MPEG Movies of Research Results
- SU(2) EYM Collapse
- Collapse of massive scalar wave packet:
r phi and
dm/dr.
-
dm/dr for a near-critical, echoing, Yang-Mills configuration
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Near-critical, echoing, Yang-Mills configuration:
Z = (W - 1)/r (red), D[Z] (green), D^2[Z] (yellow) and D^3[Z] (blue),
where D[Z] = r dZ/dr.
-
W(r)for a near-critical, non-echoing, Yang-Mills configuration
-
dm/dr vs ln(r) for a variety of critical configurations from
scalar-field collapse in Brans-Dicke theory (with Steve Liebling)
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Spherically-symmetric, self-gravitating Schrodinger field
with "annihilation layer" outer boundary conditions.
(1)
mass versus r.
(White: reference, Green: no layer, Red: layer).
Note good agreement between white and red in interior (left)
region.
(2)
mass versus log(r).
(3)
log(dm/dr) = log(psi psi*) versus log(r).
and
(4)
A more detailed view of log(dm/dr) in the layer region.
(Calculations by Reid Guenther.)
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Nick Matlis's spiral wave pattern
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"Boson star in a box". Naive (massless) radiation conditions imposed
on a massive scalar field. Obviously less than ideal, but apparently
pretty stable.
See also my RNPL examples page