{"id":183533,"date":"2025-10-01T22:01:13","date_gmt":"2025-10-01T22:01:13","guid":{"rendered":"https:\/\/www.newsbeep.com\/ca\/183533\/"},"modified":"2025-10-01T22:01:13","modified_gmt":"2025-10-01T22:01:13","slug":"multimode-phonon-polaritons-in-lead-halide-perovskites-in-the-ultrastrong-coupling-regime","status":"publish","type":"post","link":"https:\/\/www.newsbeep.com\/ca\/183533\/","title":{"rendered":"Multimode phonon-polaritons in lead-halide perovskites in the ultrastrong coupling regime"},"content":{"rendered":"<p>We fabricated an array of nanoslots (w\u00a0=\u00a0950 nm) on quartz substrates with seven different lengths (l\u00a0= 30, 40, 50, 60, 80, 120, and 160 \u03bcm) to tune the cavity mode frequency, given by \\({\\omega }_{{{{\\rm{c}}}}}\/(2\\pi )={c}_{0}\/(2l\\sqrt{{\\epsilon }_{{{{\\rm{avg}}}}}})\\), where c0 is the speed of light in vacuum and \u03f5avg\u00a0=\u00a0(\u03f5air\u00a0+\u00a0\u03f5sub)\/2 represents the average dielectric constant of air and the quartz substrate (\u03f5sub\u00a0=\u00a02.\u00a012)<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 33\" title=\"Kang, J. H., Choe, J.-H., Kim, D. S. &amp; Park, Q.-H. Substrate effect on aperture resonances in a thin metal film. Opt. Express 17, 15652&#x2013;15658 (2009).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR33\" id=\"ref-link-section-d108692028e1584\" rel=\"nofollow noopener\" target=\"_blank\">33<\/a>; see Methods for sample preparation details. The resonance frequency is predominantly governed by the geometry of a single nanoslot rather than that of the periodic array<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 34\" title=\"Garcia-Vidal, F. J., Moreno, E., Porto, J. A. &amp; Martin-Moreno, L. Transmission of light through a single rectangular hole. Phys. Rev. Lett. 95, 103901 (2005).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR34\" id=\"ref-link-section-d108692028e1588\" rel=\"nofollow noopener\" target=\"_blank\">34<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 35\" title=\"Al&#xF9;, A. &amp; Engheta, N. Light squeezing through arbitrarily shaped plasmonic channels and sharp bends. Phys. Rev. B 78, 035440 (2008).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR35\" id=\"ref-link-section-d108692028e1591\" rel=\"nofollow noopener\" target=\"_blank\">35<\/a>. Figure\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>b illustrates the structure of our samples, where perovskite films (purple) are coated both on top of and within the slots.<\/p>\n<p>These films exhibit two distinct optical phonon modes in free space, labeled as \u03bb\u00a0=\u00a01 and \u03bb\u00a0=\u00a02, corresponding to the rocking and stretching of Pb\u2013I bonds, respectively. Due to the orientational disorder of methylammonium molecules, which breaks the lattice space-group symmetry, these phonons acquire a mixed transverse-optical (TO) and longitudinal-optical (LO) character<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 36\" title=\"La-o-vorakiat, C. et al. Phonon mode transformation across the orthorhombic-tetragonal phase transition in a lead iodide perovskite CH3NH3PbI3: A terahertz time-domain spectroscopy approach. J. Phys. Chem. Lett. 7, 1&#x2013;6 (2016).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR36\" id=\"ref-link-section-d108692028e1607\" rel=\"nofollow noopener\" target=\"_blank\">36<\/a>. As a result, they not only exhibit strong infrared absorption<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 36\" title=\"La-o-vorakiat, C. et al. Phonon mode transformation across the orthorhombic-tetragonal phase transition in a lead iodide perovskite CH3NH3PbI3: A terahertz time-domain spectroscopy approach. J. Phys. Chem. Lett. 7, 1&#x2013;6 (2016).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR36\" id=\"ref-link-section-d108692028e1611\" rel=\"nofollow noopener\" target=\"_blank\">36<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 37\" title=\"Sendner, M. et al. Optical phonons in methylammonium lead halide perovskites and implications for charge transport. Mater. Horiz. 3, 613&#x2013;620 (2016).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR37\" id=\"ref-link-section-d108692028e1614\" rel=\"nofollow noopener\" target=\"_blank\">37<\/a> but also interact with lattice electrons, as recently observed<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 5\" title=\"Qu, S. et al. Mode-resolved, non-local electron&#x2013;phonon coupling in two-dimensional spectroscopy. Nat. Phys. 21, 953&#x2013;960 (2025).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR5\" id=\"ref-link-section-d108692028e1618\" rel=\"nofollow noopener\" target=\"_blank\">5<\/a>. Moreover, low-frequency phonons are particularly beneficial for achieving USC, as the normalized coupling strength g\/\u03c9 increases with decreasing phonon frequency. This study, therefore, focuses on the phonons that are most relevant to strong interactions with both photonic and electronic degrees of freedom. Since electron\u2013phonon interactions dictate charge mobility and recombination through long-range Coulomb forces, phonon-polariton formation involving low-frequency hybrid TO\/LO phonons could offer effective pathways to engineer charge transport in lead halide perovskites.