Intensity distribution in random lasers: comparison between a stochastic differential model of interacting modes and random phase sum-based models

Gonzalez, Ivan R. R.

Abstract

Random lasers (RLs) are a special type of laser with a feedback mechanism arising from the random photon scattering in a disordered medium. Their emitted intensity is inherently stochastic. Here we compare results for the intensity distribution from two classes of models. The first concerns electromagnetic wave scattering in a random medium with field amplitudes and phases as independent random or locally correlated variables [random phase sum (RPS)-based models]. In the second, stochastic differential equations describe the mode dynamics in a random medium. Whereas RPS-based models imply Rayleigh, exponential, and K distributions, in the second class we extend to any degree f of optical nonlinearity previous results valid only up to the sixth order, introducing a novel family of intensity distributions, the generalized Izrailev distributions of order f . Model predictions are compared to very large experimental datasets from two quite distinct RLs: a Nd3+-doped nanopowder and a mixture of colloids containing TiO2 particles and a dye solution. While RPS models do not provide good data fits, excellent agreement is found with the stochastic differential model, indicating that it properly captures the influence of high-order nonlinearities on the intensity distribution of RLs.

Más información

Título según WOS: Intensity distribution in random lasers: comparison between a stochastic differential model of interacting modes and random phase sum-based models
Título según SCOPUS: Intensity distribution in random lasers: Comparison between a stochastic differential model of interacting modes and random phase sum-based models
Título de la Revista: Journal of the Optical Society of America B: Optical Physics
Volumen: 38
Número: 8
Editorial: Optica Publishing Group (formerly OSA)
Fecha de publicación: 2021
Página final: 2398
Idioma: English
DOI:

10.1364/JOSAB.433317

Notas: ISI, SCOPUS