Covers the modeling of fluid instabilities with linear perturbation theory and explores the origin of unpredictability in turbulence through the Navier-Stokes equations.
Explores the origin of radionuclides from supernova explosions and their role in nature, covering topics such as nuclear astrophysics, cosmic element formation, and stellar evolution.
Explores the historical discovery and mechanisms behind stellar pulsations, emphasizing their classification and significance in understanding stellar structure.
Explores the Diffusion Approximation method for solving the RTE in tissue optics, emphasizing its limitations and applications, along with the practical aspects of Monte Carlo simulations.
Delves into the origin of chemical elements in the universe through nuclear astrophysics, exploring processes like Big Bang nucleosynthesis and stellar evolution.
