Institute for Astronomy and Astrophysics

Oscillations of Rotating and Magnetized stars in Numerical Relativity

We review recent progress in modelling oscillations of rotating and magnetized stars, using techniques of numerical relativity. Specifically, new results on axisymmetric oscillations of uniformly rotating stars and of hot remnants of core collapse will be discussed. In addition, we discuss progress in studying internal magnetohydrodynamic and magneto-elastic oscillations of magnetars.