
About
Vishnu Varma R Vejayan is Research Associate in Theoretical Stellar Astrophysics at Keele University's Lennard-Jones School of Chemical and Physical Sciences. Research employs advanced 3D simulations to investigate stellar convection, magnetohydrodynamics, and supernova mechanisms in massive star evolution.
Recent publications focus on hydrodynamic modeling of late-stage stellar evolution, including neon/oxygen burning phases, convective shell mergers, and magnetoconvection in rapidly rotating supernova progenitors. Computational approaches reveal insights into explosion dynamics, remnant formation, and nuclear burning processes.
Collaborative work appears in Monthly Notices of the Royal Astronomical Society and Galaxies, advancing understanding of multi-dimensional stellar phenomena.
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