Evidence map›Paper›PMID 33298838›Full record

ArticleLight, science & applications2020

Nonlinear ionization dynamics of hot dense plasma observed in a laser-plasma amplifier.

F Tuitje, P Martínez Gil, T Helk, J Gautier, F Tissandier, J-P Goddet, A Guggenmos, U Kleineberg, S Sebban, E Oliva and 2 more

Abstract readLetter
In one paragraph

Article in Light, science & applications, 2020. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

0numbers the graph read from it
0cells of the map it votes in
0citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

0 citing papers in PubMed.

No citing paper in PubMed yet.

4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

12 authors.

F TuitjeInstitute for Optics and Quantum Electronics, Abbe Center of Photonics, University of Jena, Jena, Germany. frederik.tuitje@uni-jena.de.
P Martínez GilDepartamento de Ingeniería Energética and Instituto de Fusión Nuclear "Guillermo Velarde", ETSI Industriales, Universidad Politécnica de Madrid, Madrid, Spain.
T HelkInstitute for Optics and Quantum Electronics, Abbe Center of Photonics, University of Jena, Jena, Germany.
J GautierLaboratoire d'Optique Appliquée, ENSTA Paris, Ecole Polytechnique, CNRS, Institut Polytechnique de Paris, Palaiseau, France.
F TissandierLaboratoire d'Optique Appliquée, ENSTA Paris, Ecole Polytechnique, CNRS, Institut Polytechnique de Paris, Palaiseau, France.
J-P GoddetLaboratoire d'Optique Appliquée, ENSTA Paris, Ecole Polytechnique, CNRS, Institut Polytechnique de Paris, Palaiseau, France.
A GuggenmosDepartment for Physics, Ludwig-Maximilian-University Munich, Garching, Germany.
U KleinebergDepartment for Physics, Ludwig-Maximilian-University Munich, Garching, Germany.
S SebbanLaboratoire d'Optique Appliquée, ENSTA Paris, Ecole Polytechnique, CNRS, Institut Polytechnique de Paris, Palaiseau, France.
E OlivaDepartamento de Ingeniería Energética and Instituto de Fusión Nuclear "Guillermo Velarde", ETSI Industriales, Universidad Politécnica de Madrid, Madrid, Spain. eduardo.oliva@upm.es.ORCID http://orcid.org/0000-0003-2284-0927
C SpielmannInstitute for Optics and Quantum Electronics, Abbe Center of Photonics, University of Jena, Jena, Germany.ORCID http://orcid.org/0000-0002-5223-4170
M ZürchInstitute for Optics and Quantum Electronics, Abbe Center of Photonics, University of Jena, Jena, Germany. mwz@berkeley.edu.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Understanding the behaviour of matter under conditions of extreme temperature, pressure, density and electromagnetic fields has profound effects on our understanding of cosmologic objects and the formation of the universe. Lacking direct access to such objects, our interpretation of observed data mainly relies on theoretical models. However, such models, which need to encompass nuclear physics, atomic physics and plasma physics over a huge dynamic range in the dimensions of energy and time, can only provide reliable information if we can benchmark them to experiments under well-defined laboratory conditions. Due to the plethora of effects occurring in this kind of highly excited matter, characterizing isolated dynamics or obtaining direct insight remains challenging. High-density plasmas are turbulent and opaque for radiation below the plasma frequency and allow only near-surface insight into ionization processes with visible wavelengths. Here, the output of a high-harmonic seeded laser-plasma amplifier using eight-fold ionized krypton as the gain medium operating at a 32.8 nm wavelength is ptychographically imaged. A complex-valued wavefront is observed in the extreme ultraviolet (XUV) beam with high resolution. Ab initio spatio-temporal Maxwell-Bloch simulations show excellent agreement with the experimental observations, revealing overionization of krypton in the plasma channel due to nonlinear laser-plasma interactions, successfully validating this four-dimensional multiscale model. This constitutes the first experimental observation of the laser ion abundance reshaping a laser-plasma amplifier. The presented approach shows the possibility of directly modelling light-plasma interactions in extreme conditions, such as those present during the early times of the universe, with direct experimental verification.

Identifiers

PMID33298838
PMCPMC7673011

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