Planck - stelactic - cosmological black hole symmetry?

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Discussion Overview

The discussion explores the concept of concentric black holes, specifically focusing on the relationships between stelactic, Planck, and cosmological black holes. It delves into theoretical implications, potential symmetries, and the nature of black holes in the context of the universe's structure and early formation.

Discussion Character

  • Exploratory, Conceptual clarification, Debate/contested

Main Points Raised

  • One participant suggests that stelactic black holes mediate a symmetry between Planck and cosmological black holes, proposing a duality based on their event horizons and the nature of Hawking radiation.
  • Another participant questions whether there is a critical mass that differentiates stellar from galactic black holes and how this differentiation might have originated in the early universe.
  • A participant expresses excitement about the idea of concentric black holes and requests further information or references.
  • One participant posits that the observable universe may have a mass-radius ratio conducive to being a black hole, suggesting that conventional stelactic black holes could have central singularities resembling those of Planck black holes.

Areas of Agreement / Disagreement

Participants exhibit a mix of curiosity and speculation, with no clear consensus on the relationships or characteristics of the black holes discussed. Multiple competing views remain regarding their nature and implications.

Contextual Notes

The discussion includes speculative ideas about black hole symmetries and relationships, with assumptions about mass and density ratios that are not fully explored or defined. The implications of these concepts on cosmology and black hole physics remain unresolved.

Loren Booda
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Like nested dolls, these black holes appear coexisting concentrically where the central stelactic (stellar-galactic) black hole mediates a symmetry between the other two.

For instance, consider how stelactic Hawking radiation manifests under inversion of its event horizon. The events within this horizon are, upon inversion, gravitationally-reversed (a la dark energy), with the Planck ("singularity") and cosmological ("Hubble") black holes exhibiting duality.

Can you see more significant interrelationships amongst them, other than they are black holes?
 
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Is there a critical (mass) demarcation between stellar and galactic black holes, and how might this differentiation have arisen in the early universe?
 
Wow, concentric black holes, that is certainly news to me and is very exciting. Got a link please?
 
It just seems to make sense to me. The observable universe is on the order of the right mass-radius ratio to be a black hole, wherein exist "conventional" stelactic black holes whose central "singularities" themselves are of maximal density, perhaps a composite like that characteristic of Planck black holes.
 

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