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Phase-matched optical parametric conversion of ultrashort pulses in a hollow waveguide

dc.contributor.authorDurfee, Charles G.en_US
dc.contributor.authorBackus, Sterlingen_US
dc.contributor.authorMurnane, Margaret M.en_US
dc.contributor.authorKapteyn, Henry C.en_US
dc.date.accessioned2011-11-15T16:01:12Z
dc.date.available2011-11-15T16:01:12Z
dc.date.issued1998-02-20en_US
dc.identifier.citationDurfee, Charles G.; Backus, Sterling; Murnane, Margaret M.; Kapteyn, Henry C. (1998). "Phase-matched optical parametric conversion of ultrashort pulses in a hollow waveguide." AIP Conference Proceedings 426(1): 331-335. <http://hdl.handle.net/2027.42/87447>en_US
dc.identifier.otherAPCPCS-426-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87447
dc.description.abstractWe demonstrate for the first time nonresonant phase-matched frequency conversion of ultrashort pulses in gases. Broad-bandwidth ultrafast pulses, tunable around 270 nm, were generated from a Ti:sapphire amplifier system using 2ω+2ω−ω2ω+2ω−ω parametric wave mixing in a capillary waveguide. Both the fundamental and the second-harmonic light were coupled into the lowest-order (EH11)(EH11) mode. The output pulses have an energy >4μJ at a 1kHz repetition rate, in the EH11EH11 spatial mode. This method can be made to generate 10–20fs pulses, and is the first phase-matching technique which is applicable to frequency conversion into the deep- and vacuum-ultraviolet regions of the spectrum. © 1998 American Institute of Physics.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titlePhase-matched optical parametric conversion of ultrashort pulses in a hollow waveguideen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumCenter for Ultrafast Optical Science, University of Michigan, Ann Arbor, Michigan 48109-2099en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87447/2/331_1.pdf
dc.identifier.doi10.1063/1.55242en_US
dc.identifier.sourceSuperstrong fields in plasmasen_US
dc.owningcollnamePhysics, Department of


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