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dc.contributor.authorChoudhary, A.
dc.contributor.authorLagatsky, Alexander Alexandrovich
dc.contributor.authorKannan, P.
dc.contributor.authorSibbett, Wilson
dc.contributor.authorBrown, C Tom A
dc.contributor.authorShepherd, D. P.
dc.date.accessioned2013-08-06T08:31:02Z
dc.date.available2013-08-06T08:31:02Z
dc.date.issued2012-11-01
dc.identifier63085125
dc.identifierc3d4b14a-2233-4b0c-9b12-de07f3544adf
dc.identifier000310577700021
dc.identifier84868316016
dc.identifier.citationChoudhary , A , Lagatsky , A A , Kannan , P , Sibbett , W , Brown , C T A & Shepherd , D P 2012 , ' Diode-pumped femtosecond solid-state waveguide laser with a 4.9 GHz pulse repetition rate ' , Optics Letters , vol. 37 , no. 21 , pp. 4416-4418 . https://doi.org/10.1364/OL.37.004416en
dc.identifier.issn0146-9592
dc.identifier.otherORCID: /0000-0002-4405-6677/work/86537128
dc.identifier.urihttps://hdl.handle.net/10023/3922
dc.descriptionThis research was funded through Engineering and Physical Sciences Research Council grants EP/H035745/1 and EP/H038035/1.en
dc.description.abstractWe report on the first demonstration of a passively mode-locked, diode-pumped, monolithic Yb:glass channel waveguide laser that incorporates a semiconductor saturable absorber mirror. Stable and self-starting mode-locking is achieved in a Fabry-Perot cavity configuration producing a pulse repetition rate up to 4.9 GHz. The shortest pulse duration of 740 fs is generated with 30 mW of average output power at a center wavelength of 1058 nm. A maximum output power of 81 mW is produced during mode-locking with corresponding pulse duration of 800 fs.
dc.format.extent3
dc.format.extent197164
dc.language.isoeng
dc.relation.ispartofOptics Lettersen
dc.subjectKW peak poweren
dc.subjectCarbon nanotubesen
dc.subjectFibre lasersen
dc.subjectQ Scienceen
dc.subject.lccQen
dc.titleDiode-pumped femtosecond solid-state waveguide laser with a 4.9 GHz pulse repetition rateen
dc.typeJournal articleen
dc.contributor.sponsorEPSRCen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1364/OL.37.004416
dc.description.statusPeer revieweden
dc.identifier.grantnumberEP/H038035/1en


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