Universe expansion -> t = - inifinite

AI Thread Summary
The discussion centers on the expanding universe and its implications for cosmology, particularly regarding the concept of time and the universe's diameter. It explores the idea that the universe's expansion has not always accelerated, as suggested by the LambdaCDM model, which indicates a prior phase of deceleration. Participants debate the nature of the universe's initial state, suggesting it was not a singular point but a concentrated mass, and emphasize the importance of using computer models to understand cosmic evolution. The conversation also touches on the differences between cosmological models like FRW and de Sitter lambdavacuum, questioning their predictive power regarding future expansion or contraction. Ultimately, the discussion seeks to clarify complex concepts for better understanding while acknowledging the need for further study.
JPC
Messages
204
Reaction score
1
hey

Was thinking
since the universe is actually expanding at an increasing speed
We can ask the question : how did all the matter+energy get reunite in one small point ?

well, can we just say that if we consider , 't' : time :
t=-infinite : the beginning of everything
t = 0 : today
t = +oo : the end of everything.

That if 'd' the diameter of the universe at a time t

Lim -oo (d) = 0
lim +oo (d) = +oo

Meaning, that its all about limits
 
Space news on Phys.org
JPC said:
since the universe is actually expanding at an increasing speed

according to the standard (LambdaCDM) model that cosmologists mostly use, the universe has NOT ALWAYS been accelerating its expansion

for a long time (billions of years) the expansion was slowing down and the Hubble rate was decreasing

so what you see now does not tell you that it has always been doing that
=======================

a lot of work going on now is about models that have not always been expanding.

in these models there is a before-the-big-bang contraction phase and an abrupt turnaround when a critical density was reached (near the socalled Planck density)

It wouldn't have been actually a "point" as people used to imagine, but just very concentrated

If you want links to the technical papers, just say.
========================

the point is that just because at present it is doing such-and-such doesn't mean we can extrapolate back assuming that it has always

it's better to use a computer model with some quantum law of gravity built in, and actually run it backwards and see what happens-------or to use a equation model with solvable equations
either way you may find that there is a turnaround (gravity acting different at very high density)
 
Last edited:
but if D = F(t)
where D : diameter of the universe (aprox)
t : time

what are the variations of the function f ?
- always increasing, (with or without constant at some intervals) : (french : croissant) ?
- Increasing, then decreasing ?
- other ?

and what are the limits of f(x) at :
- infinite and + infinite ?
 
No one really knows exactly ?
 
Shouldn't this be in the Cosmology forum?

I think you have misunderstood careless references to "diameter of the universe", which doesn't mean what (almost certainly) you think: a more correct term is scale parameter.

Of course the time dependence of the scale parameter in the FRW lambdadusts is known (as a function of proper time as measured by the dust particles). See the last chapter of the excellent undergraduate textbook by D'Inverno for the answers you seek. You can look for old sci.physic.* posts by myself discussing in detail FRW dusts with nonzero Lambda. In some cases this parameter is most conveniently expressed parametrically but in the case of flat hyperslices it can be easily written as an explicit function of "time".

More important: if you "run time backwards" in the FRW models you come to an initial time, which we call the Big Bang. (In some special cases the same thing happens if you run time forwards, except we call that the Big Crunch.) There are some other cosmological models, such as the de Sitter lambdavacuum, in which one can "run time backwards" indefinitely. It is possible to analyse the global structure of cosmological models such as FRW models and de Sitter lambdavacuum using methods pioneered by Penrose and others. See for example Hawking and Ellis, The Large Scale Structure of Space-Time, Cambridge University Press, 1973.
 
Last edited:
Oh, yes maybe this post should be put in cosmology, but now that its posted the forum won't let me change its location.

Thanks for all the references you have given me, but I am just a 12th grade student in a French semi-International Scientific section, i don't want to get lost in High level explanations until i reach the scientific level.

Im just looking for simple explanations for a general understanding. I will be looking for the details latter in my post-school studies.

---------------------------------------------------------------------

but which model as more proof, justification :
- FRW or de Sitter lambdavacuum ?

Right now the universe is expanding at an increased rate.
Is it because of black matter with a negative mass that acts as a expansion force ?

And if the Universe is accelerating, how does FRW explain that the universe will come back together in a big crush ?
 
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
The formal paper is here. The Rutgers University news has published a story about an image being closely examined at their New Brunswick campus. Here is an excerpt: Computer modeling of the gravitational lens by Keeton and Eid showed that the four visible foreground galaxies causing the gravitational bending couldn’t explain the details of the five-image pattern. Only with the addition of a large, invisible mass, in this case, a dark matter halo, could the model match the observations...
Hi, I’m pretty new to cosmology and I’m trying to get my head around the Big Bang and the potential infinite extent of the universe as a whole. There’s lots of misleading info out there but this forum and a few others have helped me and I just wanted to check I have the right idea. The Big Bang was the creation of space and time. At this instant t=0 space was infinite in size but the scale factor was zero. I’m picturing it (hopefully correctly) like an excel spreadsheet with infinite...
Back
Top