in-depth study of the intra-stark spectroscopy in the x-ray range … · 2luli - upmc univ paris...
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In-depth Study of the Intra-Stark Spectroscopy in the X-Ray Range under
Relativistic Laser-Plasma Interaction
E. Oks,1 E. Dalimier,2 A.Ya. Faenov,3,4 P. Angelo,2 S.A. Pikuz,4,5 T.A. Pikuz,4,6 , I.Yu.
Skobelev4,5, S.N. Ryazanzev4,7, P. Durey8, L. Doehl8, D. Farley8, C. Baird8, K.L. Lancaster8,
C.D. Murphy8, N. Booth,9 C. Spindloe9, P. Mckenna10, N. Neumann11, M. Roth11, R.
Kodama3,6 and N. Woolsey8
1Physics Department, 206 Allison Lab, Auburn University, Auburn, AL 36849, USA 2LULI - UPMC Univ Paris 06: Sorbonne Universités ; CNRS, Ecole Polytechnique, CEA:
Université Paris-Saclay - F-75252 Paris cedex 05, France 3Open and Transdisciplinary Research Iniative, Osaka University, Suita, Osaka, 565-0871, Japan 4Joint Institute for High Temperatures, Russian Academy of Sciences, Moscow 125412, Russia 5National Research Nuclear University MEPhI, Moscow 115409, Russia. 6PPC and Graduate School of Engineering, Osaka University, 2-1, Yamadaoka, Suita, Osaka 565-
0871, Japan 7Moscow State University, Moscow, 119991, Russia 8York Plasma Institute, Department of Physics, University of York, York YO10 5DD, UK 9Central Laser Facility, STFC Rutherford Appleton Laboratory, Didcot OX11 0QX, UK 10Department of Physics, SUPA, University of Strathclyde, Glasgow G4 0NG, UK
11Institut fur Kernphysik, Technische Univesitat Darmstadt, Schlossgartenstraße 9, 64289 Darmstadt,
Germany
Corresponding authors emails: [email protected],
Abstract
Intra-Stark Spectroscopy (ISS) is the spectroscopy within the quasistatic Stark profile of a spectral
line. In the ISS some local depressions (“dips”) occur at certain locations of the quasistatic Stark
profile of a spectral line. This phenomenon arises when radiating atoms/ions are subjected
simultaneously to a quasistatic field F and to a quasimonochromatic electric field E(t) at the
characteristic frequency ω. The present paper advances the study of the relativistic laser-plasma
interaction from our previous paper (Oks et al, Optics Express 25 (2017) 1958). First, by
improving the experimental conditions and the diagnostics, it provides a systematic spectroscopic
study of the simultaneous production of the Langmuir waves and of the ion acoustic turbulence at
the surface of the relativistic critical density. It demonstrates a reliable reproducibility of the
Langmuir-wave-caused dips at the same locations in the experimental profiles of Si XIV Ly-beta
line, as well as of the deduced parameters (fields) of the Langmuir waves and ion acoustic
turbulence in different laser shots. Second, this study employs for the first time the most rigorous
condition of the dynamic resonance, on which the ISS phenomenon is based, compared to all
previous studies in all kinds of plasmas in a wide range of electron densities. It shows how
different interplays the Langmuir wave field with the field of the ion acoustic turbulence lead to
different manifestations in spectral line profiles, including the disappearance of the Langmuir-
wave-caused dips.
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