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Abstract
Ultrashort pulse generation hinges on the careful management of dispersion. Traditionally, this has exclusively involved second-order dispersion, with higher-order dispersion treated as a nuisance to be minimized. Here, we show that this higher-order dispersion can be strategically leveraged to access an uncharted regime of ultrafast laser operation. In particular, our mode-locked laser—with an intracavity spectral pulse shaper—emits pure-quartic soliton pulses that arise from the interaction of fourth-order dispersion and the Kerr nonlinearity. Phase-resolved measurements demonstrate that their pulse energy scales with the third power of the inverse pulse duration. This implies a strong increase in the energy of short pure-quartic solitons compared with conventional solitons, for which the energy scales as the inverse of the pulse duration. These results not only demonstrate a novel approach to ultrafast lasers, but more fundamentally, they clarify the use of higher-order dispersion for optical pulse control, enabling innovations in nonlinear optics and its applications.
By suppressing the second- and third-order intracavity dispersion using an intracavity spectral pulse shaper, a mode-locked laser that emits pure-quartic soliton pulses that arise from the interaction of the fourth-order dispersion and the Kerr nonlinearity is demonstrated.
Details
; Hudson, Darren D 2
; Tam Kevin K K 1
; de Sterke C Martijn 3
; Blanco-Redondo, Andrea 4
1 The University of Sydney, Institute of Photonics and Optical Science (IPOS), School of Physics, Sydney, Australia (GRID:grid.1013.3) (ISNI:0000 0004 1936 834X)
2 Macquarie University, MQ Photonics, Department of Physics and Astronomy, Sydney, Australia (GRID:grid.1004.5) (ISNI:0000 0001 2158 5405); CACI Photonics Solutions, Florham Park, USA (GRID:grid.1004.5)
3 The University of Sydney, Institute of Photonics and Optical Science (IPOS), School of Physics, Sydney, Australia (GRID:grid.1013.3) (ISNI:0000 0004 1936 834X); The University of Sydney, The University of Sydney Nano Institute (Sydney Nano), Sydney, Australia (GRID:grid.1013.3) (ISNI:0000 0004 1936 834X)
4 Nokia Bell Labs, Holmdel, USA (GRID:grid.1013.3)





