Under what conditions does star bifurcation occur?

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    Bifurcation Star
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Discussion Overview

The discussion revolves around the conditions under which a star might bifurcate, exploring theoretical scenarios and models related to stellar behavior. The scope includes theoretical considerations and alternative models regarding stellar dynamics.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested

Main Points Raised

  • Some participants propose that star bifurcation may occur when a star collides with another massive object.
  • Others suggest that rapid rotation could lead to bifurcation due to centrifugal forces, although this is considered unlikely.
  • A participant mentions that the latter scenario is part of an alternative model aimed at explaining the anomalous distribution of angular momentum in the solar system.
  • Another viewpoint is that the closer an object is to the characteristics of a black hole (in terms of radial density, charge, and angular momentum), the less likely it is to spontaneously bifurcate.

Areas of Agreement / Disagreement

Participants express differing views on the likelihood of bifurcation occurring under various conditions, indicating that multiple competing perspectives remain without consensus.

Contextual Notes

Participants acknowledge the improbability of the scenarios discussed, but the discussion does not resolve the underlying assumptions or dependencies related to the conditions for bifurcation.

Loren Booda
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Under what conditions might a star bifurcate?
 
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Loren Booda said:
Under what conditions might a star bifurcate?
I can only think of:
1. When coliding with another massive object, or:
2. When rotation is so fast that the star is torn apart by centrifugal forces. (unlikely in both cases)
 
Labguy,

Although both cases are highly improbable, the latter figures prominently in an alternative model I've been toying with to explain the anomalous distribution of angular momentum with in our solar system.
 
I believe the more akin an object is to its corresponding black hole (radial density, charge and angular momentum), the less chance it has of spontaneously bifurcating.
 

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