The neutron stars are described by a gamma=2 polytropic equation of
state. The evolution begins at a late stage in their long inspiral to
coalescence driven by gravitational radiation (initially they are in a
quasi equilibrium orbit with a relative separation of ra=0.25, proper
separation of 61.3km).
MPEG format (9.5 MB)
Quicktime format (3 MB)
A gravitational plane wave hitting a neutron star.
Evolution of two spatial derivatives of the metric gxx (d^2 gxx / dz^2).
ns_pw1.mov SGI format (1.3Mb)
ns_pw2.mov SGI format (1.1Mb)
ns_pw2.qt Quicktime format (4.0Mb)
ns_pw3.mov SGI format (2.4Mb)
ns_pw3.qt Quicktime format (5.6Mb)
arrows.qt (File size 5.4Mb)
isoline.qt (File size
7.6Mb)
The AVS module file used to create this,
IsoLineVector.v
ortho.qt (File size 10.5Mb)
twoiso.qt (File size 6.6Mb bytes)
The AVS module file used to create this,
TwoIsoSurfaces.v
glancing_iso.qt(File size 2.8Mb)
OrthoGlancing.qt (File size
1.1Mb
bytes)
The AVS module file used to create this,
OrthoMovie.v
nsns_newt.qt (File size
3.0Mb
bytes)
DensEngy.qt (File size
845k)
The AVS module file used to create this,
DensEngy.v
NoShiftLowRes.mov Quicktime format (.6Mb)
YesShiftLowRes.mov Quicktime format (2.0Mb)
YesShiftwArLowRes.mov Quicktime format (2.4Mb)
lapseLowRes.mov Quicktime format (1.0Mb)
GRInspiral.mov Quicktime format (2.5Mb)