<\/p>\n<p>Nanoslot resonators provide significant electric field enhancement due to strong optical confinement within and around the slots<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 38\" title=\"Seo, M. A. et al. Terahertz field enhancement by a metallic nano slit operating beyond the skin-depth limit. Nat. Photonics 3, 152&#x2013;156 (2009).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR38\" id=\"ref-link-section-d108692028e1632\" rel=\"nofollow noopener\" target=\"_blank\">38<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 39\" title=\"Kim, D. et al. Giant field enhancements in ultrathin nanoslots above 1 terahertz. ACS Photonics 5, 1885&#x2013;1890 (2018).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR39\" id=\"ref-link-section-d108692028e1635\" rel=\"nofollow noopener\" target=\"_blank\">39<\/a>. Since the phonon-photon coupling strength \\(g\\propto \\sqrt{N\/V}\\), where N is the number of unit cells in the crystal and V is the resonator mode volume, the small mode volume of nanoslot resonators enables ultrastrong light\u2013matter interaction regimes even with small perovskite crystals.<\/p>\n<p>The in-plane spatial distribution of the cavity mode, computed using COMSOL for a perovskite-filled nanoslot, is shown in Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>c (left panel). The field profile follows a sinusoidal pattern<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 16\" title=\"Roh, Y. et al. Ultrastrong coupling enhancement with squeezed mode volume in terahertz nanoslots. Nano Lett. 23, 7086&#x2013;7091 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR16\" id=\"ref-link-section-d108692028e1683\" rel=\"nofollow noopener\" target=\"_blank\">16<\/a> along the y-axis, with an electric field enhancement factor of 20 relative to transmission through a bare quartz substrate. The strong confinement of the x-component of the electric field (Ex) along the x- and z-axes results in a nearly uniform electric field within the perovskite region (Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>c, right panel). Although the nanoslot thickness is 130 nm, the cavity mode extends beyond the nanoslot into the surrounding MAPbI3 layer, as depicted in Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>c. The electric field strength above the nanoslot remains comparable to that inside, indicating that the perovskite film covering the slot also contributes to light\u2013matter coupling. Notably, when t becomes comparable to the mode\u2019s spatial extent along z, where t is the perovskite film thickness, g saturates at its maximum value; see Supplementary Note\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">4<\/a> and Supplementary Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">8<\/a>.<\/p>\n<p>We characterized the perovskite-nanoslot hybrid system using THz-TDS at room temperature. A normal-incident THz beam was linearly polarized along the x-axis. In free space, a 200-nm-thick MAPbI3 film exhibits transmittance dips at \u03c91\/(2\u03c0)\u00a0=\u00a00.96 THz and \u03c92\/(2\u03c0)\u00a0=\u00a01.9 THz, corresponding to the two phonon modes \u03bb\u00a0=\u00a01 and \u03bb\u00a0=\u00a02, respectively (Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>a). The bare cavity resonance appears as a single peak in the transmission spectrum. Figure\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>b displays the cavity resonance frequency as a function of cavity length l. By adjusting l, the cavity mode can be brought into resonance with either the \u03bb\u00a0=\u00a01 mode (\u03c9c\u00a0=\u00a0\u03c91) or the \u03bb\u00a0=\u00a02 mode (\u03c9c\u00a0=\u00a0\u03c92).<\/p>\n<p>Fig. 2: Terahertz transmission spectra.<a class=\"c-article-section__figure-link\" data-test=\"img-link\" data-track=\"click\" data-track-label=\"image\" data-track-action=\"view figure\" href=\"https:\/\/www.nature.com\/articles\/s41467-025-63810-7\/figures\/2\" rel=\"nofollow noopener\" target=\"_blank\"><img decoding=\"async\" aria-describedby=\"Fig2\" src=\"https:\/\/www.newsbeep.com\/ca\/wp-content\/uploads\/2025\/10\/41467_2025_63810_Fig2_HTML.png\" alt=\"figure 2\" loading=\"lazy\" width=\"685\" height=\"317\"\/><\/a><\/p>\n<p>a Transmission spectra for bare cavities (nanoslots) with different lengths l (green curves) showing a single cavity mode. The green dashed line shows the simulated transmittance through the nanoslot (l\u00a0=\u00a080\u2009\u03bcm). Transmission spectrum for a 200-nm-thick bare MAPbI3 film (black curve) showing two transmission dips due to the two optical phonon modes (\u03bb\u00a0=\u00a01 and \u03bb\u00a0=\u00a02) with angular frequencies \u03c91 and \u03c92, respectively. b The bare cavity resonance frequency as a function of nanoslot length l in the reciprocal axis (green circles). The linear fit (green dashed line) shows good agreement with the experimental data. The \u03bb\u00a0=\u00a01\u2013cavity and \u03bb\u00a0=\u00a02\u2013cavity resonances occur with an 80-\u03bcm-long slot and with a 50-\u03bcm-long slot, respectively, when the cavity mode frequency coincides with the phonon frequencies (red and blue dashed lines). c Transmission spectra for the MAPbI3\u2013nanoslots hybrid system showing three polariton branches. UP upper polariton, MP middle polariton, and LP lower polariton. The dashed lines indicate the two phonon frequencies. The spectra are vertically offset by 0.2 for clarity. d Numerical simulation (COMSOL) of the transmission as a function of cavity frequency (color map). Each spectrum has been normalized by its maximum transmittance to clearly show the three polariton branches; the black solid circles are the experimental results.