PsiReal
Similar to the `pseudo-realistic' subcritical movie,
this movie shows the Re{\Psi_4} outgoing and
Re{\Psi_0} ingoing components of the gravitational field in
their full 3D structure.
As this wave contains enough energy concentration to form a black hole,
the waves `get stuck' at the central region and an apparent horizon occurs.
Some gravitational radiation is emitted from the newly formed highly
distorted black hole, but the final state is a static black hole
(i.e. a Schwarzschild Black Hole).
| Simulation code: |
Miguel Alcubierre
,
Gabrielle Allen
,
Bernd Bruegmann
,
Gerd Lanfermann
,
Lars Nerger
,
Ed Seidel
, Ryoji Takahashi,
Tom Goodale, Daniel Holz, Steve Brandt, Paul Walker, Thomas Radke (AEI)
John Shalf (NCSA)
Toni Arbona, Joan Masso and Carles Bona (University of the Balearic Islands)
Wai-Mo Suen
,
Malcolm Tobias
(WashU)
(
AEI
,
WashU
) |
|
