extract the two column eigenvectors linked with the positive-traveling eigenvalues. We then arrange these eigenvectors in the first and third columns of the matrix so that they can be properly multiplied by Cs and Cp. The remaining two eigenvectors related to backward-traveling waves are discarded. Now, the partial transfer matrix of an anisotropic semi-infinite layer can be expressed as a 4×4 matrix, where the first and third columns contain the “positive” eigenvectors, while the second and fourth columns are set equal to zero.

    Now that the overall transfer matrix is found for the full system needed for our ATR investigation, which can be composed of an arbitrary number of anisotropic layers or arbitrary anisotropy axis orientation, the reflection and transmission coefficients of the whole system can easily be found using [AsBsApBp]=[T11T12T13T14T21T22T23T24T31T32T33T34T41T42T43T44][Cs0Cp0].In this work, we are most interested in the reflection coefficients, and for all polarizations from this transfer matrix these are rpp,rps,rsp,rss. Namely, rpp represents the ratio of p-polarized light exiting the medium to p-polarized light entering the medium, i.e., when As=0. As a function of the transfer matrix components, rpp is given by rpp=BpApAs=0,where As=M11Cs+M13Cp=0,Cs=M13M11Cp,Bp=M41Cs+M43Cp,and Ap=M31Cs+M33Cp.Substituting Cs into Bp and Ap we obtain rpp=BpApAs=0=M11M43M41M13M11M33M13M31.

    By similar analysis, we can find the other reflection coefficients. For instance, rss represents the ratio of s-polarized light exiting the medium to s-polarized light entering the medium, i.e., when Ap=0, and it is given by rss=BsAsAp=0=M21M33M23M31M11M33M13M31.Similarly, rsp represents the ratio of p-polarized light exiting the medium to s-polarized light entering the medium, i.e., when Ap=0, and it is given by rsp=BpAsAp=0=M41M33M43M31M11M33M13M31.Finally, rps represents the ratio of s-polarized light exiting the medium to p-polarized light entering the medium, i.e., when As=0, and it can be written as rps=BsApAs=0=M11M23M21M13M11M33M13M31.

    With these coefficients, the reflectance for each polarization can be calculated as Rpp=rpprpp*,Rps=rpsrps*,Rsp=rsprsp*,and Rss=rssrss*.

    We can also define quantities Rp=Rpp+Rpsand Rs=Rsp+Rss,which represent the total reflectance of p-polarized and s-polarized incident radiation, respectively. Note that throughout the main body of our work, our reflectivity is given by the quantity Rp as we only considered the case of p-polarized incident radiation.

    APPENDIX C: CRITICAL COUPLING BY VARYING AIR GAP

    As mentioned in Section 5, our experimental air gap size was inconsistent due to silicon beads of thickness d=1.5  μm moving and stacking on top of each other upon azimuthal rotation of the sample. Therefore, we theoretically investigated various air gap sizes that would match most closely with the experimental results. For our experimental data (Figs. 1 and 3 of the main article), we selected a theoretical air gap of d=2  μm to compare with experimental ATR results. In Fig. 8, we show two other air gap sizes [in Fig. 8(a) d=1.5  μm and in Fig. 8(b) d=2.5  μm]. We can see how in both the elliptical surface wave is slightly not matching with the experimental result. In Fig. 8(a) the peak frequency at β=180° is slightly lower in the theoretical results compared with the experimental while in Fig. 8(b) the coupling of the surface polariton is much stronger and overall frequencies match well with the experiment; however it is coupled slightly more than the experimental value as evidenced by higher reflectance at bulk frequencies. As these are qualitative observations, it was deemed that d=2  μm was most appropriate for inclusion within the main body of this paper as it is a good match for both the frequency of the surface mode and overall intensity matching.

    The dependence of ATR in crystal quartz on the azimuthal angle β when φ=90° and kxk0=1.66. We show our experimental work alongside two different theoretical air gap sizes, where in (a) d=1.5 μm and in (b) d=2.5 μm.

    Figure 8.The dependence of ATR in crystal quartz on the azimuthal angle β when φ=90° and kxk0=1.66. We show our experimental work alongside two different theoretical air gap sizes, where in (a) d=1.5  μm and in (b) d=2.5  μm.