<\/p>\n<p>Figure\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a> c presents the transmission spectra of MAPbI3\u2013nanoslot structures for different l values. As the nanoslots predominantly reflect incoming radiation, the observed polariton modes appear as transmission peaks. The spectra exhibit three distinct polariton branches: lower (LP), middle (MP), and upper (UP) polartions. These branches are separated by the uncoupled phonon modes \u03bb\u00a0=\u00a01 and \u03bb\u00a0=\u00a02 (dashed lines). As l decreases, the LP branch shifts toward \u03bb\u00a0=\u00a01, the MP branch moves away from \u03bb\u00a0=\u00a01 and approaches \u03bb\u00a0=\u00a02, while the UP branch shifts away from \u03bb\u00a0=\u00a02. Two anticrossings are observed at l\u00a0=\u00a080\u2009\u03bcm and l\u00a0=\u00a050\u2009\u03bcm, corresponding to \u03c9c\u00a0\u2248\u00a0\u03c91 and \u03c9c\u00a0\u2248\u00a0\u03c92, respectively (Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>b). Due to the larger oscillator strength of the \u03bb\u00a0=\u00a02 mode (Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>a), the second Rabi splitting at l\u00a0=\u00a050\u2009\u03bcm exceeds the first at l\u00a0=\u00a080\u2009\u03bcm.<\/p>\n<p>We carried out finite element simulations (COMSOL) to validate our experimental results, using conductivity values extracted from THz-TDS measurements (Supplementary Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>) as input parameters. The simulated transmission spectra (Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>d, colormap) closely match the experimental data, with black solid circles marking the resonance frequencies obtained from Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>c via Lorentzian fitting. Minor discrepancies in the UP frequencies are attributed to slight shifts in the bare cavity mode (dashed green line, Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>a) and additional coupling with a 3.8 THz phonon mode in the z-cut quartz substrate.<\/p>\n<p>We also investigated a 2D perovskite material composed of metal halide layers separated by organic molecules, which enhances stability compared to 3D perovskites<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" title=\"Smith, I. C., Hoke, E. T., Solis-Ibarra, D., McGehee, M. D. &amp; Karunadasa, H. I. A layered hybrid perovskite solar-cell absorber with enhanced moisture stability. Angew. Chem. Int. Ed. 53, 11232&#x2013;11235 (2014).\" href=\"#ref-CR40\" id=\"ref-link-section-d108692028e1981\">40<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" title=\"Tsai, H. et al. High-efficiency two-dimensional Ruddlesden-Popper perovskite solar cells. Nature 536, 312&#x2013;316 (2016).\" href=\"#ref-CR41\" id=\"ref-link-section-d108692028e1981_1\">41<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 42\" title=\"Sidhik, S. et al. Two-dimensional perovskite templates for durable, efficient formamidinium perovskite solar cells. Science 384, 1227&#x2013;1235 (2024).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR42\" id=\"ref-link-section-d108692028e1984\" rel=\"nofollow noopener\" target=\"_blank\">42<\/a> and holds promise for solar cell applications. Unlike 3D MAPbI3 (Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>a), the presence of BA cations (CH3(CH2)3NH3) reduces the number of Pb-I bonds per unit volume, weakening the phonon mode oscillator strength. The layered structure, (BA)2(MA)n\u22121PbnI3n+1 (with n\u00a0=\u00a02)<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 41\" title=\"Tsai, H. et al. High-efficiency two-dimensional Ruddlesden-Popper perovskite solar cells. Nature 536, 312&#x2013;316 (2016).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR41\" id=\"ref-link-section-d108692028e2023\" rel=\"nofollow noopener\" target=\"_blank\">41<\/a>, is shown in Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>b. Here, n denotes the number of PbI6 octahedral layers between the BA spacer layers. The phonon modes \u03bb\u00a0=\u00a01 and \u03bb\u00a0=\u00a02 are slightly blueshifted compared to MAPbI3, with dips in the transmittance of a bare (BA)2MAPb2I7 200-nm-thick film at \u03c91\/(2\u03c0)\u00a0=\u00a01.09 THz and \u03c92\/(2\u03c0)\u00a0=\u00a02 THz, respectively (Supplementary Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>). The transmission spectra of 2D perovskites embedded in nanoslot resonators resemble those of their 3D counterparts, with a larger Rabi splitting for \u03bb\u00a0=\u00a02 due to its higher oscillator strength.