{"title":"Transmission‐Mode Silicon‐Rich Nitride Mie‐Void Metasurfaces in the Visible","authors":"Oren Goldberg, Noa Mazurski, Uriel Levy","doi":"10.1002/lpor.72080","DOIUrl":"https://doi.org/10.1002/lpor.72080","url":null,"abstract":"Mie‐void metasurfaces have so far been developed mainly in reflection, where subwavelength voids embedded in high‐index media support localized resonances and spectrally selective optical responses. Here we introduce Mie‐void metasurfaces operating in transmission, implemented using the silicon‐rich nitride (SRN) platform for visible‐range operation. We show that this transition is not a simple change in geometry: placing the voids in a finite film on a substrate introduces slab‐guided and Fabry–Pérot‐like contributions that hybridize with the underlying Mie‐void response. Rigorous coupled‐wave analysis shows that the dominant spectral transformation arises from replacing the semi‐infinite host with a finite SRN film, while the substrate acts as a secondary perturbation. Thickness‐dependent dispersion maps reveal an avoided crossing between interacting modes, identifying film thickness as a clean parameter for tracking the coupled modal evolution. Experimentally, we demonstrate depth‐dependent transmission spectra in good agreement with simulation, and realize visible structural colors and spatially encoded transmitted‐light patterns within a single metasurface architecture. These results establish transmission‐mode Mie‐void metasurfaces as a viable inverse‐dielectric platform for transmissive spectral filtering, optical encoding, and display‐oriented photonic elements.","PeriodicalId":204,"journal":{"name":"Laser & Photonics Reviews","volume":"15 1","pages":""},"PeriodicalIF":11.0,"publicationDate":"2026-10-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149198998","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"General orbital perturbation theory in Schwarzschild space-time","authors":"Oleksii Yanchyshen,Eva Hackmann,Claus Lämmerzahl","doi":"10.1088/1361-6382/aeb5c4","DOIUrl":"https://doi.org/10.1088/1361-6382/aeb5c4","url":null,"abstract":"Abstract We derive general relativistic Gaussian equations for osculating elements for orbits under the influence of a perturbing force without any restrictions in an underlying Schwarzschild space-time. Such a formulation provides a way to describe the evolution of orbital parameters in strong gravity relativistic settings. As examples of external forces we considered Kerr and q-metric space-times generated forces, for which we solve equations for osculating elements in linear approximation. For the Kerr space-time in the post-Newtonian limit, our result reproduces the well-known Lense-Thirring precession of the longitude of the ascending node.","PeriodicalId":10282,"journal":{"name":"Classical and Quantum Gravity","volume":"32 1","pages":""},"PeriodicalIF":3.5,"publicationDate":"2026-10-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149209035","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Jossian A. García,Vicente Sierra,Claudia Moreno,Javier M. Antelis
{"title":"Conditional Derivative GANs for Parameter-Conditioned Synthesis of Gravitational Waves from Core-Collapse Supernovae","authors":"Jossian A. García,Vicente Sierra,Claudia Moreno,Javier M. Antelis","doi":"10.1088/1361-6382/aeb595","DOIUrl":"https://doi.org/10.1088/1361-6382/aeb595","url":null,"abstract":"Abstract Gravitational wave signals from core-collapse supernovae encode critical astrophysical information, including key astrophysical parameters such as the ratio of rotational kinetic to gravitational potential energy at bounce, pre-collapse differential rotation, and the nuclear equation of state. However, the limited number of observed core-collapse supernovae events makes it challenging to build robust data-driven models. The generation of synthetic gravitational wave signals from core-collapse supernovae can therefore provide a valuable tool for data augmentation in machine learning pipelines, particularly for the training and testing of detection and parameter estimation algorithms. Although recent efforts have explored the use of generative models to synthesize waveform-like data, existing approaches lack the ability to condition outputs on specific astrophysical parameters. To address this, we propose a model capable of generating gravitational wave signals conditioned on astrophysical parameters of core-collapse supernovae rotation. The proposed conditional derivative generative adversarial network is trained on the Richers et al. catalog, which contains 1,824 simulated time-series gravitational wave waveforms and their corresponding physical parameters. Quantitative evaluation using time-domain similarity and distributional metrics shows that the generated signals reproduce the key statistical and morphological features of the original dataset. This work introduces a conditional generative framework for rotating core-collapse supernovae gravitational wave signals, that enables fast, low-cost data augmentation and parameterized modeling, improving ML-based detection and parameter estimation.
","PeriodicalId":10282,"journal":{"name":"Classical and Quantum Gravity","volume":"10 1","pages":""},"PeriodicalIF":3.5,"publicationDate":"2026-10-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149209038","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
ACS PhotonicsPub Date : 2026-10-16DOI: 10.1021/acsphotonics.6c01318
Johannes Bürger,Erika Cortese,Simone Di Muzio,Daniele Sanvitto,Simone De Liberato,Dario Ballarini
{"title":"Exciton-Tunable\u0000Phase Control and Superstrong Coupling\u0000through Multimode Polariton Engineering in Planar Waveguides","authors":"Johannes Bürger,Erika Cortese,Simone Di Muzio,Daniele Sanvitto,Simone De Liberato,Dario Ballarini","doi":"10.1021/acsphotonics.6c01318","DOIUrl":"https://doi.org/10.1021/acsphotonics.6c01318","url":null,"abstract":"Abstract Strong light–matter coupling in optical waveguides provides a versatile platform for engineering hybrid polaritonic modes and their dispersion. Here, we investigate multimode exciton–photon coupling in visible semiconductor waveguides supporting several transverse electric modes. Using rigorous coupled-wave analysis combined with a coupled-oscillator model, we show that the photonic band structure can be engineered across a range of regimes, from conventional multimode strong coupling to the superstrong coupling regime, where the Rabi coupling becomes comparable to the spacing between adjacent photonic modes. In the latter regime, hybridization between orthogonal electromagnetic modes is enabled by restricting the active material to a subregion of the mode volume where the photonic modes exhibit strong mutual overlap. This breaking of the orthogonality leads to polaritonic branches whose composition can be tuned among several photonic modes and the exciton. We demonstrate that small shifts of the exciton resonance produce pronounced changes in the propagation constants of different polariton branches, enabling exciton-controlled phase modulation through modal interference and, in the superstrong coupling regime, direct modal switching across a continuous S-shaped dispersion. The resulting figures of merit predict π phase shifts for exciton energy shifts of only a few meV over propagation lengths of tens of micrometers, while larger shifts are still required for mode switching. These results establish multimode waveguide polaritons as a versatile platform spanning multiple coupling regimes, for compact phase and intensity control in integrated photonic architectures.","PeriodicalId":23,"journal":{"name":"ACS Photonics","volume":"482 1","pages":""},"PeriodicalIF":7.0,"publicationDate":"2026-10-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149210032","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}