    APPENDIX D: CROSS POLARIZATION CONVERSION OF THE GHOST HYPERBOLIC POLARITON

    Asymmetric cross polarization conversion has previously been observed in bulk Type I hyperbolic dispersion [34]. In Fig. 9, we show the value Rps, the reflected radiation that possesses s-polarization from incident p-polarized radiation, associated with Type II hyperbolic dispersion and the GHP. In Fig. 9(a), where there is no air gap (d=0  μm) and φ=90°, we can see minimal cross polarization conversion, at a maximum in an “X” shape at 45° intervals of the angle β. In Fig. 9(b), where φ=90° and d=0.1  μm, the maximum Rps has increased to around 0.27 due to the GHP, in a more pronounced symmetric “X” shape. When we tilt the anisotropy to φ=60° with no air gap (d=0  μm) in Fig. 9(c), asymmetry is introduced in the cross polarization conversion, with negative kx values possessing Rps values around 0.15, in contrast with positive kx values possessing Rps values around 0.1. Re-introducing the air gap (d=0.1  μm) in Fig. 9(d), Rps becomes much more noticeably asymmetric, reaching a maximum of around 0.36 for negative kx values, and a maximum of around 0.26 for positive kx values. Moreover, the pronounced “X” shape has compressed inwards, joining slightly at kx/k0=0.

    The cross polarization conversion (Rps) induced by the GHP in quartz at ω/2πc=460 cm−1. This quantity is the amount of s-polarized light reflected off the surface from incident p-polarized radiation. The radius corresponds to kx where εp=50, and the azimuthal angle corresponds to the angle β. The white circle denotes where kx/k0=1. In (a) there is no air gap (d=0 μm) and φ=90°. In (b) the anisotropy orientation is unchanged (φ=90°) and an air gap is introduced to study the GHP, with d=0.1 μm. In (c), the air gap is removed (d=0 μm) and the anisotropy is rotated to φ=60° to alter the hyperbolic dispersion. In (d), the anisotropy orientation is unchanged (φ=60°) and an air gap is introduced again to study the GHP, with d=0.1 μm.

    Figure 9.The cross polarization conversion (Rps) induced by the GHP in quartz at ω/2πc=460  cm1. This quantity is the amount of s-polarized light reflected off the surface from incident p-polarized radiation. The radius corresponds to kx where εp=50, and the azimuthal angle corresponds to the angle β. The white circle denotes where kx/k0=1. In (a) there is no air gap (d=0  μm) and φ=90°. In (b) the anisotropy orientation is unchanged (φ=90°) and an air gap is introduced to study the GHP, with d=0.1  μm. In (c), the air gap is removed (d=0  μm) and the anisotropy is rotated to φ=60° to alter the hyperbolic dispersion. In (d), the anisotropy orientation is unchanged (φ=60°) and an air gap is introduced again to study the GHP, with d=0.1  μm.

    APPENDIX E: AIR GAP DEPENDENCE OF THE GHOST HYPERBOLIC POLARITON

    As outlined previously in Appendix C, the chosen air gap size affects the coupling with the surface polariton due to the decay length of evanescent waves at the prism/air interface.

    In Fig. 10, we show how changing the air gap affects the reflectance associated with the GHP in quartz at ω/2πc=465  cm1, when the anisotropy is aligned with the surface (φ=90°). In Fig. 10(a) d=0.1  μm and the GHP is clearly tracing the bulk hyperbolic dispersion. At kx/k0=0, the GHP’s drop in reflectance is quite thick, supported for ky/k0 values between four and six. We increase the air gap thickness to d=0.15  μm in Fig. 10(b), where the GHPs signature hyperbolic shape becomes thinner and moves in closer to the bulk dispersion, now supported for ky/k0 values between 3.5 and 4.5 when kx/k0=0. The four directional lobes are slightly more prominent here, but supported at smaller k values than Fig. 10(a). Increasing the air gap thickness further to d=0.2  μm in Fig. 10(c) begins to diminish the reflective presence of the GHP. At kx/k0=0, the GHP is supported for ky/k0 values between three and four, overlapping with the bulk hyperbola, where bulk propagation was forbidden with no air gap as shown in Fig. 4(a) in the main paper. Increasing the air gap to d=0.25  μm in Fig. 10(d) removes most traces of the GHP’s reflective footprint, except for the drop in reflectivity at kx/k0=0.

    The dependency of the ATR response of quartz on the air gap thickness d at constant frequency ω/2πc=465 cm−1 and the anisotropy axis aligned with the surface (φ=90°), with the radius corresponding to kx where εp=80, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) d=0.1 μm. In (b) d=0.15 μm. In (c) d=0.2 μm. In (d) d=0.25 μm.

