SELFPROOF 0304
- EXTREMAL BLACKHOLE
CURRENT COSMOLOGY MODEL
An
extremal blackhole is a blackhole with the minimal possible mass that
can be compatible with a given charge and angular momentum. In other
words, this is the smallest possible blackhole that can exist while
rotating at a given fixed constant speed. The concept of an extremal
blackhole is theoretical and none have thus far been observed in
nature. However, many theories are based on their existence.
(Wikipedia 24 Jan 2012)
MALTA COSMOLOGY TEMPLATE
- A blackhole consists of a minimum of three teels matrixed to each other as three stable/overstable teelpairs. (see Argument 0312)
- Every blackhole has a vergence velocity. (see Argument 0315)
- Every blackhole has an escape velocity. (see Argument 0316)
- A blackhole is either overstable, stable, or understable. (see Argument 0317)
- The
degree of a blackhole's overstability or undestability changes
commensurately with any change in its vergence velocity and/or escape
velocity.
- Blackholes are solidbonded, liquidbonded, or
gasbonded depending on the stability condition of their adjacent
teelpairs. (see Argument 0319)
- Blackholes
of sufficient mass stratify their teelpairs according to their energy
measure into a central solidbonded teelcore, surrounded by a
liquidbonded teelocean, surrounded by a gasbonded teelosphere.
(see Argument 0320)
COMMENTARY
In
the extremal blackhole concept, for a given spinrate there is a mass
measure below which a blackhole cannot endure. This is true, viz:
- Relative to something, the solidbonded teelcore of a blackhole always spins (rotates).
- The
teelocean and/or teelosphere of a blackhole may spin sympathetically
with the teelcore or may be chaotic to a greater or lesser
degree.
- The spinrate of a blackhole conditions both its vergence and its escape velocity in a multiprocess.
- An
increase in spinrate triggers a commensurate increase in vergence
velocity (because the realspeed of the blackhole's teels has increased).
- An
increase in spinrate triggers a commensurate decrease in escape
velocity (because the density of the teels in the blackhole has
decreased).
- A decrease in spinrate affects the vergence velocity and the escape velocity conversely.
- In a stable blackhole, an increase in spinrate will be accompanied by a decrease in mass.
- In
a stable blackhole, a decrease in spinrate will be accompanied by an
increase in mass, subject to the availability of teels from beyond the
blackhole's gravitysheath interface.
- In an overstable
blackhole, an increase in spinrate will not trigger an alteration
in mass until the blackhole becomes understable.
- In an overstable blackhole, a decrease in
spinrate will be accompanied by an increase in mass, subject to the
availability of teels from beyond the blackhole's gravitysheath
interface.
- In an understable blackhole, an increase in spinrate
will commensurately increase the rate at which the mass is already
decreasing.
- In an understable blackhole, a decrease in
spinrate will commensurately decrease the rate at which the mass is
already decreasing.
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