Warm Dense Matter
This compressed state is typically defined by temperatures of tens of thousands of Kelvin and densities comparable with those of solids. It is a complex state of matter where multi-body particle correlations and quantum effects must be considered. With relatively few observational data points we much turn to both simulations and experiments to understand their properties. For example: What is the pressure at the center of Jupiter? What is the sound-speed or viscosity at the center of Trappist-1e? An Earth-sized exo-planet just 40 light-years away!
Inertial Confinement Fusion
Inertial confinement fusion efforts use high-powered lasers to compress small captules of Deuterium and Tritium to extremely high densities. These capsules reach temperatures in excess of 100 million degrees Celcius and, for a very small period of time, a mini version of a star is created. The goal of all this work is create an unlimited, clean energy source here on earth that can help us deal with the dwindling supply of fossil fuels and other natural resources.
In our most recent work we investigated the statistical properties of supersonic turbulence; the faster-than-sound stochastic motion of the plasma. Understanding how these plasmas behave informs our understanding of molecular clouds and the processes within, including star formation.More Details
On Earth, we can generate high energy density states of matter using high-powered lasers. These lasers rapidly deposit large quantities of energy into an extremely small area and, on a nanosecond timescale, are capable of reproducing a multitude of astrophysical situations. We perform experiments on table-top laser facilities here at UNR, the larger laser in the world – the National Ignition Facility, and the three kilometer long next generation light source – LCLS.
In order to model our experimentals we perform a number of simulations across a range of temporal and spatial scales. Atomistic simulations that employ molecular dynamics are capable of following the trajectory of every particle. If we attempt to treat the electron fully quantum mechanically, such as in Density Functional Theory or Wave Packet Molecular Dynamics, we are limited to systems of just a few hundred ions, even when utilizing highly parallelized high-performance computing systems. Classical simulations employ the Born-Oppenheimer approximation to avoid treating the electrons, but in doing so are able to treat systems consisting of a few millions atoms. However, this still represents micron sized systems, around 1/100th of the size of a human hair. To model even larger systems we must resort to continuum methods such as magneto-hydrodynamics.
Recent Publications1. R. Davis et al., Ion Modes in Dense Ionized Plasmas through Non-Adiabatic Molecular Dynamics (2020) 2. B. Larder, D. O. Gericke, S. Richardson, P.Mabey, T. G. White and G. Gregori, Fast nonadiabatic dynamics of many-body quantum systems, Science Advances 5(11), eaaw1634 (2019) 3. T. G White, M. Oliver, P. Mabey, et al., Supersonic plasma turbulence in the laboratory, Nature Communications 10(1), 1758 (2019) 4. E. E. McBride, T. G. White et al., Setup for meV-resolution inelastic X-ray scattering measurements and X-ray diffraction at the Matter in Extreme Conditions endstation at the Linac Coherent Light Source, Review of Scientific Instruments 89(10), 10F104 (2018)
Celebrating the end of the Fall 2019 Semester with a group ice skating trip!
From left: Dr Mathew
Oliver (Post Doc), Jacob Molina (UG) , Wataru Hayashi (UG), Thomas White, Emily
Chau (UG), Ryan Davis (Grad)
UG Student and McNair Scholar
If you are interested in joining the group please reach out. Research and collaboration opportunities are often available
Previous Group Members