Re: Analyse This!
- From: "Ahmed Ouahi, Architect" <ahmed.ouahi@xxxxxxxxx>
- Date: Fri, 18 Aug 2006 01:23:12 +0300
Unfortunately or a fortunately, for the time being, a spacetime is usually a
manner to try to see as to try to figure out, anything which it should be a
flat but however, a pliant matter, on which would be a resting an heavy
round object, as, for instance, an iron ball.
Therefore, a weight of an iron ball would eventually cause a material on
which it would be sitting to stretch slightly.
However, it would be this, which it should be a roughly analogous along an
effect, that any mass of an any object, for instance the Sun itself has on a
spacetime along which it would strech and absolutely curve, and this is what
is all about.
--
Ahmed Ouahi, Architect
Best Regards!
"me" <ililililil@xxxxxxxxxxxx> wrote in message
news:1155850286.580415.31770@xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
something called the
Igor wrote:
me wrote:
Igor wrote:
me wrote:
Tom Roberts wrote:
Ahmed Ouahi, Architect wrote:
More or less reflexively, he dropped into his equations
effects ofcosmological constant, which arbitrarily counterbalanced the
lapse, but itgravity, serving as a kind of mathematical pause button.
Books on the history of science always forgive Einstein this
it. He calledwas actually a fairly appalling piece of science and he knew
Thinkingit ' the biggest blunder of my life '. "
From today's perspective this was not a blunder at all.
thatabstractly, one cannot eliminate from the Lagrangian any terms
derivativessatisfy the symmetries required of the theory (chiefly general
covariance). If one restricts the terms to those with no
fieldhigher than the second, and requires linearity in those second
derivatives, one obtains the Lagrangian that yields the Einstein
non-trivialequation, with cosmological constant. It is the simplest
theLagrangian that obeys the necessary symmetries.
It is, of course, up to experiments to determine the value of
"quitecosmological constant. Until rather recently, the value was
measure itsmall, consistent with zero"; with improved techniques we now
theto be nonzero. Einstein originally favored zero, because then
however,Newtonian limit comes out correct; with a very small value,
fact,deviations from Newtonian mechanics would not be detectable.
Tom Roberts
if it is consistent with zero, who is expanding the universe
thank you for this email
You don't need a cosmological constant to provide expansion. In
it.Einstein originally used it to pull the universe back together, but
whay, was the gravity not strong enuff?
Not strong enough to maintain a static universe that wasn't expanding.
when the universe was found to actually be expanding,.he discarded
universeOr haven't you been paying attention?
is it pushed from inside or is it pulled from outside?
It's the result of the big bang.
from inside or from outside?
No inside or outside on a manifold. There's just spacetime. The
actual "shape" of that manifold is what has always been debated.
this because there should be more vacum and empty space
outside than it is here inside
Where's this outside that you're talking about? GR models the
expansionas an open or closed spacetime manifold. There is no outside.
i tell you what, is somthing bigbang is exploding then
expanding, it does it against the outside
an imploding and contraction does it against inside
dont you know it? where have you been?
You don't know what you're talking about. Tell me where the inside and
outside are on the surface of a sphere. They don't exist. All you
have is the surface. Think of it in those terms. A spacetime manifold
is somewhat analagous to this, except in 4 dimensions instead of the 2
dimensions on the sphere.
thank you for this new e-mail
apparently you make things clear for me,
but still,
this surface to universe analogy went too
far, everybody use it, even reporters and
moviemakers, and obviously thay dont
know what they are talkin aboit
whay using a 2d surface analoguous to
a 4d manifold
whay not using 3d analogous to 4d
another question I have is about the big bang
if by using powerful telescopes
1. we can detect the primitive bigbang light and radiation
2. we can detect that everywhere in 3D
3. the distance to the bigbang light is increasing because
the
are we inside the bigbang now?
In a sense. We see the effects of the big bang all around us, but
thetemperature of the universe has cooled to just under 3 K.
thanks, now that you agree with inside, then an outside must
exists
Depends on whether you are talking about 3 dimensions of 4. In 3
dimensions, we appear to be inside something, but that space is not the
total picture and is emnbedded in 4 dimensional spacetime, where the
is it a rank 3 tensor with 4 elements?
universe is a self-contained manifold. No inside or outside. Now, you
might be able to come up with a theory where spacetime were embedded in
higher dimensions, but it would not be GR.
only a holywood filmmaker would do that
because if we reverese the expantion, then we have no choice, but
being inside the bigbang
That's called the big crunch, essentially running the big bang in
reverse. It was once thought that it might be the ultimate fate of
theuniverse if there was sufficient total mass for gravity to overcome
thatoutward expansion and pull everything back together again. But it
doesn't look like it will happen due to the accelerated expansion
we now see.
what is better, to expand or to impand?
Impand is not even a word. Why am I wasting my time?
no, you dont, you make things more clear to me, thanks
.
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