THE MALTA COSMOLOGY TEMPLATE

Chapter 5 - Darkmatter

PARTS

Part 1 - Centrifugal Blackholes (cont)

ARGUMENT 0507

• ARGUMENT 0323: Within a blackhole, its teelosphere is either overstable, stable, or understable.
• ARGUMENT 0326: Within a blackhole, an understable teelosphere loses mass and energy into the teelocean and across the gravitysheath interface while an overstable teelosphere gains mass and energy from the teelocean and across the gravitysheath interface.
• ARGUMENT 0506: The default flow pattern for a blackhole teelosphere is centrifugal with low level teels streaming toward the equator and high level teels streaming toward the poles.

• In a centrifugal teelosphere, the teels with the greatest totalspeed are above the blackhole's teelcore equator.
• This region is the blackhole's teelospheric equator.
• If the blackhole is understable, the teelospheric equator is the principal ejection point for excess teels.

• In a centrifugal blackhole, the principal point for the ejection of teels across the gravitysheath interface is the teelospheric equator.

• teelospheric equator:   The principal teel ejection point in the teelosphere of a centrifugal blackhole. It is a circumferential line dividing the blackhole's two equal hemispheres. It is usually but not necessarily above the blackhole's teelcore equator.