<\/p>\n<p>Fig. 3: Phonon-polariton properties in perovskite\u2013nanoslot hybrid systems.<a class=\"c-article-section__figure-link\" data-test=\"img-link\" data-track=\"click\" data-track-label=\"image\" data-track-action=\"view figure\" href=\"https:\/\/www.nature.com\/articles\/s41467-025-63810-7\/figures\/3\" rel=\"nofollow noopener\" target=\"_blank\"><img decoding=\"async\" aria-describedby=\"Fig3\" src=\"https:\/\/www.newsbeep.com\/ca\/wp-content\/uploads\/2025\/10\/41467_2025_63810_Fig3_HTML.png\" alt=\"figure 3\" loading=\"lazy\" width=\"685\" height=\"576\"\/><\/a><\/p>\n<p>Top: MAPbI3 films (3D perovskite). Bottom: (BA)2MAPb2I7 (2D perovskite) films. a, b Crystal structures of MAPbI3 and (BA)2MAPb2I7. BA: \\({{{{\\rm{CH}}}}}_{3}{({{{{\\rm{CH}}}}}_{2})}_{3}{{{{\\rm{NH}}}}}_{3}^{+}\\), MA: \\({{{{\\rm{CH}}}}}_{3}{{{{\\rm{NH}}}}}_{3}^{+}\\). c, f Polariton dispersion as a function of cavity frequency; UP upper polariton, MP middle polariton, LP lower polariton. Solid circles: Peak frequencies extracted from the experimental transmission spectra. Solid lines: Fit of the extracted peak frequencies using the microscopic Hopfield model. The dashed lines indicate the \u03bb\u00a0=\u00a01 and \u03bb\u00a0=\u00a02 phonon modes and the cavity resonance. The two polariton gaps (see text) are denoted as \u03941 and \u03942. d, g Phonon Hopfield coefficients (H.C.) of the LP as a function of cavity frequency, showing a divergence in the low cavity frequency limit. e, h Theoretical predictions: Equal-time second-order phonon\u2013phonon correlation functions \\({g}_{\\lambda,{\\lambda }^{{\\prime} }}^{(2)}(\\tau=0)\\) for a polariton thermal state at room temperature as a function of cavity frequency. The inset in (e) shows \\({g}_{\\lambda,{\\lambda }^{{\\prime} }}^{(2)}(0)\\) as a function of temperature T for a cavity frequency of 0.1 THz.<\/p>\n<p>While classical electrodynamics simulations accurately reproduce the transmission spectra, we now adopt a complementary approach by utilizing a multimode Hopfield model<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 43\" title=\"Hopfield, J. J. Theory of the contribution of excitons to the complex dielectric constant of crystals. Phys. Rev. 112, 1555&#x2013;1567 (1958).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR43\" id=\"ref-link-section-d108692028e2430\" rel=\"nofollow noopener\" target=\"_blank\">43<\/a> to gain a deeper understanding of the ultrastrong light\u2013matter coupling in our system and investigate its potential implications. The microscopic Hamiltonian is given by (see \u201cMethods\u201d)<\/p>\n<p>$$\\hat{H}=\t \\hslash {\\omega }_{{{{\\rm{c}}}}}{\\hat{a}}^{{{\\dagger}} }\\hat{a}+\\sum\\limits_{\\lambda }\\hslash {\\omega }_{\\lambda }{\\hat{b}}_{\\lambda }^{{{\\dagger}} }{\\hat{b}}_{\\lambda }-i\\sum\\limits_{\\lambda }\\hslash {g}_{\\lambda }\\left({\\hat{b}}_{\\lambda }^{{{\\dagger}} }-{\\hat{b}}_{\\lambda }\\right)\\left(\\hat{a}+{\\hat{a}}^{{{\\dagger}} }\\right) \\\\ \t+\\sum\\limits_{\\lambda }\\frac{\\hslash {g}_{\\lambda }^{2}}{{\\omega }_{\\lambda }}{\\left(\\hat{a}+{\\hat{a}}^{{{\\dagger}} }\\right)}^{2},$$<\/p>\n<p>\n                    (1)\n                <\/p>\n<p>where \\({\\hat{a}}^{{{\\dagger}} }\\) (\\(\\hat{a}\\)) represents the creation (annihilation) operator of a cavity photon, while \\({\\hat{b}}_{\\lambda }^{{{\\dagger}} }\\) (\\({\\hat{b}}_{\\lambda }\\)) denotes the creation (annihilation) operator of a phonon in the mode \u03bb. The first two terms correspond to the bare photon and phonon Hamiltonians, respectively. The third term describes the light\u2013matter interaction, with a coupling strength given by \\({g}_{\\lambda }=\\frac{{\\nu }_{\\lambda }}{2}\\sqrt{\\frac{{\\omega }_{\\lambda }}{{\\omega }_{{{{\\rm{c}}}}}}}\\), which is proportional to the effective ion plasma frequency \u03bd\u03bb. The fourth term, known as the A2-term, induces a blueshift in the cavity mode frequency. The effective ion plasma frequency is determined by the effective charges associated with Pb2+ and I\u2212 ions; see \u201cMethods\u201d and Supplementary Note\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a> for details.<\/p>\n<p>The eigenfrequencies and eigenvectors of the Hamiltonian Eq. (<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"equation anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Equ1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>) are obtained via the Hopfield transformation: \\({\\hat{p}}_{\\alpha }={\\sum }_{\\lambda }{X}_{\\lambda,\\alpha }{\\hat{b}}_{\\lambda }+{\\sum }_{\\lambda }{\\widetilde{X}}_{\\lambda,\\alpha }{\\hat{b}}_{\\lambda }^{{{\\dagger}} }+{Y}_{\\alpha }\\hat{a}+{\\widetilde{Y}}_{\\alpha }{\\hat{a}}^{{{\\dagger}} }\\), where \\({\\hat{p}}_{\\alpha }\\) is the annihilation operator of a polariton in the mode \u03b1\u00a0= LP, MP, UP, with frequency \u03c9\u03b1. Up to a constant term, Eq. (<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"equation anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Equ1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>) can then be expressed in its diagonal form as \\(\\hat{H}={\\sum }_{\\alpha }\\hslash {\\omega }_{\\alpha }{\\hat{p}}_{\\alpha }^{{{\\dagger}} }{\\hat{p}}_{\\alpha }\\). The system enters the USC regime when the normalized coupling strength at resonance satisfies g\u03bb\/\u03c9\u03bb\u00a0=\u00a0\u03bd\u03bb\/2\u03c9\u03bb \u2273 0.1. In this regime, the counter-rotating terms \\(\\propto {\\hat{b}}_{\\lambda }\\hat{a},{\\hat{b}}_{\\lambda }^{{{\\dagger}} }{\\hat{a}}^{{{\\dagger}} }\\) in the Hamiltonian Eq. (<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"equation anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Equ1\" rel=\"nofollow noopener\" target=\"_blank\">1<\/a>), along with the anomalous Hopfield coefficients \\({\\widetilde{Y}}_{\\alpha }\\) and \\({\\widetilde{X}}_{\\lambda,\\alpha }\\), play a significant role.<\/p>\n<p>Figure\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>c presents the polariton dispersion for the MAPbI3\u2013nanoslots system. The coupling strengths g\u03bb are extracted by fitting the peak frequencies (solid circles) of the transmission spectra to the calculated eigenfrequencies \u03c9\u03b1 (solid lines). When the nanoslot resonator is resonant with the phonon modes \u03bb\u00a0=\u00a01 and \u03bb\u00a0=\u00a02, we obtain normalized coupling strengths of g1\/\u03c91\u00a0=\u00a00.28 (\u03c9c\u00a0=\u00a0\u03c91) and g2\/\u03c92\u00a0=\u00a00.3 (\u03c9c\u00a0=\u00a0\u03c92), respectively. These values confirm that both phonon modes are in the USC regime with the nanoslot resonator. The corresponding Rabi splittings at the two resonances are 0.45 THz and 1.13 THz. Notably, while the Rabi splitting equals exactly 2g for a single matter and cavity mode in the strong coupling regime, this relation breaks down in the USC regime due to counter-rotating terms. In our case, the inclusion of two phonon modes leads to further deviations from the 2g value. Importantly, the polariton dispersion should be understood as the result of the simultaneous coupling of both phonon modes to the cavity mode, with all three degrees of freedom treated on equal footing. This becomes evident when examining the contribution of the two phonon modes to the MP mode at around the resonance between the \u03bb\u00a0=\u00a01 phonon and the cavity mode. As shown in Supplementary Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">4b<\/a>, the contribution \\({W}_{\\lambda }^{{{{\\rm{MP}}}}}=| {X}_{\\lambda,{{{\\rm{MP}}}}}{| }^{2}-| {\\widetilde{X}}_{\\lambda,{{{\\rm{MP}}}}}{| }^{2}\\) of the two phonon modes (\u03bb\u00a0=\u00a01,\u00a02) to the MP mode is indeed of comparable magnitude, indicating that the MP branch involves significant hybridization with both phonon modes.<\/p>\n<p>In the USC regime, distinctive features appear not only near resonance, but also when the resonator frequency is much lower than the phonon frequencies, \u03c9c \u226a \u03c9\u03bb. Unlike in the strong coupling regime, the polariton modes do not converge to the uncoupled mode frequencies when \u03c9c \u226a \u03c9\u03bb. This behavior defines the so-called polariton gaps<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 19\" title=\"Forn-D&#xED;az, P., Lamata, L., Rico, E., Kono, J. &amp; Solano, E. Ultrastrong coupling regimes of light-matter interaction. Rev. Mod. Phys. 91, 025005 (2019).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR19\" id=\"ref-link-section-d108692028e3988\" rel=\"nofollow noopener\" target=\"_blank\">19<\/a>,<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 44\" title=\"Maisen, C. et al. Ultrastrong coupling in the near field of complementary split-ring resonators. Phys. Rev. B 90, 205309 (2014).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR44\" id=\"ref-link-section-d108692028e3991\" rel=\"nofollow noopener\" target=\"_blank\">44<\/a>, given by \\({\\Delta }_{1}={\\lim }_{{\\omega }_{{{{\\rm{c}}}}}\\to 0}{\\omega }_{{{{\\rm{MP}}}}}-{\\omega }_{1}\\) and \\({\\Delta }_{2}={\\lim }_{{\\omega }_{{{{\\rm{c}}}}}\\to 0}{\\omega }_{{{{\\rm{UP}}}}}-{\\omega }_{2}\\), as shown in Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>c. As detailed in Supplementary Note\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>, the frequencies of the MP and UP modes, \u03c9MP and \u03c9UP, asymptotically approach \\({\\widetilde{\\omega }}_{1}=\\sqrt{{\\omega }_{1}^{2}+{\\nu }_{1}^{2}}\\) and \\({\\widetilde{\\omega }}_{2}=\\sqrt{{\\omega }_{2}^{2}+{\\nu }_{2}^{2}}\\), respectively, in the low-resonator frequency limit \u03c9c\u00a0\u2192\u00a00.