What’s new?

Metagratings and more general metasurfaces are starting to draw ever more attention in different applications. They are known for maintaining a high diffraction efficiency in non-paraxial situations. Polarization-insensitive designs are possible with an appropriate selection of the types of nanopillars as the unit cells for the metagrating. Following the work of P. Lalanne et al. – pioneers in the field of metasurface research – we construct a blazed metagrating and optimize it in VirtualLab Fusion.

Ultrashort pulses prove helpful in many modern applications. To manipulate ultrashort pulses, especially for high-power cases, gratings are often employed to either stretch or compress the pulses. The design of such gratings needs careful consideration: they should maintain high efficiency over a spectrum band, and sometimes even for random polarization. In VirtualLab Fusion, you can design gratings using FMM/RCWA, insert the gratings into a setup with pulsed laser sources for system performance evaluation. We demonstrate with the examples below.

Resonant waveguide gratings are used for various applications due to their sensitivity to wavelength and polarization. We pick an example from the work of G. Quaranta et al. and analyze its diffraction properties in VirtualLab Fusion. Additionally, we investigate the angular selectivity/sensitivity of the selected resonant waveguide grating, and visualize the diffraction pattern behind it.

How to resolve better is one of the most important, and most prevalent, question in optics. Ernst Abbe gave his explanation on resolution in 1873 and his theory has played a role to this day. As was done first by Abbe, and then by many other scientists in their labs, we will demonstrate the theory of resolution in VirtualLab Fusion. Thanks to the grating component released in version 2020.1, we build up an imaging system with real chromium gratings as the object, and demonstrate the image formation throughout the system.

Laser guide stars – which are artificial “star” images tens of kilometers away – are important for the correction of atmospheric distortions for astronomical telescopes. The size of the star must be carefully controlled, and the slow-diffraction effect must be considered in the design so as to correctly predict the focal spot. We analyze and design such systems in VirtualLab Fusion and show how to configure the Fourier transform settings for such tasks.

It is often important to ensure good beam quality for many laser-based optical experiments and applications. Laser beams, in reality, may contain higher-order modes or exhibit wavefront perturbation, and consequently need to be cleaned up. A typical method is to use a spatial filtering setup, with two lenses and a pinhole in the intermediate focal plane, i.e. the Fourier plane. We build up such a spatial filtering setup and check how the pinhole size influences the output beam quality and power.

Diffraction effects are typically considered only at the exit pupil of a system and including intra-system diffraction (especially when it is caused by multiple truncations), as discussed by M. Mout et al., is a challenging task. With the innovations in Fourier transforms, you have direct and flexible control of the diffraction inclusion in VirtualLab Fusion 2020.1. As an example, we demonstrate the modeling of pinhole as well as surface aperture diffraction effects inside a low-Fresnel-number system, and compare the results with the typical exit pupil diffraction approach.

We are proud to present a new version of VirtualLab Fusion, in which we bring the connecting field solvers technology to the next level.

In order to adapt to different time zones worldwide, we will hold this webinar twice (all times CET):

8 July | 10:00 – 11:00 & 17:00 – 18:00