    Figure 10.The dependency of the ATR response of quartz on the air gap thickness d at constant frequency ω/2πc=465  cm1 and the anisotropy axis aligned with the surface (φ=90°), with the radius corresponding to kx where εp=80, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) d=0.1  μm. In (b) d=0.15  μm. In (c) d=0.2  μm. In (d) d=0.25  μm.

    APPENDIX F: FREQUENCY DEPENDENCE OF THE GHOST HYPERBOLIC POLARITON

    Quartz

    We have shown how the GHP can be supported in the Type II hyperbolic region in quartz. However, compared to calcite where the positive ε is constant through the Type II region, in quartz both ε and ε vary greatly throughout the hyperbolic band. With a constant air gap d=0.1  μm and the anisotropy axis aligned with the surface (φ=90°), in Fig. 11, we show how the GHP is supported at different frequencies throughout the Type II hyperbolic region in quartz, from 455 to 470  cm1. As the frequency increases within this range, the magnitude of the positive ε increases from 8 to 13.5, while the negative ε shrinks from 27 to 6. In Fig. 11(a) at 455  cm1, the hyperbolic dispersion is quite flat, so the GHP is not very clear, but can be slightly observed emanating outwards as faint horizontal lines at ky/k0=4. In Figure 11(b) at 460  cm1 the GHP is much more prevalent, as observed in the main paper. Increasing the frequency further to 465  cm1 in Fig. 11(c), the hyperbolic dispersion widens, causing the GHP to be supported at narrower kx values, but larger ky values. This trend continues with the increasing frequency to 470  cm1 in Fig. 11(d), with a much narrower reflective footprint, with a smaller dip in reflectance compared to Figs. 11(b) and 11(c). These results suggest how the GHP can isolate specific frequencies depending on crystal orientation.

    The frequency-dependent ATR response of quartz with a constant air gap d=0.1 μm and the anisotropy axis aligned with the surface (φ=90°), with the radius corresponding to kx where εp=80, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) ω/2πc=455 cm−1. In (b) ω/2πc=460 cm−1. In (c) ω/2πc=465 cm−1. In (d) ω/2πc=470 cm−1.

    Figure 11.The frequency-dependent ATR response of quartz with a constant air gap d=0.1  μm and the anisotropy axis aligned with the surface (φ=90°), with the radius corresponding to kx where εp=80, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) ω/2πc=455  cm1. In (b) ω/2πc=460  cm1. In (c) ω/2πc=465  cm1. In (d) ω/2πc=470  cm1.

    The frequency-dependent ATR response of calcite with a constant air gap d=0.5 μm and the anisotropy axis aligned with the surface (φ=90°), with the radius corresponding to kx where εp=18, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) ω2πc=1460 cm−1. In (b) ω2πc=1470 cm−1. In (c) ω2πc=1480 cm−1. In (d) ω2πc=1490 cm−1.

    Figure 12.The frequency-dependent ATR response of calcite with a constant air gap d=0.5  μm and the anisotropy axis aligned with the surface (φ=90°), with the radius corresponding to kx where εp=18, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) ω2πc=1460  cm1. In (b) ω2πc=1470  cm1. In (c) ω2πc=1480  cm1. In (d) ω2πc=1490  cm1.

    APPENDIX G: CROSS POLARIZATION CONVERSION OF THE LEAKY HYPERBOLIC POLARITON

    As mentioned previously, asymmetric cross polarization conversion has previously been observed in bulk Type I hyperbolic dispersion [34]. In Fig. 13, we show the value Rps, the proportion of the reflected radiation that possesses s-polarization from incident p-polarized radiation, associated with Type I hyperbolic dispersion and the LHP.

    The cross polarization conversion (Rps) induced by the LHP in quartz at ω2πc=545 cm−1. This quantity is the amount of s-polarized light reflected off the surface from incident p-polarized radiation. The radius corresponds to kx where εp=4.5, and the azimuthal angle corresponds to the angle β. The white circle denotes where kx/k0=1. In (a) there is no air gap (d=0 μm) and φ=90°. In (b) the anisotropy orientation is unchanged (φ=90°) and an air gap is introduced to study the LHP, with d=10 μm. In (c), the air gap is removed (d=0 μm) and the anisotropy is rotated to φ=70° to alter the hyperbolic dispersion. In (d), the anisotropy orientation is unchanged (φ=70°) and an air gap is introduced again to study the LHP, with d=10 μm.

