European X-ray laser explores a poorly understood state of matter

7 August 2024

EurekAlert!: [https://www.eurekalert.org/news-releases/1054008]

Warm dense matter occurs inside Jupiter-type giant planets (where it surrounds the rocky core as a metallic liquid at a temperature of many thousands of kelvin) and in the interiors of small stars – brown dwarfs. (Source: IFJ PAN / NASA)

The properties of warm dense matter have until recently been little known. Now, thanks to the use of X-ray lasers, physicists are gaining more and more information about this important but still mysterious state of matter. The first comprehensive observations of ionisation processes in warm dense matter, carried out at the European X-ray Free-Electron Laser (European XFEL), have just been presented in one of the most prestigious physics journals.

State of matter with a temperature of a few thousand degrees and a high density, close to that of a solid, can be found, among others, in the interiors of brown dwarfs or gaseous planets. Although common in the Universe, it is very difficult to be produced and analysed in the laboratory. A new era in experimental research of this so-called warm dense matter (WDM) state began just a dozen years ago, when physicists launched the first free-electron X-ray lasers. At the forefront of this type of device is the nearly 3.5 km-long European XFEL laser. A series of experiments recently carried out there made it possible to observe for the first time how quickly a metal transforms into the exotic state of ionised WDM to become transparent (non-absorbing) to X-rays at the end of the process. The achievement of the international team of scientists – including those from the Institute of Nuclear Physics of the Polish Academy of Sciences (IFJ PAN) in Cracow – is discussed in a paper published in the journal Nature Physics.

X-Ray Free-Electron Lasers (XFELs) are used to generate high-intensity X-ray pulses lasting single femtoseconds, i.e. millionths of a billionth of a second. These can be used to study the structure of matter at atomic length scales and to track phenomena on extremely short time scales. One of only a dozen such devices in the world is the European XFEL in Hamburg, built in cooperation with the DESY research centre.

“In our experiment at the European XFEL, we illuminated copper samples with X-ray pulses lasting 15 femtoseconds, using different, gradually increasing intensities”, Prof. Beata Ziaja-Motyka (IFJ PAN, DESY) introduces the experiment. The first author of the paper in question, Dr. Laurent Mercadier from the European XFEL, adds some physical details: “When a single X-ray laser pulse reached the material, it caused strong ionisation. The electrons released in the process were characterised by high temperatures. Under these extreme conditions, the copper was transformed into a state of warm dense matter. We meticulously recorded how much radiation passed through the matter and from this inferred the ionisation changes in the observed system.”

Simulations carried out using the BOLTZMANN SOLVER software, developed since 2004 at DESY by Prof. Ziaja-Motyka, were particularly helpful in interpreting the measurement results. This tool was used to simulate changes in the electronic occupancy of individual energy levels in WDM depending on the intensity of the incident laser radiation.

By confronting experimental data with simulations, it was established that when the X-ray intensity becomes sufficiently high, atoms of WDM become strongly ionised. As a result of this phenomenon, new energy levels appear which can be occupied by excited electrons – making WDM opaque for photons resonant with transitions to these new energy levels. These states had already been observed previously with optical lasers, however, the lasers’ energy limitations did not allow them to be studied in more detail. Now, thanks to the European X-ray laser XFEL, it is possible to characterise them accurately also in response to various intensities of X-ray pulses. In accordance with theoretical predictions for X-ray absorption spectra, prepared by Dr. Joshua Kas (University of Washington, USA) and Dr. Andrei Benediktovitch (DESY, Hamburg), it was further observed that with increasing the laser intensity the warm dense matter becomes first opaque and then – at highest intensities – transparent to the laser pulse.

“The appearance of ‘transparency’ – i.e. lack of absorption – in WDM is a consequence of the high ionisation of WDM atoms occurring at sufficiently high X-ray pulse intensities. The energy of the Xray photons available in the experiment then becomes too small to excite further electrons. As a result, these photons cannot be absorbed by the warm dense matter at all”, explains Prof. Ziaja- Motyka.

Knowledge of the properties of warm dense matter and the processes taking place within it is not only of astrophysical, but also of practical, engineering importance. Matter in this state plays an important role in certain types of controlled nuclear fusion (ICF – Inertial Confinement Fusion), and also appears during the ablation of metallic heat shields of spacecraft returning from orbit to Earth.

The team of physicists at the European X-ray XFEL laser, led by Prof. Nina Rohringer (DESY, Universität Hamburg), intends to continue research into the electron and ionisation processes occurring in WDM and their dynamics. On the Polish side, the work is co-financed by the Institute of Nuclear Physics of the Polish Academy of Sciences.

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Contact:

Prof. Beata Ziaja-Motyka
Institute of Nuclear Physics, Polish Academy of Sciences
Center for FEL Science, DESY
tel.: +48 12 662 8209
email: ziaja@mail.desy.de

Scientific papers:

„Transient Absorption of Warm Dense Matter Created by an X-Ray Free-Electron Laser”
L. Mercadier, A. Benediktovitch, S. Krusic, J. J. Kas, J. Schlappa, M. Agaker, R. Carley, G. Fazio, N. Gerasimova, Y. Y. Kim, L. Le Guyader, G. Mercurio, S. Parchenko, J. J. Rehr, J.-E. Rubensson, S. Serkez, M. Stransky, M. Teichmann, Z. Yin, M. Zitnik, A. Scherz, B. Ziaja-Motyka, N. Rohringer
Nature Physics 2024
DOI: https://doi.org/10.1038/s41567-024-02587-w

Images:

Warm dense matter occurs inside Jupiter-type giant planets (where it surrounds the rocky core as a metallic liquid at a temperature of many thousands of kelvin) and in the interiors of small stars – brown dwarfs. (Source: IFJ PAN / NASA)