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astro-ph.SR2025
Numerical Simulations Confirm Wave-Induced Shear Mixing in Stellar Interiors
A. Varghese, R. P. Ratnasingam, L. Ramírez-Galeano +2
Internal Gravity Waves (IGWs) are thought to cause mixing in stellar interiors, a process that has been widely studied both theoretically and numerically. Our aim is to determine t…
astro-ph.SR2025
Angular Momentum Transport by Internal Gravity Waves Across Age
Tamara Marie Rogers, Rathish Previn Ratnasingam
We present two-dimensional numerical simulations of convection and waves in a 7 solar mass star across stellar ages ranging from zero age to terminal-age-main-sequence. We show tha…