Recent content by Quantizer

  1. Q

    Boundaries of Time in The Evolution of The Universe

    The reason why I ask is in relation to recent posts on this thread ... What physical processes can cause a DeSitter Contraction to kick in an already expanding DeSitter Phase very far in the future of the Universe, thanks
  2. Q

    Boundaries of Time in The Evolution of The Universe

    Good answer, can there exist conditions, a specific scenario whereby dark energy or equivalent repulsive forces causing expansion to become zero in the very far future post Hawking Radiation Era, such that there is no increase in degrees of freedom in any variable, only then can we achieve...
  3. Q

    Boundaries of Time in The Evolution of The Universe

    Entropy is increasing due to 2nd Law of Thermodynamics towards Thermodynamic Equilibrium of Maximum Entropy ...
  4. Q

    Boundaries of Time in The Evolution of The Universe

    However, beyond the Black Hole era, post Hawking Radiation, there should be near nothing to decay, and there is nothing but near emptiness, how can Entropy increase unbounded, if there is nothing to propagate further disorder, surely Entropy must reach a maximum, and does this happen as the...
  5. Q

    Boundaries of Time in The Evolution of The Universe

    Given The Hawking-Hartle state is an initial state of the very early universe If the universe very far in the future asymptotically approaches 0K, what is the name of this final state of Maximum Entropy Does time stop at Maximum Entropy final state of the universe Given the assumption that...
  6. Q

    DeSitter and AntiDeSitter Universe

    Thanks for that Mordred, a few pages in and already intrigued by some of the astronomical exponentials being put forward
  7. Q

    DeSitter and AntiDeSitter Universe

    Q2 Are there any scenarios for an AntiDeSitter Model in the chronology of the Universe
  8. Q

    DeSitter and AntiDeSitter Universe

    Q1 What Einstein model currently describes a Homogeneous and Isotropic approximated Universe with Matter with positive Lambda, is it still Friedmann (FLRW) or have models moved on Which Einstein model describes an Inhomogeneous and Anisotropic very early universe with primordial density...
  9. Q

    DeSitter and AntiDeSitter Universe

    If the DeSitter Universe is modeled by Empty Universe 1. Very Early Universe with Inflaton Field 2. Very Far Universe in Future when Black Holes have evaporated
  10. Q

    Best Numerical Analysis Software for Physics

    Numerical Analysis of - Einstein Field Equations - Schrodinger Equations As a starter and graphs of solutions
  11. Q

    Best Numerical Analysis Software for Physics

    Two criteria 1. Freely Available 2. Large support for additional scientific libraries/packages/modules for reuse http://en.wikipedia.org/wiki/Comparison_of_numerical_analysis_software Which one would you recommend and why?
  12. Q

    Quantum Vacuum and Quantum Foam

    Indeed, every action has a reaction If Spontaneity is the reaction what is inducing it ... Will dig further into this ... Thoughts anybody is there a certain type of vacuum that is yet to be explored Given that we already have Classical Vacuum QED Vacuum QCD Vacuum LQG Vacuum
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    Quantum Vacuum and Quantum Foam

    Ok thanks, still would like to research this area, as I would like to understand the relationship or even an approach to the subject area, any good starting points would be appreciated Ie what physical process triggers virtual particles to appear out of a ZPE field I'm already aware of...
  14. Q

    Quantum Vacuum and Quantum Foam

    Ok so we perceive Quantum Foam as Quantised SpaceTime at Planck Scales that spawns virtual particles hence explaining why we have additional energy over and above ZPE
  15. Q

    Quantum Vacuum and Quantum Foam

    Ok Simon thanks, if QV is represented by ZPE lowest ground state, then how do you get the high energies at QV by probing it at QF scales
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