<\/p>\n<p>This unconventional behavior is linked to strong light\u2013matter hybridization, which persists even in this far-detuned, low-resonator-frequency regime. This is reflected in the divergence of the light\u2013matter coupling strength, \\({g}_{\\lambda }\\propto \\sqrt{1\/{\\omega }_{{{{\\rm{c}}}}}}\\), and the A2-term, which scales as \\({g}_{\\lambda }^{2}\\), as \u03c9c\u00a0\u2192\u00a00. In this regime, the MP (UP) mode is mainly a hybrid of the phonon mode \u03bb\u00a0=\u00a01 (\u03bb\u00a0=\u00a02) and cavity photons. The corresponding normal (Y\u03b1) and anomalous (\\({\\widetilde{Y}}_{\\alpha }\\)) Hopfield coefficients become large and comparable, scaling as \\({Y}_{{{{\\rm{MP}}}}} \\sim {\\widetilde{Y}}_{{{{\\rm{MP}}}}} \\sim {\\nu }_{1}\/\\sqrt{{\\omega }_{{{{\\rm{c}}}}}{\\widetilde{\\omega }}_{1}}\\) and \\({Y}_{{{{\\rm{UP}}}}} \\sim {\\widetilde{Y}}_{{{{\\rm{UP}}}}} \\sim {\\nu }_{2}\/\\sqrt{{\\omega }_{{{{\\rm{c}}}}}{\\widetilde{\\omega }}_{2}}\\). In contrast, the LP mode mixes the cavity field with both phonon modes. The phonon contributions to this polariton, quantified by the coefficients X\u03bb,LP and \\({\\widetilde{X}}_{\\lambda,{{{\\rm{LP}}}}}\\), also grow large and comparable, with \\({X}_{\\lambda,{{{\\rm{LP}}}}} \\sim {\\widetilde{X}}_{\\lambda,{{{\\rm{LP}}}}} \\sim {\\nu }_{\\lambda }\/\\sqrt{{\\omega }_{{{{\\rm{c}}}}}{\\omega }_{\\lambda }}\\). These coefficients are shown in Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>d, while the other Hopfield coefficients are provided in Supplementary Figs.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a> and <a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">5<\/a>.<\/p>\n<p>Due to the large anomalous Hopfield coefficients, the polaritonic ground state \\(\\left\\vert G\\right\\rangle\\), defined by \\({\\prod }_{\\alpha }{\\hat{p}}_{\\alpha }\\left\\vert G\\right\\rangle=0\\), takes the form of a multimode squeezed vacuum in the low resonator frequency regime. This state contains correlated photon pairs, contributed by the MP and UP, as well as intermode and intramode phonon pairs originating from the LP. This multimode squeezed vacuum exhibits strong entanglement between the two phonon modes, as discussed below.<\/p>\n<p>It is important to highlight that while both the normal and anomalous Hopfield coefficients diverge in the limit \u03c9c\u00a0\u2192\u00a00, the total phonon and photon weights remain finite due to the normalization of the Hopfield coefficients (see Supplementary Figs.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">4<\/a> and <a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">6<\/a>). Moreover, we stress that the low-resonator-frequency regime (long cavity) does not imply the absence of a cavity, as its transverse confinement remains deeply subwavelength.<\/p>\n<p>A distinctive feature of the multimode USC regime is the presence of anomalous correlations between the phonon modes. By inverting the Hopfield transformation, one obtains the correlation functions:<\/p>\n<p>$$\\langle {\\hat{b}}_{\\lambda }^{{{\\dagger}} }{\\hat{b}}_{{\\lambda }^{{\\prime} }}\\rangle=\\sum\\limits_{\\alpha }{\\left({\\widetilde{X}}_{\\lambda }^{\\alpha }\\right)}^{*}{\\widetilde{X}}_{{\\lambda }^{{\\prime} }}^{\\alpha }(1+{n}_{\\alpha })+\\sum\\limits_{\\alpha }{X}_{\\lambda }^{\\alpha }{\\left({X}_{{\\lambda }^{{\\prime} }}^{\\alpha }\\right)}^{*}{n}_{\\alpha },$$<\/p>\n<p>\n                    (2)\n                <\/p>\n<p>$$\\langle {\\hat{b}}_{\\lambda }{\\hat{b}}_{{\\lambda }^{{\\prime} }}\\rangle=-\\sum\\limits_{\\alpha }{\\left({X}_{\\lambda }^{\\alpha }\\right)}^{*}{\\widetilde{X}}_{{\\lambda }^{{\\prime} }}^{\\alpha }(1+{n}_{\\alpha })-\\sum\\limits_{\\alpha }{\\left({X}_{{\\lambda }^{{\\prime} }}^{\\alpha }\\right)}^{*}{\\widetilde{X}}_{\\lambda }^{\\alpha }{n}_{\\alpha }.$$<\/p>\n<p>\n                    (3)\n                <\/p>\n<p>Here, \\({n}_{\\alpha }=\\langle {\\hat{p}}_{\\alpha }^{{{\\dagger}} }{\\hat{p}}_{\\alpha }\\rangle\\) represents the population in the polariton mode \u03b1. In the polaritonic ground state (n\u03b1\u00a0=\u00a00), Eqs. (<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"equation anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Equ2\" rel=\"nofollow noopener\" target=\"_blank\">2<\/a>) and (<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"equation anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Equ3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>) show that such correlations arise only when the anomalous Hopfield coefficients \\({\\widetilde{X}}_{\\lambda }^{\\alpha }\\) are nonzero. Moreover, these correlations are further enhanced in excited polariton states where n\u03b1\u00a0\u2260\u00a00. To explore the impact of multimode USC on correlated phonon emission, we consider the second-order correlation function<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 45\" title=\"Humphries, B. S., Green, D., Borgh, M. O. &amp; Jones, G. A. Phonon signatures in photon correlations. Phys. Rev. Lett. 131, 143601 (2023).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR45\" id=\"ref-link-section-d108692028e5796\" rel=\"nofollow noopener\" target=\"_blank\">45<\/a>, which quantifies the joint probability of a phonon being emitted in the mode \\({\\lambda }^{{\\prime} }\\) at time t\u00a0+\u00a0\u03c4 given that a phonon was emitted in the mode \u03bb at time t:<\/p>\n<p>$${g}_{\\lambda,{\\lambda }^{{\\prime} }}^{(2)}(\\tau )=\\frac{\\langle {\\hat{b}}_{{\\lambda }^{{\\prime} }}(t+\\tau ){\\hat{b}}_{\\lambda }(t){\\hat{b}}_{\\lambda }^{{{\\dagger}} }(t){\\hat{b}}_{{\\lambda }^{{\\prime} }}^{{{\\dagger}} }(t+\\tau )\\rangle }{\\langle {\\hat{b}}_{\\lambda }(t){\\hat{b}}_{\\lambda }^{{{\\dagger}} }(t)\\rangle \\langle {\\hat{b}}_{{\\lambda }^{{\\prime} }}(t+\\tau ){\\hat{b}}_{{\\lambda }^{{\\prime} }}^{{{\\dagger}} }(t+\\tau )\\rangle }.