4.6 Article

70 mJ nonlinear compression and scaling route for an Yb amplifier using large-core hollow fibers

期刊

OPTICS LETTERS
卷 46, 期 4, 页码 896-899

出版社

OPTICAL SOC AMER
DOI: 10.1364/OL.412296

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资金

  1. Austrian Science Fund [P27491]
  2. Canada Foundation for Innovation
  3. Natural Sciences and Engineering Research Council of Canada
  4. Fonds de Recherche du Quebec sur la Nature et les Technologies
  5. National Natural Science Foundation of China [11874121]
  6. Shanghai Municipal Science and Technology Basic Research [19JC1410900]
  7. Alexander vonHumboldt-Stiftung
  8. PROMPT
  9. Austrian Science Fund (FWF) [P27491] Funding Source: Austrian Science Fund (FWF)

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This Letter investigates the energy-scaling rules of hollow-core fiber-based nonlinear pulse propagation and compression merged with high-energy Yb-laser technology. A demonstration shows that high-energy Yb laser amplifier pulses were compressed down to a record peak power. This work presents a critical advance of a high-energy pulse nonlinear interactions platform with potential applications in various fields such as intense THz, X-ray pulses, and Wakefield acceleration.
In this Letter, we investigate the energy-scaling rules of hollow-core fiber (HCF)-based nonlinear pulse propagation and compression merged with high-energy Yb-laser technology, in a regime where the effects such as plasma disturbance, optical damages, and setup size become important limiting parameters. As a demonstration, 70 mJ 230 fs pulses from a high-energy Yb laser amplifier were compressed down to 40 mJ 25 fs by using a 2.8-m-long stretched HCF with a core diameter of 1 mm, resulting in a record peak power of 1.3 TW. This work presents a critical advance of a high-energy pulse (hundreds of mJ level) nonlinear interactions platform based on high energy sub-ps Yb technology with considerable applications, including driving intense THz, X-ray pulses, Wakefield acceleration, parametric wave mixing and ultraviolet generation, and tunable long-wavelength generation via enhanced Raman scattering. (C) 2021 Optical Society of America

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