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morningstar
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How is the age of the universe measured? Is it by the distance light has traveled since the big bang? Does that imply a closed universe?
1. Through model fitting. We have a model for the contents of the universe (matter, radiation, dark matter, dark energy, etc.), and determine the model parameters based upon the data. Extrapolating this model back in the past leads to a singularity in the model. We don't take this singularity seriously: it is obviously an incorrect description of the very early universe. But it serves as a decent-enough zero point. These days, the data are good enough that it doesn't matter that much which particular model you choose for the age of our universe.morningstar said:How is the age of the universe measured? Is it by the distance light has traveled since the big bang? Does that imply a closed universe?
Well, sort of. A very common coordinate system to use in cosmology is the comoving coordinate system: coordinates that expand as the universe expands. In comoving coordinates, the coordinate distance between objects tends to not change (except for local motions due to gravitational collapse).morningstar said:thanks chalnoth,
although the distance that light has traveled since the big bang cannot be measured, are there any theoretical models that hold the size of the universe- as measured by the expansion of light since the big bang- constant? in a model like that it would seem that everything inside the universe is shrinking.
Well, the problem there is that there is no absolute definition for "total energy" for the universe. In fact, overall, energy doesn't even appear to be conserved in an expanding universe. See here for a rather in-depth discussion of energy conservation in General Relativity:morningstar said:if all the energy of the universe can be measured within the body of light emitted by the big bang, then it seems that, what we perceive to be, spatial expansion/inflation, is not really making the universe any bigger, it is simply redistributing energy; and making cosmological bodies smaller, in a very real sense.
There's no difference between the two descriptions. In the normal description, atoms are stable and the universe is expanding. In the other, atoms are shrinking while the universe is stable. We usually choose the former description because rewriting electricity and magnetism as well as quantum mechanics to take this shrinking into account would be horribly complicated, and would contain a number of terms that don't seem to make sense (e.g. the value of the cosmological constant). But it's useful to use the second description when we don't care about describing the behavior of atoms precisely, as it makes some cosmological calculations easier.morningstar said:great link!
if we are shrinking- relative to the size of the universe and the light that is moving away from us since the big bang- then we must be shrinking at an accelerating rate. could this be the cause of our perception that cosmological bodies are moving away from us? it seems that, relative to the size of the universe, they must be getting closer to us. do comoving coordinates account for that?
I don't think it can. It's just a change in coordinates, after all. But it is very difficult in practice to adjust the laws of physics to compensate for this coordinate change.Chronos said:Btw, the shrinking universe idea conflicts with an abundance of observational evidence.
Well, no, it doesn't make our clocks slower. But it necessitates rewriting a lot of physics to keep everything consistent. As Chronos notes, however, there's no reason to believe our universe has an edge.morningstar said:aside from the math, if we hold a theoretical edge of the universe constant, and everything inside as shrinking, then isn't the speed of light changing as our rulers literally get smaller to measure it. though I understand that would make our clocks slower, so we wouldn't perceive it as slowing. but the distance that light would cover would be shorter- relative to the size of the universe- over a duration of time that we measured to be the same?
Chalnoth said:Well, no, it doesn't make our clocks slower. But it necessitates rewriting a lot of physics to keep everything consistent. As Chronos notes, however, there's no reason to believe our universe has an edge.
Well, no, the speed of light is the ratio of distance to time. So when you start changing the length scales, then the speed of light changes as well, because the ratio of distance to time changes. If you also changed time, you'd have something completely different going on. It's possible to do, but then that just adds another level of complexity to an already complex problem.morningstar said:is not the measure of light simply a measure of time? if our rulers are shrinking and we measure light to be the same speed then time must be slowing at the same rate. it seems our perception of time is as a fish's perception of water- per chronos' post-script.
Chalnoth said:Well, no, the speed of light is the ratio of distance to time. So when you start changing the length scales, then the speed of light changes as well, because the ratio of distance to time changes.
Yeah, but making the change to a coordinate system where atoms shrink is really just a coordinate system change. Sure, it makes the calculations for how matter behaves horribly complicated, but it is just a coordinate system change.Chronos said:Everything we think we know about physics pretty much gets tossed out the window if spectral lines vary with respect to the age of the universe. We would, instead of a difficult problem, be faced with one that is well nigh insurmountable.
Scientists use a variety of methods, including measuring the expansion rate of the universe, studying the cosmic microwave background radiation, and analyzing the light from distant objects to estimate the age of the universe.
Light is the fastest known entity in the universe, and it carries valuable information about the age and history of the universe. By studying the light from distant objects, scientists can uncover clues about the universe's past and its rate of expansion.
A closed universe is one in which the expansion of the universe will eventually halt and reverse. This concept is important because it affects the calculations used to estimate the age of the universe. If the universe is closed, it will have a finite age, whereas an open universe can have an infinite age.
The cosmic microwave background radiation is the leftover radiation from the Big Bang that fills the entire universe. By studying the patterns and fluctuations in this radiation, scientists can estimate the age of the universe and gain insights into its early stages of development.
The current estimated age of the universe is around 13.8 billion years. This number is based on various cosmological models and observations, such as the expansion rate of the universe, the cosmic microwave background radiation, and the abundance of certain elements in the universe. However, as our understanding of the universe evolves, this estimated age may change. Some possible explanations for the current estimated age include the rate of expansion, the presence of dark matter and dark energy, and the accuracy of our measuring techniques.