| Autor: |
Bang W; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA., Albright BJ; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA., Bradley PA; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA., Gautier DC; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA., Palaniyappan S; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA., Vold EL; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA., Santiago Cordoba MA; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA., Hamilton CE; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA., Fernández JC; Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA. |
| Abstrakt: |
With the development of several novel heating sources, scientists can now heat a small sample isochorically above 10,000 K. Although matter at such an extreme state, known as warm dense matter, is commonly found in astrophysics (e.g., in planetary cores) as well as in high energy density physics experiments, its properties are not well understood and are difficult to predict theoretically. This is because the approximations made to describe condensed matter or high-temperature plasmas are invalid in this intermediate regime. A sufficiently large warm dense matter sample that is uniformly heated would be ideal for these studies, but has been unavailable to date. Here we have used a beam of quasi-monoenergetic aluminum ions to heat gold and diamond foils uniformly and isochorically. For the first time, we visualized directly the expanding warm dense gold and diamond with an optical streak camera. Furthermore, we present a new technique to determine the initial temperature of these heated samples from the measured expansion speeds of gold and diamond into vacuum. We anticipate the uniformly heated solid density target will allow for direct quantitative measurements of equation-of-state, conductivity, opacity, and stopping power of warm dense matter, benefiting plasma physics, astrophysics, and nuclear physics. |
