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"Joseph Lazio" <[EMAIL PROTECTED]> wrote in message news:[EMAIL PROTECTED] > >>>>> "DL" == Denis Loubet <[EMAIL PROTECTED]> writes: > > DL> "Jack Sarfatti" <[EMAIL PROTECTED]> wrote in message > DL> news:[EMAIL PROTECTED] > >> "I think we are so confused that we should keep an open mind to > >> tinkering with gravity," said Dr. Michael Turner, a cosmologist at > >> the University of Chicago. > >> > >> http://www.nytimes.com/2003/11/11/science/11GRAV.html > >> previously > >> > >> Q to Ed Witten: How can the cosmological constant be so close to > >> zero but not zero? > > DL> "Close to zero"? WTF does "close" mean? Is there a "maximum value" > DL> we can compare it to to see how "close" it is? > > The current estimates are that the energy density contributed by the > cosmological constant (or dark energy) is 0.7, in units of the closure > energy density. There are various models of particle/high-energy > physics that make predictions about the cosmological constant. The > typical value predicted is 10^50 or so. Excellent! Thank you. (I'm going to pretend to understand that.) ;-) -- Denis Loubet [EMAIL PROTECTED] http://www.io.com/~dloubet
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