研究成果 - 汪治平 博士
原子物理與光學組

強場物理與超快技術實驗室
主持人:汪治平 博士
電子郵件:點此顯示(開新頁)
辦公室:340
辦公室電話:+886-2-2366-8263
實驗室:223
實驗室電話:+886-2-2366-8223
主持人:汪治平 博士
電子郵件:點此顯示(開新頁)
辦公室:340
辦公室電話:+886-2-2366-8263
實驗室:223
實驗室電話:+886-2-2366-8223
Energetic picosecond 10.2-μm pulses generated in a BGGSe crystal for nonlinear seeding of terawatt-class CO2 amplifiers
Optics Express
We demonstrate what we believe to be a new approach to energetic picosecond
10.2-μm pulse generation based on nonlinear mixing of subnanosecond single-frequency 1338-
nm pulses and broadband 1540-nm chirped pulses in a BGGSe crystal followed by a grating
compressor for the purpose of seeding high-power CO2 amplifiers. The energy of the 10.2-μm
pulses exceeding 60 μJ with 3.4%-rms fluctuation can be routinely obtained. Single-shot pulse
duration measurement, performed by Kerr polarization rotation time-resolved by a streak camera,
together with the pulse spectrum, indicates the pulse width is between 2.7-3 ps. Numerical
calculations show that power broadening and dynamic gain saturation with Rabi-flopping can
be induced with such an intense seed in a multi-atmospheric CO2 amplifier. These nonlinear
effects greatly suppresses pulse splitting due to the comb-like spectrum of the CO2 molecule. A
peak power exceeding 1 TW is expected after multipass of amplification while maintaining an
appropriate high intensity by controlling the beam size along the path.
10.2-μm pulse generation based on nonlinear mixing of subnanosecond single-frequency 1338-
nm pulses and broadband 1540-nm chirped pulses in a BGGSe crystal followed by a grating
compressor for the purpose of seeding high-power CO2 amplifiers. The energy of the 10.2-μm
pulses exceeding 60 μJ with 3.4%-rms fluctuation can be routinely obtained. Single-shot pulse
duration measurement, performed by Kerr polarization rotation time-resolved by a streak camera,
together with the pulse spectrum, indicates the pulse width is between 2.7-3 ps. Numerical
calculations show that power broadening and dynamic gain saturation with Rabi-flopping can
be induced with such an intense seed in a multi-atmospheric CO2 amplifier. These nonlinear
effects greatly suppresses pulse splitting due to the comb-like spectrum of the CO2 molecule. A
peak power exceeding 1 TW is expected after multipass of amplification while maintaining an
appropriate high intensity by controlling the beam size along the path.
link: 相關連結
目前位置:本所人員 / 研究人員 / 汪治平 / 研究成果
中央研究院 原子與分子科學研究所版權所有 |
個人隱私權聲明 |
保有個資檔案公開項目彙整表 |
行動版
地址: 106319 台北市羅斯福路四段一號 或 106923 臺北臺大郵局 第23-166號信箱
電話:886-2-2362-0212 傳真:886-2-2362-0200 電子郵件:iamspublic@gate.sinica.edu.tw
最後更新於 2025-04-30 14:15:19
地址: 106319 台北市羅斯福路四段一號 或 106923 臺北臺大郵局 第23-166號信箱
電話:886-2-2362-0212 傳真:886-2-2362-0200 電子郵件:iamspublic@gate.sinica.edu.tw
最後更新於 2025-04-30 14:15:19