Evidence map›Paper›PMID 41787936›Full record

ArticleAdvanced science (Weinheim, Baden-Wurttemberg, Germany)2026

Photon-Sphere Modes in Curved Optical Microcavities: A Black-Hole Analogue Laser.

Chenni Xu, Aswathy Sundaresan, Nazire-Begüm Kazkal, Clement Lafargue, Lior Zarfaty, Li-Gang Wang, Ofek Birnholtz, Dominique Decanini, Melanie Lebental, Patrick Sebbah

Abstract read
In one paragraph

Article in Advanced science (Weinheim, Baden-Wurttemberg, Germany), 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 1 paper.

0numbers the graph read from it
0cells of the map it votes in
1citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

1 citing paper in PubMed.

  1. Photon-Sphere Modes in Curved Optical Microcavities: A Black-Hole Analogue Laser.Advanced science (Weinheim, Baden-Wurttemberg, Germany) · 2026
    Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

10 authors.

Chenni XuDepartment of Physics, The Jack and Pearl Resnick Institute for Advanced Technology, Bar-Ilan University, Ramat-Gan, Israel.
Aswathy SundaresanDepartment of Physics, The Jack and Pearl Resnick Institute for Advanced Technology, Bar-Ilan University, Ramat-Gan, Israel.
Nazire-Begüm KazkalUniversité Paris-Saclay, CNRS, Centre de Nanosciences et de Nanotechnologies, Palaiseau, France.
Clement LafargueLaboratoire Lumière, Matière et Interfaces (LuMIn) CNRS, ENS Paris-Saclay, Université Paris-Saclay, CentraleSupélec, Gif-sur-Yvette, France.
Lior ZarfatyDepartment of Physics, The Jack and Pearl Resnick Institute for Advanced Technology, Bar-Ilan University, Ramat-Gan, Israel.
Li-Gang WangSchool of Physics, Zhejiang University, Hangzhou, China.
Ofek BirnholtzDepartment of Physics, The Jack and Pearl Resnick Institute for Advanced Technology, Bar-Ilan University, Ramat-Gan, Israel.
Dominique DecaniniUniversité Paris-Saclay, CNRS, Centre de Nanosciences et de Nanotechnologies, Palaiseau, France.
Melanie LebentalUniversité Paris-Saclay, CNRS, Centre de Nanosciences et de Nanotechnologies, Palaiseau, France.
Patrick SebbahDepartment of Physics, The Jack and Pearl Resnick Institute for Advanced Technology, Bar-Ilan University, Ramat-Gan, Israel.ORCID https://orcid.org/0000-0001-8845-1073

Funding

Centre National de la Recherche Scientifique (CNRS)French RENATECH networkGeneral Council of EssonneIsrael Academy of Sciences and HumanitiesIsrael Science Foundation 1698/22Israel Science Foundation 1871/15Israel Science Foundation 2074/15Israel Science Foundation 2630/20Israel Science Foundation 3777/25United States - Israel Binational Science Foundation 2015694United States - Israel Binational Science Foundation 2020245United States - Israel Binational Science Foundation 2022158
6 · The paper itself

Abstract

The bell-like ringdown of the gravitational field in the final stage of massive black-hole mergers is now routinely detected on Earth by the latest generation of gravitational-wave detectors. Its spectrum is interpreted as a sum of damped sinusoidal vibrations of spacetime in the vicinity of the black hole. These so-called quasinormal modes are the subject of extensive current studies, yet their physical nature remains elusive. Here, we emulate in the laboratory genuine four-dimensional (3+1)D black-hole metrics using an effective (2+1)D optical metric defined on a two-dimensional curved surface that preserves the features of light-like geodesics. We analytically compute the quasinormal modes of the optical cavity and show that, in addition to conventional whispering-gallery modes (WGMs) supported near the cavity boundary, a new family of modes is confined around the photon sphere, the unstable region where spacetime curvature traps light in circular orbits. By 3D-printing non-Euclidean dye-doped microcavities, we demonstrate lasing in both WGMs and photon-sphere modes, with the latter exhibiting spatial profiles in close agreement with analytical predictions. These results place our system within the broader framework of analogue-gravity experiments, providing a complementary photonic platform to investigate black-hole photon-sphere physics under tabletop conditions and inspiring new approaches to microcavity photonics.

Indexed as

astrophysical phenomena emulationcurvature potential trappingcurved microlasersnon‐Euclidean photonicsquasinormal modes

Identifiers

PMID41787936
PMCPMC13185855

What OpenQuestion holds

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Registered trials

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.