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Newtonian derivation of Friedmann equation

  1. Oct 25, 2006 #1
    I'm trying to derive Friedmann's equation for cosmology using Newtonian physics. I've got the force equation F=ma for the case without a cosmological constant. But now I'm trying to incorporate the cosmological constant into this force equation.

    But I'm having trouble seeing how the cosmological constant can appear to apply a force on some particle at the edge of a spherical universe of radius R. I thought that I might get somewhere through dimensional analysis if I could understant the units of the cosmological constant from its use in the Einstein Field Equation where it was initially introduced. But I find I don't know the units of any of the other entities in the EFE - the units for the metric gab or the Ricci tensor or the Ricci scalar or the energy-momentum tensor. Do the units change for different values of ab? It seems everyone likes using elaborate mathematics - and I don't see much practical use - not even dimensional units of the things they talk about. Any help out there? Thanks.
     
  2. jcsd
  3. Oct 25, 2006 #2
    It isn't obvious that what you want to do is even possible. Why don't you do a course on general relativity first (or even just say the track one exercises in Misner, Wheeler & Thorne's book)?
     
  4. Oct 27, 2006 #3
    In the pdf file, starting with page 9, at:

    http://www.astro.caltech.edu/~george/ay21/Ay21_Lecture02.pdf

    the author derives the Friedmann equation from newtonian mechanics using the force produced from the mass density of the universe.

    And at:

    http://en.wikipedia.org/wiki/Cosmological_Constant

    the cosmological constant is expressed in terms of an energy density also as:

    [tex]\[\Lambda = \frac{{8\pi G}}{{c^4 }}\rho vac\][/tex]

    from which we can just as easily derive the Friedmann equation which includes the cosmological constant.

    But I don't know how they got the last equation above. I think it may have something to do with the dimensional analysis of the terms in the Einstein field equations shown below. And I'm hoping someone here knows. Thank you.

    [tex]\[Rab - \frac{1}{2}Rgab + \Lambda gab = 8\pi Tab\][/tex]
     
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