Heat transport at warm dense matter interfaces

Wednesday, November 29, 2023 - 2:00pm

SpeakerThomas White, UNR

Program Description:

Transport properties in warm dense matter (WDM), such as thermal conductivity, have extensive theoretical predictions but lack experimental benchmarking [1]. We have developed a Fresnel Diffractive Radiography (FDR) platform at the Omega Laser Facility, which enables high spatial resolution measurements of the evolution of an isochorically-heated WDM interface [2-4]. Novel 1 µm-wide slits provide a spatially coherent X-ray source that, in the presence of sharp density gradients, result in distinct diffraction fringes. Isochoric X-ray heating of CH-coated metal wires sets up a temperature differential at the material interface. After pressure equilibration, the interface is hydrodynamically stable, and the evolution of the interface is driven primarily through thermal conduction, which modifies the temperature and density profiles. We present results for the thermal conductivity of warm dense tungsten and plastic, obtained through analysis of the evolving diffraction pattern. However, our results also reveal the presence of interfacial thermal resistance (ITR) at the boundary between two WDM systems.

 

1) T. G. White et al. PTRSA 381, 20220223 (2023).

2) C. H. Allen et al. AO 61, 1987 (2022).

3) M. Oliver et al. RSI 93, 093502 (2022).

4) M. O. Schoelmerich et al. RSI 94, 013104 (2023).

 

Heat transport at warm dense matter interfaces
Find Stanford Synchrotron Radiation Lightsource on TwitterFind Stanford Synchrotron Radiation Lightsource on YouTubeFind Stanford Synchrotron Radiation Lightsource on Flickr