THE MALTA COSMOLOGY TEMPLATE

Chapter 3 - Blackholes

PARTS

Part 3 - Blackhole Structure (cont)

ARGUMENT 0320

• ARGUMENT 0319: Blackholes are solidbonded, liquidbonded, or gasbonded depending on the stability condition of their adjacent teelpairs.

• Increasing the mass of a blackhole allows teels with the least spinspeed to sink to the centre and those with the most to rise to the surface.
• Arising from this, blackholes have three distinct strata forms:
  
  
  • FORM 1:   Teels with the least spinspeed form overstable and stable teelpairs and sink to become a blackhole's solidbonded teelcore.
  • FORM 2:   Teels with more spinspeed form a mix of overstable, stable, and understable teelpairs surrounding the teelcore to become the blackhole's liquidbonded teelocean.
  • FORM 3:   Teels with yet more spinspeed form understable teelpairs surrounding the teelocean as the blackhole's gasbonded teelosphere. 

• Teels with yet more spinspeed escape across the blackhole's gravitysheath interface.

• 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.

• teelcore:   The matrix of solidbonded teelpairs at the centre of a blackhole. 

• teelocean:   The stratum of liquidbonded teelpairs that may surround the teelcore of a blackhole. 

• teelosphere:   The stratum of gasbonded teelpairs that may surround the teelcore/teelocean of a blackhole.