How Do Observers Measure the Universe's Age and Size in Cosmology?

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In summary, the age and size of the universe are measured with respect to the cosmic microwave background's rest frame, using different distance measures in cosmology. However, not every observer in the universe agrees on these measurements due to the concept of comoving observers. The age of the universe is defined as the proper time experienced by a comoving observer since the big bang, but there is no absolute size. The proper times of comoving observers form the "cosmological time," but there is time dilatation when comparing time between different observers using the standard special relativity procedure. This is not a contradiction as cosmological coordinates and special relativity coordinates differ in their definition of simultaneity.
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MaxwellsDemon
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Forgive me if these questions are asked here a lot, but I couldn't find any posts answering them in the first few pages... I'm just starting to learn a bit about cosmology...because I'm currently learning general relativity. I'm just curious, what does it mean to say that the universe has a certain age and a certain size? With respect to what are these measured? Does every observer in the universe agree on the value of these measurements? I ask because in special relativity, different observers don't agree on things like the rate of the passage of time. If every observer agrees on the age and size of the universe, can't these values be used to define an absolute time and an absolute length from which all others can be measured?
 
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Basically the age of the universe is measured with respect to the cosmic microwave background's rest frame. Same is true for size, but instead of one definition of "length", in cosmology you have like 3 or 4. You can find the descriptions for different distance measures for example from wikipedia, http://en.wikipedia.org/wiki/Distance_measures_(cosmology)
 
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Does every observer in the universe agree on the value of these measurements?
No.
The universe is modeled as being full of a "fluid" - that's dust, gas, radiation , stars etc.
At each point, there can be one preferred observer, the one who is at rest with the averaged local fluid. These are called "comoving observers".
The "age of the universe" is defined as the proper time that such an observer exerienced since the big bang.
Any observer with a significant speed relative to these will be younger, when compared at the same location.

If every observer agrees on the age and size of the universe, can't these values be used to define an absolute time and an absolute length from which all others can be measured?
There is no absolute size, but, by definition, the proper times of comoving observers form the "cosmological time".
Still, if different comoving observers compare time via the standard SR procedure, there is time dilatation between them. Cosmological coordinates and SR coordinates differ in their definition of simultaneity, so that's not a contradiction.
 

Related to How Do Observers Measure the Universe's Age and Size in Cosmology?

1. What is the Big Bang Theory?

The Big Bang Theory is the prevailing scientific explanation for the origin of the universe. It states that the universe began as a single point of extremely high density and temperature, and has been expanding and cooling ever since.

2. How old is the universe?

According to current scientific estimates, the universe is approximately 13.8 billion years old. This age is determined by measuring the rate of expansion of the universe and extrapolating backwards.

3. What is dark matter?

Dark matter is a type of matter that does not emit or interact with light, making it invisible to telescopes. It is thought to make up about 27% of the universe and is believed to play a key role in the formation and evolution of galaxies.

4. What is the fate of the universe?

The fate of the universe is currently unknown and is a subject of ongoing research and debate among scientists. Depending on the amount of dark matter and dark energy in the universe, it could continue to expand forever, eventually leading to a "heat death," or it could experience a "Big Crunch" and collapse back in on itself.

5. What is the cosmic microwave background radiation?

The cosmic microwave background radiation (CMB) is a form of electromagnetic radiation that fills the entire universe. It is a remnant of the Big Bang and is one of the strongest pieces of evidence for the theory. It appears as a faint glow in the microwave portion of the electromagnetic spectrum.

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