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Inflation of singularity at moment of evaporation?

  1. Mar 16, 2013 #1
    I have had an idea kicking around in my head for some time now. It all started last summer when I was kayaking down a river and I had stopped in an eddy to relax for a moment. The rate of flow of the water was strong enough to make sizable vortices along the eddy fence around the boulder that was creating the eddy in which I was resting. These vortices reminded me of the similar way in which spacetime is curved into a singularity. Long story short; black holes have been on my mind for almost a year now. I have progressed my understanding through the formation and into the evaporation of the singularity. The fact that some matter/information is lost during the evaporation perplexes me. This does not make sense to me. My suspicion is that when the mass of the singularity reaches a point in which it no longer exceeds the Tolman-Oppenheimer-Volkoff limit the singularity becomes unstable and the remaining mass, which would have been converted to energy by the force of infinite gravity, inflates into a new dimension/universe. This is just an idea of mine. Any input and discussion would be appreciated.
     
  2. jcsd
  3. Mar 16, 2013 #2

    Chronos

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    The singularity problem is largely resolved by LQG. Not that it is a particular attractive, solution, but, a good starting point. The extra dimensions thing appears to be unnecessary background noise, IMO.
     
  4. Mar 16, 2013 #3

    martinbn

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    Chronos, how does LQG solve the singularity problem?
     
  5. Mar 16, 2013 #4
    I do not feel that LQG correctly solves for a singularity. I have not been able to find a concrete solution that could anyway. I would like to see how it does. As far as I can tell, through quantum mechanics, it could be possible for a singularity to inflate into its own dimension. Please correct me if I am wrong.
     
    Last edited: Mar 16, 2013
  6. Mar 16, 2013 #5
    http://en.m.wikipedia.org/wiki/Nikodem_Popławski

    The link above is in regards to the Poplawski. He is a cosmologist that wrote a torsion based model of a universe inside every blackhole. Although I personally do not agree with his model it may interest you.

    His model has two problems I have read counter papers about.
    1) it does not explain early large structure formation.
    2) Does not explain the CMB homogeneous and isotropic measurements.
     
  7. Mar 16, 2013 #6

    Chronos

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    There are a number of approaches in LQG that are singularity free - e.g.,
    A no-singularity scenario in loop quantum gravity, http://arxiv.org/abs/1206.5765
     
  8. Mar 17, 2013 #7
    Mordred- I have seen his stuff before and I do not agree with his work either. Thank you for your reply, however.

    Chronos- Thank you for the link. It looks most interesting.
     
  9. Mar 20, 2013 #8
    Perhaps the spin of a singularity can exceed its gravimetric attraction (at the edge of rotation) making the singularity 'evaporate'? - mini black holes
     
  10. Mar 20, 2013 #9

    Chronos

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    Actually, an event horizon cannot spin fast enough to overcome the gravity of its singularity. It can, however, flatten out to become a Kerr-Newman black hole.
     
  11. Mar 21, 2013 #10
    Then its Hawking Radiation?

    So supposely Hawking Radiation is responsible for the evaporation in mini-blackhole.?
    .
    How would a Kerr-Newman black hole affect this?
     
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