13.07.2015 Views

SAM – saturable absorber mirror

SAM – saturable absorber mirror

SAM – saturable absorber mirror

SHOW MORE
SHOW LESS
  • No tags were found...

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

The reflection bandwidth of the <strong>SAM</strong> has to be larger than the pulse bandwidth. In case ofa <strong>SAM</strong> with an underlying Bragg-<strong>mirror</strong> the reflection bandwidth is determined by the ratioof the refractive indices n H /n L of the layers in the thin film stack. More about Bragg<strong>mirror</strong>s...The relative spectral width w = ∆λ/λ of the high reflectance zone of a conventionalsemiconductor AlAs/GaAs thin film stack is about 0.1. Therefore the width of the highreflection zone of an AlAs/GaAs Bragg-<strong>mirror</strong> with a center wavelength of 1000 nm is about100 nm. From the tables above this results in a minimum pulse duration of about 20 fs. Forshorter pulses other <strong>mirror</strong> types, for instance dielectric or metallic <strong>mirror</strong>s has to be used.7.3 Absorption bandwidthAn ideal <strong>SAM</strong> has a constant <strong>saturable</strong> absorption for all wavelength of the pulse spectrum.In case of a 5 fs pulse the width of this wavelength interval is some hundreds ofnanometers.SeongKyeong Photonics 12 info@skphotonics.com

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!