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The idea that universes somehow 'evolve' stems naturally from this.It doesn't take all that much to create a universe. Resources on a cosmic scale are not required. It might even be possible for someone in a not terribly advanced civilization to cook up a new universe in a laboratory. Which leads to an arresting thought: Could that be how our universe came into being?
"When I invented chaotic inflation theory, I found that the only thing you needed to get a universe like ours started is a hundred-thousandth of a gram of matter," Linde told me in his Russian-accented English when I reached him by phone at Stanford. "That's enough to create a small chunk of vacuum that blows up into the billions and billions of galaxies we see around us. It looks like cheating, but that's how the inflation theory works—all the matter in the universe gets created from the negative energy of the gravitational field. So, what's to stop us from creating a universe in a lab? We would be like gods!"
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"You might take this all as a joke," he said, "but perhaps it is not entirely absurd. It may be the explanation for why the world we live in is so weird. On the evidence, our universe was created not by a divine being, but by a physicist hacker."
Linde's theory gives scientific muscle to the notion of a universe created by an intelligent being. It might be congenial to Gnostics, who believe that the material world was fashioned not by a benevolent supreme being but by an evil demiurge. More orthodox believers, on the other hand, will seek refuge in the question, "But who created the physicist hacker?" Let's hope it's not hackers all the way up. - The Big Lab Experiment
But then Linde thought of another channel of communication between creator and creation—the only one possible, as far as he could tell. The creator, by manipulating the cosmic seed in the right way, has the power to ordain certain physical parameters of the universe he ushers into being. So says the theory. He can determine, for example, what the numerical ratio of the electron's mass to the proton's will be. Such ratios, called constants of nature, look like arbitrary numbers to us: There is no obvious reason they should take one value rather than another. (Why, for instance, is the strength of gravity in our universe determined by a number with the digits 6673?) But the creator, by fixing certain values for these dozens of constants, could write a subtle message into the very structure of the universe. And, as Linde hastened to point out, such a message would be legible only to physicists.
If the singularity at the centre of a black hole lies in the future, representing a final state, the singularity of a white hole lies in the past, as a beginning, as in the big bang. So if our universe is a white hole, the big question is: is there a black hole universe on the other side of the big bang? - more on this hereSo, you've spawned your baby universe in your massively expensive laboratory, but you are worried it will off-set the balance of nature (the first law of thermodynamics)? What if that first law could be balanced both in and outside the system we understand as this universe?
My question:How do astronomers account for the temporal distinctiveness of their galactic subjects in their calculations? I understand that observations of the red shift of quasars delinates a speed increase in the expansion of the universe - yet my brain explodes when I try to understand how the enormous expanse of time is factored into these models.Answers:
The hardest concepts for me to conceive are ones that factor the enormous AGE of the universe into their workings. I understand that by observing quasar red shift and comparing it to the shift of 'nearby' galaxies astronomers have determined that universe expansion is actually increasing. Surely though the fact that these quasar entities exist 'back in time' alters the nature of the data streaming from them? The photons of light astronomers gather in their observations have not just travelled great distances of space, but also great expanses of time, yet when the light was first emitted from these 'distant' objects their distinction in space was not as great as it is now (i.e. when the universe was smaller) a weird conflict indeed... This is where I reach the event horizon of my understanding.
Why doesn't the time aspect completely alter the nature of evidence gathered? Working with data that comes from billions of years hence must make calculations incredibly obscure.
In what ways is this temporality a help and a hinderance? How are the factors of time, space and motion / change plotted to form the model?
posted by edd:I think the brief answer to the original question is that you can build mathematically quite simple models of distance, time and redshift relations which let you 'do things right' and allow for all these factors properly, all deriving from General Relativity. This lets you do things like work out how big an object appears at cosmological distances, and as you are getting at when you talk about the distant universe being smaller, this 'angular diameter distance' isn't monotonic, so more distant things start looking bigger rather than smaller as they get further away. wikipedia link.
Me again:I definitely get the most confused when thinking about the speed of light, the speed the universe is expanding (and the way this has changed through time), the distance between objects now compared to when the light was first emitted. on top of this, surely we have been moving away from all the light sources also? The red shift is not just a factor of an object's motion in relation to us, but in both our motions in relation to each other.More answers:
And yet this motion means nothing at any one point on the time axis because the radiation (light etc.) we gather the information from was emitted when the universe was arranged completely differently.
All this together causes severe confusion.
Is there a good analogy to the 4 dimensional model of our universe (time + 3 space)? If I could visualise us now in relation to the motion, the distance, the time etc. I might have a better grasp of all this (the trumpet idea mentioned thus far is the kind of thing I mean).
posted by edd:You're right to worry about the distance between objects now and that when the light was first emitted. To work around this, cosmologists work in 'comoving' distance, which basically factors out the universe's expansion, and they can then work out from that the distance between the objects then, the distance now, the distance the light travelled and how far away it actually looks - all of which are generally different. The important thing is that our models of how the universe expands tells us quantitatively how they are different, so we can handle this all fine. It does generally cause severe confusion when one tries to think about it, but you can with practice get to grips with it, and most importantly as I've said, we've got equations that tell us exactly what happens....and...
What I think you're getting at with regards to 'our motions in relation to each other' is if we've got some velocity through space towards an object, or if the object has some velocity through space towards us, ignoring the expanding space bit. That's 'peculiar velocity', and is impossible to measure for most galaxies, and we have to satisfy ourselves with the fact that this effect is small compared to cosmological redshift, and that it statistically speaking can be averaged out and accounted for in other ways quite often.
posted by andrew cooke:it is hard, and there's no easy answer. astronomers use mathematical models of how the universe evolves to help understand their observations, but these models themselves are uncertain.Full discussion here...
so you end up with astronomers doing two conflicting things:
1: looking at distant objects because they want to understand the early universe (how stars and galaxies first formed, for example). in research like this, you use the models to calculate how far back in time you are observing etc etc and you are hoping to find things that are different to how you see them today (eg "baby galaxies")
2: trying to find distant objects that are the same as those nearby so that they can use the apparent difference to calibrate the models. in other words, if you take something far away, and correct your observations using maths based on the models, you should end up with something that looks like things nearby (and if you don't, you can learn something about the models for how the universe evolves). in research like this you are hoping to find things that are the same (intrinsically) to those you find today (nearby).
so there is a conflict/balancing act because both (a) what the early univese was like and (b) how the universe has evolved are both uncertain, and given an observation you typically assume one to find the other.
in fact, current ideas suggest that objects in the universe changed quite a lot right at the beginning, but then didn't do much more. so for well over half the age of the universe, things have been pretty much the same. you can probably see how that helps - models of the universe can be calibrated by looking back "not too far", and then are extrapolated to the very early times.
disclaimer - this is a bit simplified, but i think it's basically right.
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trouble is, cosmology just changed :o)
poking around on the net turned up this - is that any good?
this is pretty hard (especially angular size) in my opinon. just take your time...
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