Sitzung

Session 12 - Warm Dense Matter

30.01.2026, 10:30
Darmstädter Haus

Darmstädter Haus

Oberseitestr. 38 D- 87568 Hirschegg

Vorsitzende der Sitzung

Session 12 - Warm Dense Matter: Session 12 - Warm Dense Matter

  • Stephan Neff (Facility for Antiproton and Ion Research in Europe GmbH(FAIR))

Präsentationsmaterialien

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  1. Martin Schanz (GSI Helmholtzzentrum für Schwerionenforschung GmbH(GSI))
    30.01.26, 10:30
    Invited Talk

    Magnetic lens-based proton radiography is a unique and powerful diagnostics technique capable of resolving ultra-fast processes on the ns-scale in dense matter with unprecedented micrometer spatial resolution. Recently, the PRIOR-II proton radiography facility has been designed, constructed and commissioned at the GSI Helmholtz Centre for Heavy Ion Research, pushing the technical boundaries of...

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  2. Philipp Hesselbach
    30.01.26, 11:00
    Talk

    The HHT experiment area at GSI offers the unique capability to heat matter by intense bunches of high-energy heavy-ions from the SIS-18 heavy-ion synchrotron and to probe the generated short-lived states with X-rays created by the PHELIX laser facility. Focusing ~300-ns-long bunches of up to $4\times 10^9$ $\text{U}^{73+}$ ions down to sub-millimeter spot-sizes, aluminum samples were heated to...

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  3. Julian Lütgert (Universität Rostock Physik(URO-PH))
    30.01.26, 11:20
    Talk

    The graphitization-threshold of diamond is of significant interest for nanodiamond synthesis from laser-shocked plastics, for particle detectors, and for the application in diamond anvil cells.
    We report on experiments conducted at the HHT facility (GSI), in which a monocrystalline diamond target was volumetrically heated using a uranium ion beam. The PHELIX laser enabled measurements of...

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  4. Johannes Rips (University of Rostock)
    30.01.26, 11:40
    Talk

    Accurately determining the ionization state of warm dense carbon is critical
    for predictive modeling in high-energy-density physics, particularly for inertial
    confinement fusion experiments and for advancing the understanding of astro-
    physical systems such as white dwarf envelopes [1,2]. However, obtaining direct
    measurements under the relevant extreme conditions remains challenging....

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