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:::::Yill, your grand total of contributions to this site has been 3 edits to this page, all easily refutable.  Frankly, I don't think greater efforts at "formatting consistency" are justified.--[[User:Aschlafly|Andy Schlafly]] 03:01, 31 March 2010 (EDT)
 
:::::Yill, your grand total of contributions to this site has been 3 edits to this page, all easily refutable.  Frankly, I don't think greater efforts at "formatting consistency" are justified.--[[User:Aschlafly|Andy Schlafly]] 03:01, 31 March 2010 (EDT)
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Yill, you raise excellent points, most of which have not been raised before.  We should sharpen those points, here on this page, and then address them on the actual article page.  This will take a fair amount of discussion.  I could start by bringing up the discussion of point 7, inaccuracy of relativity at the quantum mechanical scale.  One question that was raised was "Is there a discontinuity at that [microscopic boundary] distance? Such an approach is absurd.". No. The way quantum mechanics and classical theories interact at the (microscopic) scales where this happens is well known. It is, of course, generally known as the Bohr correspondence principle, described in any textbook on quantum mechanics, and known in more detail as Ehrenfest's theorem, described in more advanced textbooks. (Very briefly, the quantum mechanical realm eases into the classical realm according to the Ehrenfest theorem.) We should make some citations to those, and put in a careful explanation that, under QM, '''all''' classical theories are incorrect, and QM is the correct theory for everything, from atoms to planets. Classical theories are just extremely good approximations outside of the quantum-mechanical realm. And, of course, we do not know how that quantum-mechanical realm operated immediately after the big bang (that's what inflation theory is about), but that doesn't affect what we ''do'' know about general relativity in the macroscopic realm.
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The item about point 10 is excellent. Gravitons arose ''after GR'', from attempts to unify the theories. They have nothing to do with the macroscopic aspects of GR, which is what GR is actually all about.
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[[User:KrisJ|KrisJ]] 10:04, 31 March 2010 (EDT)
    
== Curavture of Space ==
 
== Curavture of Space ==
    
Re [http://www.conservapedia.com/index.php?title=Counterexamples_to_Relativity&curid=97238&diff=766130&oldid=742826 this] edit: I don't disagree, but the example is a bad one. Based on local observations, one would assume that the Earth itself is flat, but it clearly isn't. My own point of view is that since the Universe can never be proved to be one thing or another, it is part of God's own ineffable being - it is almost folly to inquire further. [[User:RobertE|RobertE]] 18:24, 30 March 2010 (EDT)
 
Re [http://www.conservapedia.com/index.php?title=Counterexamples_to_Relativity&curid=97238&diff=766130&oldid=742826 this] edit: I don't disagree, but the example is a bad one. Based on local observations, one would assume that the Earth itself is flat, but it clearly isn't. My own point of view is that since the Universe can never be proved to be one thing or another, it is part of God's own ineffable being - it is almost folly to inquire further. [[User:RobertE|RobertE]] 18:24, 30 March 2010 (EDT)
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