THE MALTA COSMOLOGY TEMPLATE



Chapter 3 - Blackholes






PARTS



Chapter
Home


Part 1
Teelpairs


Part 2
Blackholes


Part 3
Blackhole structure


Part 4
Blackhole mechanics


Part 5
Blackhole selfstabilisation


Part 6
Blackhole gravitational attunement


Part 7
Blackhole teelospheric attunement


Part 8
Selfproof

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Part 1 - Teelpairs (cont)

ARGUMENT 0310

BROUGHT FORWARD:
  • ARGUMENT 0307: Every adjacent teelpair's gravitysheath is surrounded by a gravitysheath interface.
  • ARGUMENT 0308: Every adjacent teelpair has a vergence velocity.
  • ARGUMENT 0309: Every adjacent teelpair has an escape velocity.
REASONING:
  • At the gravitysheath interface of an adjacent teelpair, the escape velocity is always zero but the vergence velocity is a variable.
  • The vergence velocity can be the same as the escape velocity, or lower, or higher.
  • Arising from this, three forms of adjacent teelpair are possible:

    • FORM 1:   When the vergence velocity is lower than the escape velocity, the teelpair is overstable. As long as the vergence velocity remains lower than the escape velocity, the adjacency continues.
    • FORM 2:   When the vergence velocity is the same as the escape velocity, the teelpair is stable. As long as the vergence velocity remains the same as the escape velocity, the adjacency continues.
    • FORM 3:   When the vergence velocity is higher than the escape velocity, the teelpair is understable. Unless the vergence velocity is lowered to the same as, or less than, the escape velocity, the adjacency cannot continue.
CONCLUSION:
  • An adjacent teelpair is either overstable, stable, or understable.

GLOSSARY:  
  • overstable:   An object is overstable when its vergence velocity is lower than its escape velocity.
  • stable:   An object is stable when its vergence velocity is the same as its escape velocity.
  • understable:   An object is understable when its vergence velocity is higher than its escape velocity.





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Copyright 2013 Peter (Ed) Winchester