- #36
Nereid
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Hmm, perhaps a short course in modern cosmology would help? Ned Wright's tutorial is a good place to start.Ivan Seeking said:When I referred to the expected shift, what I meant was the red shift we would get were DE and DM not an influence.
wrt DE: AFAIK, there are only two sets of observations for which DE is introduced ... distance Ia SN, and the CMBR (esp the WMAP data). In the former, you can make a good case that it's still early days ... too many loose ends, systematic effects not well characterised, theoretical models not constrained enough (e.g. variations on WD detonation). In the latter, DE is like the icing on the cake - the concordance model fits the WMAP data pretty well without DE in the picture, but better with it in.
wrt DM: there are several types of independent observation - mutually consistent - which lead you to a 'there exists DM' conclusion; several of these involve your common garden variety redshift - doppler. The need for DM in cosmology is weaker than the need for DM in more 'local' astrophysics ... so if you choose to ditch DM in your cosmology, you have just added the headache of accounting for lots and lots more 'local' observations!