Kinema Research & Software

The Physics of Warm Dense Matter

                                  

                                        

 

Kinema Research has recently become involved in research on Warm Dense Matter (WDM) in collaboration with Richard W. Lee and Hyun-Kyung Chung at the Lawrence Livermore National Laboratory. We are developing the FLYCHK [1, 2] code for WDM plasma spectroscopy calculations. See References [1]-[4] and the abstract below.


Non-Equilibrium Modeling of Warm Dense Matter

H.-K. Chung (LLNL), W. L. Morgan (Kinema Research), and R. W. Lee (LLNL)

The advent of high brightness femtosecond hard x-ray free electron lasers will provide a new and challenging regime for plasma research. Illumination of solid materials by such light sources will produce highly non-equilibrium plasmas on time scales of tens of femtosecond having mean electron energies in the 1-10 eV range, very non-thermal electron energy distributions, and cold ions at near solid state density. We will discuss our research on modeling the plasma spectroscopy of such warm dense matter [1, 2] with emphasis on treating the electron interactions and non-Maxwell-Boltzmann energy distributions.

1. R. W. Lee, et al., Laser and Particle Beams 20, 527 (2002).

2. R. W. Lee, et al. J. Opt. Soc. Am B 20, 770 (2003).


References

1. "FLYCHK: An Extension to the K-Shell Spectroscopy Kinetics Model FLY", H.-K. Chung, W. L. Morgan, and R. W. Lee, Journal of Quantitative Spectroscopy & Radiative Transfer 81, 107 (2003).

2. "Population Kinetics Modeling For Non-LTE and Non-Maxwellian Plasmas Generated In Finite Temperature Dense Matter Experiments Arising From Short Pulse X-ray Sources", H.-K. Chung, W. L. Morgan, and R. W. Lee, Proceedings of the 3rd International Conference on Inertial Fusion Sciences and Application (September 2003).

3. "Plasma Based Studies With Intense X-Ray and Particle Beam Sources", R. W. Lee, et al., Laser and Particle Beams 20, 527 (2002). [Abstract]

4. "Finite Temperature Dense Matter Studies On Next Generation Light Sources", R. W. Lee, et al., JOSA B 770 (2003). [Abstract]

 

 

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Last modified: September 16, 2003