THE MALTA COSMOLOGY TEMPLATE

Chapter 3 - Blackholes 

PARTS

Part 4 - Blackhole Mechanics (cont)

ARGUMENT 0323

• ARGUMENT 0315: Every blackhole has a vergence velocity.
• ARGUMENT 0316: Every blackhole has an escape velocity.
• ARGUMENT 0320: 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.

• Arising from the above arguments, three forms of teelosphere are possible:
  
  
  • FORM 1: When the vergence velocity is lower than the escape velocity, the teelosphere is overstable. As long as the vergence velocity remains lower than the escape velocity, the teelosphere continues to be overstable.
  • FORM 2: When the vergence velocity is the same as the escape velocity, the teelosphere is stable. As long as the vergence velocity remains the same as the escape velocity, the teelosphere continues to be stable.
  • FORM 3: When the vergence velocity is higher than the escape velocity, the teelosphere is understable. Unless the vergence velocity is lowered to the same as, or less than, the escape velocity, the understability continues until the teelosphere has dissipated.

• Within a blackhole, its teelosphere is either overstable, stable, or understable.