Question.
There are some who claim that DE as a scalar field resolves the "
missing mass " problem, but as the DE force is repulsive how could that
account for galactic cohesion which is attractive?
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Haelfix - 25 Nov 2004 09:39 GMT
Good question, simple answer. DE is strong on extragalactic scales,
gravity completely swamps it at the local galactic and say everyday
life scale.
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TillEulenspiegel - 25 Nov 2004 09:39 GMT
So then you think that DE would follow sort of an inverse of Newtons
square of the distance or it is a scaler field ( as I believe) where
the gradient doesn't change , but is rather static. Even a small force
differential at great distances would have an effect over the age of
the universe? I.E. The fact that the outer bodies are accelerating
because the FGrav is less over greater distances.
That still doesn't account for the cohesive behavior of Galaxy's. With
the mass we measure they should fly apart. So there must be something
we cannot see of measure ATT. CDM or HDM. The invocation of DE can
solve the overall energy budget, but can't account for missing mass at
close distances.
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Uncle Al - 26 Nov 2004 07:18 GMT
> Question.
> There are some who claim that DE as a scalar field resolves the "
> missing mass " problem, but as the DE force is repulsive how could that
> account for galactic cohesion which is attractive?
You are confusing curve fitting for spiral galaxy persistence (dark
matter, attraction) with curve fitting for excess universal expansion
(dark energy, repulsion). There comes a time when adding more
epicycles (perturbative approaches) is less attractive than
formulating better overall theory.

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