PreprintCC BY-NC-ND 4.0arXiv
Radiation-pressure induced chaos in multipendular Fabry-Perot resonators
Abstract
The occurrence of chaos in multipendular FP resonators (without light propagation delay) is illustrated. The probability of evolving a chaotic solution in a given time, starting from initial conditions contained in a neighbourhood of a stable equilibrium point, is estimated, and its dependence on the most relevant system parameters is investigated. The possible relevance of these results for interferometric gravitational wave antennas is discussed.
Related
- Multimode oscillation and its route to chaos in transverse-mode-coupled optomechanical resonators
- Induced Directional Switching of Platicon Microcombs in Photonic Crystal Ring Resonators
- Compact laser power measurement at tens of watts via amplified radiation pressure
- Chaos-Modulated Photothermal Fingerprinting of Pb(NO₃)₂-Induced Perturbations in Wastewater Using Phase-Space and Fractional Thermal-Memory Signatures
- Multimode radiation pressure actuation of a mechanical resonator using a spatial mode sorter
BibTeX
@misc{pierro2026radiationpressure,
title = {{Radiation-pressure induced chaos in multipendular Fabry-Perot resonators}},
author = {V. Pierro and I. M. Pinto},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.25872},
eprint = {2609.25872},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.25872},
note = {CC BY-NC-ND 4.0},
}
RIS
TY - UNPB
TI - Radiation-pressure induced chaos in multipendular Fabry-Perot resonators
AU - V. Pierro
AU - I. M. Pinto
PY - 2026
DA - 2026/09/22
PB - arXiv
DO - 10.48550/arxiv.2609.25872
UR - https://arxiv.org/abs/2609.25872
AB - The occurrence of chaos in multipendular FP resonators (without light propagation delay) is illustrated. The probability of evolving a chaotic solution in a given time, starting from initial conditions contained in a neighbourhood of a stable equilibrium point, is estimated, and its dependence on the most relevant system parameters is investigated. The possible relevance of these results for interferometric gravitational wave antennas is discussed.
ER -