    Figure 13.The cross polarization conversion (Rps) induced by the LHP in quartz at ω2πc=545  cm1. This quantity is the amount of s-polarized light reflected off the surface from incident p-polarized radiation. The radius corresponds to kx where εp=4.5, and the azimuthal angle corresponds to the angle β. The white circle denotes where kx/k0=1. In (a) there is no air gap (d=0  μm) and φ=90°. In (b) the anisotropy orientation is unchanged (φ=90°) and an air gap is introduced to study the LHP, with d=10  μm. In (c), the air gap is removed (d=0  μm) and the anisotropy is rotated to φ=70° to alter the hyperbolic dispersion. In (d), the anisotropy orientation is unchanged (φ=70°) and an air gap is introduced again to study the LHP, with d=10  μm.

    In Fig. 13(a), where there is no air gap (d=0  μm) and φ=90°, cross polarization conversion is minimal and totally symmetric and extends outside of the free space light cone (denoted by the white circle). By introducing an air gap of d=10  μm [see Fig. 13(b) where φ=90°] we can see how the cross polarization conversion has increased to a value of around 0.35, and is totally symmetric. When we tilt the anisotropy to φ=70° in Fig. 13(c) with no air gap, asymmetry is introduced in the cross polarization conversion, which is identical to the process previously observed in Ref. [34]. Tilting the anisotropy to φ=60° in Fig. 13(d), Rps becomes much more noticeably asymmetric, reaching a maximum of around 0.7 for negative kx values, and a maximum of around 0.1 for positive kx values. Interestingly, this is within the free-space light cone, showing how evanescent behavior from introducing the air gap is influencing polarization, despite this being at incident angles smaller than what would induce total internal reflection.

    APPENDIX H: FREQUENCY DEPENDENCE OF THE LEAKY HYPERBOLIC POLARITON

    We have shown how LHPs can be supported in the Type I hyperbolic region and ENZ region in quartz. With a constant air gap d=10  μm and the anisotropy axis aligned with the surface (φ=90°), in Fig. 14, we show how the leaky polariton is supported at different frequencies in this region, from 540 to 555  cm1. As the frequency increases within this range, ε increases from 0.64 to positive 0.26, while the positive ε increases from 1.33 to 1.69. The reflectivity begins with a closed lenticular shape, with the LHP supported very closely to the light line (the white circle). As the frequency increases, the points of this lenticular shape move outward to higher kx values and begin to open as ε becomes positive, moving further apart. This shows how in the ENZ region, the leaky polariton propagates at an angle in the x-y plane. When ε is negative, this canalizes the polariton along the x axis.

    The frequency-dependent ATR response of quartz with a constant air gap d=10 μm and the anisotropy axis aligned with the surface (φ=90°), with the radius corresponding to kx where εp=4.5, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) ω/2πc=540 cm−1. In (b) ω/2πc=545 cm−1. In (c) ω/2πc=550 cm−1. In (d) ω/2πc=555 cm−1.

    Figure 14.The frequency-dependent ATR response of quartz with a constant air gap d=10  μm and the anisotropy axis aligned with the surface (φ=90°), with the radius corresponding to kx where εp=4.5, and the azimuthal angle corresponding to the angle β. The white circle denotes where kx/k0=1. In (a) ω/2πc=540  cm1. In (b) ω/2πc=545  cm1. In (c) ω/2πc=550  cm1. In (d) ω/2πc=555  cm1.

    [4] R. E. Camley, T. Dumelow, R. L. Stamps. Chapter 2: Negative refraction and imaging from natural crystals with hyperbolic dispersion. Solid State Physics, 67, 103-182(2016).

    [19] A. Moradi, A. Moradi. Reflection and refraction of electrostatic waves at hyperbolic surfaces. Theory of Electrostatic Waves in Hyperbolic Metamaterials, 63-85(2023).

    [46] M. I. D’yakonov. New type of electromagnetic wave propagating at an interface. Sov. J. Exp. Theor. Phys., 67, 714(1988).

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    Mark Cunningham, Adam L. Lafferty, Mario González-Jiménez, Rair Macêdo, "Optical footprint of ghost and leaky hyperbolic polaritons," Photonics Res. 13, 2291 (2025)

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    Paper Information

    Category: Surface Optics and Plasmonics

    Received: Feb. 5, 2025

    Accepted: May. 19, 2025

    Published Online: Jul. 31, 2025

    The Author Email: Mark Cunningham (m.cunningham.2@research.gla.ac.uk)

    DOI:10.1364/PRJ.558334

    CSTR:32188.14.PRJ.558334

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