THE MALTA COSMOLOGY TEMPLATE

Chapter 3 - Blackholes

PARTS

Part 4 - Blackhole Mechanics

ARGUMENT 0321

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

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