Lecture Notes in Physics 617: Current Trends in Relativistic Astrophysics
L. Fernández-Jambrina, L.M. González-Romero (Eds.)
Table of Content on page XIII
even-alp-ah.mpg
Movie shows the evolution of the lapse and apparent horizon for even-parity
distorted black hole with excision and dynamic shifts. T shows evolution
time for this simulation. This terminated around T=50M.
even-shift-ah.mpg
Movie shows the evolution of the shift and apparent horizon for even-parity
distorted black hole with excision and dynamic shift. T shows evolution time
for this simulation. This terminated around T=50M. As the shift drives the
system towards a static Schwarzschild black hole spacetime, horizon grows
until certain time and the oscillate towards a static Schwarzschild black hole.
rot-shift-ah.mpg
Movie shows the evolution of the shift and apparent horizon for rotating
distorted black hole with dynamic shift and without excision. T shows the
coordinate time so that the last picture shows them at around t=40M. As the
shift drives the system towards a static Kerr black hole spacetime, horizon
grows until certain time and then oscillates towards a static Kerr black hole.