Black hole event horizon as surface of spacetime symmetry

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SUMMARY

The discussion centers on the relationship between black hole event horizons and spacetime symmetry, emphasizing that the spacetime geometry outside a black hole can transform through the event horizon into the internal geometry of the black hole. It highlights the conservation of entropy in relation to Hawking radiation, where one quantum escapes while another approaches the singularity. The event horizon serves as a mirror symmetry point, inverting universal spacetime to actualize black hole spacetime. The proportionality of horizon surface area to black hole entropy is affirmed from both external and internal perspectives.

PREREQUISITES
  • Understanding of black hole thermodynamics, particularly Hawking radiation.
  • Familiarity with concepts of spacetime geometry and singularities.
  • Knowledge of entropy conservation in physical systems.
  • Basic grasp of relativistic physics and event horizons.
NEXT STEPS
  • Research the implications of Hawking radiation on black hole entropy.
  • Explore the mathematical framework of spacetime geometry around black holes.
  • Investigate the concept of relative velocity effects on event horizons.
  • Study the relationship between entropy and surface area in black hole physics.
USEFUL FOR

The discussion is beneficial for theoretical physicists, astrophysicists, and students interested in advanced concepts of black hole mechanics and spacetime theories.

Loren Booda
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The spacetime geometry outside a black hole may be transformable through the event horizon as the black hole internal geometry, and conversely.

Consider Hawking radiation with respect to black hole entropy. While one quantum escapes to universal infinity, the other approaches the corresponding infinitesimal singularity. Entropy is always conserved between opposite horizons, thermally isolated, singularity and Hubble area. The event horizon represents their mirror symmetry, at which the universal spacetime inverts to actualize the black hole spacetime and reciprocate the relative surface curvature. The hole itself, surrounded by the entropic cosmos, is thus anentropic in character. The relation that horizon surface area is proportional to black hole entropy holds for both perspectives, either outside or within the hole.

Please refer to my second and third articles at http://www.quantumdream.net
 
Last edited by a moderator:
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Greetings !

Hmm... This indirectly made me think of something:
The EH is actualy a relative feature, isn't it ?
basically, the greater your velocity relative to the
BH the EH will "retreat" towards the singularity
on one "side" until your velocity gets infitesimally
close to c and you can almost get a "glimpse" of it.
Right ?

Sure would be an interesting way to study BHs...:wink:

Live long and prosper.
 
Almost, drag, but remember that singularities are awfully bashful!
 

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