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In article ,
Yousuf Khan writes: Well, before there was Dark Energy, there was a model that fit the data too. That was the hot Dark Matter model, where the place of Dark Energy was filled by neutrinos. By "before," you mean pre-COBE? There are a lot of new data since then. If future data disagree with current models, the models will have to change. That's how science works. -- Help keep our newsgroup healthy; please don't feed the trolls. Steve Willner Phone 617-495-7123 Cambridge, MA 02138 USA |
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On Wednesday, November 2, 2016 at 5:31:44 AM UTC-7, Jeff-Relf.Me wrote:
You still have to explain why the expansion doesn't=20 slow down due to the gravity of everything it contains. =20 Expansion does slow down because of gravity. That's put into the equations via Omega_M. See Ned Wright's cosmology calculator http://www.astro.ucla.edu/~wright/CosmoCalc.html and its tutorial and glossary. In article , dlzc writes: Saying Dark Energy, something that is uniformly distributed across the Universe at each epoch, and yet varies with time (at least between the Big Bang Event and now), isn't a model I can wrap my head around, yet. Nobody knows what Dark Energy is or whether it varies in time. There are now upper limits on time variation, but that should be measured much better in the next several years, so stay tuned. If Dark Energy is a cosmological constant, it won't vary with time (in proper coordinates). If it is something else, then it might vary. It's also conceivable that Dark Energy could vary with position, but I doubt details will be worked out until there's a serious chance of observing that possibility. Or maybe the working out has been done but not publicized because of the difficulty of observational tests. -- Help keep our newsgroup healthy; please don't feed the trolls. Steve Willner Phone 617-495-7123 Cambridge, MA 02138 USA |
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On 11/7/2016 5:43 PM, Steve Willner wrote:
In article , Yousuf Khan writes: Well, before there was Dark Energy, there was a model that fit the data too. That was the hot Dark Matter model, where the place of Dark Energy was filled by neutrinos. By "before," you mean pre-COBE? There are a lot of new data since then. If future data disagree with current models, the models will have to change. That's how science works. No, not pre-COBE, COBE data was already around, supernova data came around later, and then they changed the interpretation of COBE & WMAP data to fit the Dark Energy hypothesis. Yousuf Khan |
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