$$<\/p>\n<p>\n                    (4)\n                <\/p>\n<p>Although classical wave-based methods could, in principle, be used to study intensity correlations, such calculations are technically challenging and non-trivial to implement. For this reason, we focus in this work on quantum predictions for the second-order correlation functions. Assuming a thermal polariton state at temperature T, with \\({n}_{\\alpha }={\\left({e}^{\\hslash {\\omega }_{\\alpha }\/{k}_{{{{\\rm{B}}}}}T}-1\\right)}^{-1}\\) and kB the Boltzmann constant, the equal-time intramode (\\(\\lambda={\\lambda }^{{\\prime} }\\)) and intermode (\\(\\lambda \\, \\ne \\, {\\lambda }^{{\\prime} }\\)) correlation functions are given by<\/p>\n<p>$${g}_{\\lambda,\\lambda }^{(2)}(0)=2+\\frac{\\langle {\\hat{b}}_{\\lambda }{\\hat{b}}_{\\lambda }\\rangle \\langle {\\hat{b}}_{\\lambda }^{{{\\dagger}} }{\\hat{b}}_{\\lambda }^{{{\\dagger}} }\\rangle }{{\\langle {\\hat{b}}_{\\lambda }{\\hat{b}}_{\\lambda }^{{{\\dagger}} }\\rangle }^{2}},$$<\/p>\n<p>\n                    (5)\n                <\/p>\n<p>$${g}_{\\lambda,{\\lambda }^{{\\prime} }}^{(2)}(0)=1+\\frac{\\langle {\\hat{b}}_{\\lambda }{\\hat{b}}_{{\\lambda }^{{\\prime} }}^{{{\\dagger}} }\\rangle \\langle {\\hat{b}}_{{\\lambda }^{{\\prime} }}{\\hat{b}}_{\\lambda }^{{{\\dagger}} }\\rangle }{\\langle {\\hat{b}}_{\\lambda }{\\hat{b}}_{\\lambda }^{{{\\dagger}} }\\rangle \\langle {\\hat{b}}_{{\\lambda }^{{\\prime} }}{\\hat{b}}_{{\\lambda }^{{\\prime} }}^{{{\\dagger}} }\\rangle }+\\frac{\\langle {\\hat{b}}_{\\lambda }{\\hat{b}}_{{\\lambda }^{{\\prime} }}\\rangle \\langle {\\hat{b}}_{{\\lambda }^{{\\prime} }}^{{{\\dagger}} }{\\hat{b}}_{\\lambda }^{{{\\dagger}} }\\rangle }{\\langle {\\hat{b}}_{\\lambda }{\\hat{b}}_{\\lambda }^{{{\\dagger}} }\\rangle \\langle {\\hat{b}}_{{\\lambda }^{{\\prime} }}{\\hat{b}}_{{\\lambda }^{{\\prime} }}^{{{\\dagger}} }\\rangle },$$<\/p>\n<p>\n                    (6)\n                <\/p>\n<p>respectively. For vanishing anomalous Hopfield coefficients (\\({\\widetilde{X}}_{\\lambda }^{\\alpha }=0\\,\\forall \\lambda\\)) or in the absence of phonon\u2013photon coupling (\u03bd\u03bb\u00a0=\u00a00), Eq. (<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"equation anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Equ5\" rel=\"nofollow noopener\" target=\"_blank\">5<\/a>) simplifies to \\({g}_{\\lambda,\\lambda }^{(2)}(0)=2\\), which corresponds to intramode phonon bunching-a hallmark of thermal states. In contrast, the intermode correlation function satisfies \\({g}_{\\lambda,{\\lambda }^{{\\prime} }}^{(2)}(0)=1\\) for \\(\\lambda \\, \\ne \\, {\\lambda }^{{\\prime} }\\), indicating that intermode phonon emission remains uncorrelated and follows Poissonian statistics<a data-track=\"click\" data-track-action=\"reference anchor\" data-track-label=\"link\" data-test=\"citation-ref\" aria-label=\"Reference 46\" title=\"Gardiner, C. W. &amp; Zoller, P. Quantum Noise 2nd edn (Springer, 2000).\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#ref-CR46\" id=\"ref-link-section-d108692028e7650\" rel=\"nofollow noopener\" target=\"_blank\">46<\/a>.<\/p>\n<p>In the multimode USC regime, we predict a significant modification of equal-time phonon-phonon second-order correlations. As shown in Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>e, the various contributions \\({g}_{\\lambda,{\\lambda }^{{\\prime} }}^{(2)}(0)\\) to a value of 3 in the limit of a vanishing resonator frequency (\u03c9c\u00a0\u2192\u00a00). As \u03c9c increases, \\({g}_{\\lambda,{\\lambda }^{{\\prime} }}^{(2)}(0)\\) decreases monotonically, approaching 2 for intramode correlations (\\(\\lambda={\\lambda }^{{\\prime} }\\)) and 1 for intermode correlations (\\(\\lambda \\ne {\\lambda }^{{\\prime} }\\)). These limiting values correspond to the correlations expected for bare phonons, which are recovered in the high resonator frequency regime (\u03c9c \u226b \u03c9\u03bb), where the LP and MP asymptotically approach the uncoupled phonon frequencies \u03c91 and \u03c92, respectively.<\/p>\n<p>For a detuned cavity with \u03c9c\/(2\u03c0)\u00a0=\u00a00.1 THz at room temperature (T\u00a0=\u00a0300 K), our theoretical model predicts \\({g}_{1,1}^{(2)}(0)\\approx 2.86\\), \\({g}_{2,2}^{(2)}(0)\\approx 2.96\\), and \\({g}_{1,2}^{(2)}(0)\\approx 2.82\\). These results indicate that multimode USC should lead to strong phonon bunching in both intramode and intermode correlations. This effect primarily arises from the LP, which exhibits large normal and anomalous phonon Hopfield coefficients (\\({X}_{\\lambda }^{\\alpha },{\\widetilde{X}}_{\\lambda }^{\\alpha }\\)), as discussed earlier, along with a significant population in the low resonator frequency regime (nLP\u00a0\u2248\u00a080 for \u03c9c\/(2\u03c0)\u00a0=\u00a00.1 THz and T\u00a0=\u00a0300 K). The inset of Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>e illustrates the temperature dependence of the calculated second-order phonon correlations, showing that at T\u00a0=\u00a00 K, intramode and intermode correlations are enhanced by approximately 10% and 40%, respectively, compared to the bare phonon case. Notably, at room temperature, \\({g}_{\\lambda,{\\lambda }^{{\\prime} }}^{(2)}(0)\\) remains in the saturation regime.