Sapphire-based resonant waveguide-grating mirrors : advancing their intra-cavity power density capability
dc.contributor.author | Bashir, Danish | |
dc.contributor.author | Boubekraoui, Ayoub | |
dc.contributor.author | Mourkioti, Georgia | |
dc.contributor.author | Li, Fangfang | |
dc.contributor.author | Karvinen, Petri | |
dc.contributor.author | Kuittinen, Markku | |
dc.contributor.author | Mackenzie, Jacob. I. | |
dc.contributor.author | Graf, Thomas | |
dc.contributor.author | Abdou Ahmed, Marwan | |
dc.date.accessioned | 2024-12-18T08:41:40Z | |
dc.date.available | 2024-12-18T08:41:40Z | |
dc.date.issued | 2023 | de |
dc.date.updated | 2024-11-02T08:56:33Z | |
dc.description.abstract | We report on the design, fabrication, and implementation of a single-layer resonant waveguide-grating (RWG) mirror on a sapphire substrate. Our goal is to enhance these optics capability to withstand high intra-cavity power densities by exploiting the superior thermal properties of sapphire. The RWG was implemented as an intra-cavity folding mirror in an Yb:YAG thin-disk laser to generate linearly polarized and spectrally stabilized radiation. A linearly polarized output power of 191 W with an optical efficiency of 39% was obtained in multi-mode operation. This corresponds to a power density of 52 kW/cm 2 on the RWG, for which the increase of its surface temperature was measured to be 12 K, which resulted in a 46-fold reduction of the surface temperature rise dependence on the intra-cavity power density with respect to what has been reported for a RWG on a fused silica substrate. In near fundamental-mode operation, a linearly polarized emission with an output power of 90 W, an optical efficiency of 30%, and a spectral bandwidth of 28 pm FWHM was obtained. | en |
dc.description.sponsorship | Projekt DEAL | de |
dc.description.sponsorship | European Union's Horizon 2020 research and innovation | de |
dc.description.sponsorship | Universität Stuttgart | de |
dc.identifier.issn | 1432-0649 | |
dc.identifier.issn | 0946-2171 | |
dc.identifier.other | 1914925017 | |
dc.identifier.uri | http://nbn-resolving.de/urn:nbn:de:bsz:93-opus-ds-154575 | de |
dc.identifier.uri | http://elib.uni-stuttgart.de/handle/11682/15457 | |
dc.identifier.uri | http://dx.doi.org/10.18419/opus-15438 | |
dc.language.iso | en | de |
dc.relation | info:eu-repo/grantAgreement/EC/H2020/813159 | de |
dc.relation.uri | doi:10.1007/s00340-023-08144-2 | de |
dc.rights | info:eu-repo/semantics/openAccess | de |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | de |
dc.subject.ddc | 620 | de |
dc.title | Sapphire-based resonant waveguide-grating mirrors : advancing their intra-cavity power density capability | en |
dc.type | article | de |
ubs.fakultaet | Konstruktions-, Produktions- und Fahrzeugtechnik | de |
ubs.fakultaet | Fakultätsübergreifend / Sonstige Einrichtung | de |
ubs.institut | Institut für Strahlwerkzeuge | de |
ubs.institut | Fakultätsübergreifend / Sonstige Einrichtung | de |
ubs.publikation.seiten | 8 | de |
ubs.publikation.source | Applied physics B 130 (2024), No. 4 | de |
ubs.publikation.typ | Zeitschriftenartikel | de |