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Alloharmonics in high-resolution BISER spectra

https://repo.qst.go.jp/records/2003226
https://repo.qst.go.jp/records/2003226
8779e046-91bd-4f54-ac85-528025d5c5b9
アイテムタイプ 会議発表用資料 / Presentation(1)
公開日 2026-04-30
タイトル
タイトル Alloharmonics in high-resolution BISER spectra
言語 en
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言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_c94f
資源タイプ conference presentation
著者 Alexander Pirozhkov

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Alexander Pirozhkov

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Marina Pirozhkova

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Marina Pirozhkova

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Ogura Koichi

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Ogura Koichi

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Sagisaka Akito

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Sagisaka Akito

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Esirkepov Timur

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Esirkepov Timur

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A. Ya. Faenov

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A. Ya. Faenov

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Pikuz Tatiana

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Pikuz Tatiana

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Kotaki Hideyuki

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Kotaki Hideyuki

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Hayashi Yukio

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Hayashi Yukio

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Fukuda Yuji

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Fukuda Yuji

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James Kevin Koga

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James Kevin Koga

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Sergey Bulanov

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Sergey Bulanov

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Daido Hiroyuki

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Daido Hiroyuki

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Hasegawa Noboru

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Hasegawa Noboru

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Ishino Masahiko

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Ishino Masahiko

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Nishikino Masaharu

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Nishikino Masaharu

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Koike Masato

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Koike Masato

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Kawachi Tetsuya

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Kawachi Tetsuya

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Kiriyama Hiromitsu

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Kiriyama Hiromitsu

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D. Neely

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D. Neely

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Kando Masaki

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Kando Masaki

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抄録
内容記述 Burst Intensification by Singularity Emitting Radiation (BISER) in underdense relativistic laser plasma is a bright source of temporarily and spatially coherent XUV and x-ray radiation [1-3]. BISER scales favorably with the laser power and can produce 1012 photons per pulse (with ~100 TW laser power, as in our experiment with the J-KAREN-P laser [4,5]). BISER originates from relativistic plasma singularities and has a nano-scale source size. BISER spectra have hundreds of electronvolt (eV) bandwidth and, according to the simulations [2], close to the transform-limited duration, which promises Terawatt pulses shorter than the atomic unit of time (24 attoseconds).We performed high-resolution measurements of BISER spectra and found harmonic-like spectral fringes with separation much finer (down to 0.12 eV) than the initial driving laser frequency, ~1.5 eV. Further, BISER spectra contained several fringe spacings in one shot.To explain the observations, we propose the concept of alloharmonics [6,7], i.e. spectral interference of different harmonic orders from different emission moments in a (slightly) nonperiodic generation process.The alloharmonics phenomenon generalizes classical harmonics and is critical in attosecond physics, optical frequency combs, and other fields where nonperiodic processes can generate harmonics. The discovery of alloharmonics emphasizes that x-ray spectrographs with much higher resolving power than typically used, and simultaneously with wider bandwidth, are demanded in experiments with harmonics and harmonic-like spectra.
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内容記述 2026 OPIC-XOPT
発表年月日
日付 2026-04-20
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Ver.1 2026-05-07 23:26:26.972075
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