<\/p>\n<p>Figure\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>f presents the extracted peak frequencies for the 2D perovskite (BA)2MAPb2I7\u2013nanoslots system, alongside theoretical predictions (solid lines). In this case, the \u03bb\u00a0=\u00a01 mode exhibits a very small polaritonic gap, which is consistent with the normalized coupling strength \\({g}_{1}^{{\\prime} }\/{\\omega }_{1}=0.13\\) extracted from the fit. This value suggests that \u03bb\u00a0=\u00a01 is on the verge of the USC regime, leading to reduced Hopfield coefficients X1,LP and \\({\\widetilde{X}}_{{{{\\rm{1,LP}}}}}\\) compared to the MAPbI3\u2013nanoslots system (see Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>g). Conversely, the polaritonic gap of the \u03bb\u00a0=\u00a02 mode remains similar to that observed in the MAPbI3\u2013nanoslots system, consistent with the large coupling ratio \\({g}_{2}^{{\\prime} }\/{\\omega }_{2}=0.23\\) extracted from the fit.<\/p>\n<p>At \u03c9c\/(2\u03c0)\u00a0=\u00a00.1 THz and room temperature, the calculated phonon-phonon correlations for \\(\\lambda={\\lambda }^{{\\prime} }=1\\) and \\(\\lambda=1,{\\lambda }^{{\\prime} }=2\\) are significantly lower than in the MAPbI3-nanoslots system (\\({g}_{1,1}^{(2)}(0)\\approx 2.61\\), \\({g}_{1,2}^{(2)}(0)\\approx 2.52\\)), in line with the weaker coupling strength of \u03bb\u00a0=\u00a01. However, \\({g}_{2,2}^{(2)}(0)\\approx 2.94\\) remains nearly unchanged compared to the 3D perovskite system, as shown in Fig.\u00a0<a data-track=\"click\" data-track-label=\"link\" data-track-action=\"figure anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#Fig3\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a>h.<\/p>\n<p>Using a perturbative expansion valid for \u03c9c\/\u03c9\u03bb \u226a 1 and \u03bd\u03bb\/\u03c9\u03bb \u226a 1, we show in Supplementary Note <a data-track=\"click\" data-track-label=\"link\" data-track-action=\"supplementary material anchor\" href=\"http:\/\/www.nature.com\/articles\/s41467-025-63810-7#MOESM1\" rel=\"nofollow noopener\" target=\"_blank\">3<\/a> that the second-order correlation functions can be approximated as<\/p>\n<p>$${g}_{1,1}^{(2)}(0)\\approx 2+{\\left(\\frac{{g}_{1}}{{\\omega }_{1}}\\right)}^{4}{\\left(\\frac{1+2{n}_{{{{\\rm{LP}}}}}}{1+{n}_{{{{\\rm{MP}}}}}}\\right)}^{2}$$<\/p>\n<p>\n                    (7a)\n                <\/p>\n<p>$${g}_{2,2}^{(2)}(0)\\approx 2+{\\left(\\frac{{g}_{2}}{{\\omega }_{2}}\\right)}^{4}{\\left(\\frac{1+2{n}_{{{{\\rm{LP}}}}}}{1+{n}_{{{{\\rm{UP}}}}}}\\right)}^{2}$$<\/p>\n<p>\n                    (7b)\n                <\/p>\n<p>$${g}_{1,2}^{(2)}(0)\\approx 1+2{\\left(\\frac{{g}_{1}}{{\\omega }_{1}}\\right)}^{2}{\\left(\\frac{{g}_{2}}{{\\omega }_{2}}\\right)}^{2}\\frac{{(1+2{n}_{{{{\\rm{LP}}}}})}^{2}}{(1+{n}_{{{{\\rm{MP}}}}})(1+{n}_{{{{\\rm{UP}}}}})}.$$<\/p>\n<p>\n                    (7c)\n                <\/p>\n<p>These results show that the intramode correlation functions are primarily controlled by the standard USC figure of merit, g\u03bb\/\u03c9\u03bb. In contrast, intermode correlations are governed by the product g1g2\/\u03c91\u03c92, which becomes an important figure of merit for multimode USC. For instance, we find g1g2\/\u03c91\u03c92\u00a0=\u00a00.084 in the 3D perovskite-nanoslot system and g1g2\/\u03c91\u03c92\u00a0=\u00a00.03 in the 2D system. The specific form g1g2\/\u03c91\u03c92 suggests that intermode correlations arise from the effective coupling between phonons mediated by the far-detuned cavity, where \u03c9c \u226a \u03c9\u03bb.<\/p>\n","protected":false},"excerpt":{"rendered":"We fabricated an array of nanoslots (w\u00a0=\u00a0950 nm) on quartz substrates with seven different lengths (l\u00a0= 30, 40,&hellip;\n","protected":false},"author":2,"featured_media":183534,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[24],"tags":[49,48,1099,92140,1100,314,25338,37833,66],"class_list":{"0":"post-183533","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-physics","8":"tag-ca","9":"tag-canada","10":"tag-humanities-and-social-sciences","11":"tag-materials-for-energy-and-catalysis","12":"tag-multidisciplinary","13":"tag-physics","14":"tag-polaritons","15":"tag-quantum-optics","16":"tag-science"},"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts\/183533","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/comments?post=183533"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts\/183533\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/media\/183534"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/media?parent=183533"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/categories?post=183533"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/tags?post=183533"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}