THE MALTA COSMOLOGY TEMPLATE

Chapter 3 - Blackholes

PARTS

Part 4 - Blackhole Mechanics (cont)

ARGUMENT 0322

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

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