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jalak7
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When the universe was young, and everything was closer together, did the extra gravity cause time to run slower than it does now?
It seems you are talking about 'proper' time, the time your wristwatch is showing. By no means can you tell that the time it shows runs slower.Crazymechanic said:Quite logically from what we know the simple answer would be yes.And considering that the early universe was much more dense , in fact a lot more dense I would say that time run slower for every average observer no matter where one would be in the early universe.
Crazymechanic said:Quite logically from what we know the simple answer would be yes.And considering that the early universe was much more dense , in fact a lot more dense I would say that time run slower for every average observer no matter where one would be in the early universe.
As it expanded it became more and more like the universe we know today with planets and black holes with huge mass and hence gravity around them and then with a lot of "empty" space between with quite small gravitational potential.
I'm not sure there's actually any time dilation at all from the average matter density.Mordred said:The only era in the past that might (key word might) be dense enough to dilate time would be prior to the inflationary era.
I'm pretty sure this can be solved by comparing the time coordinate in FRW to proper time. For an observer stationary with respect to the background, those two are the same thing. So yes, there is no time dilation from the expansion.Mordred said:To be honest with you neither am I. Granted I also cannot find any reliable source with an estimate of the density of the Planch and GUT epoch. Some of the older particle physics articles covering the TOE aspects of these epochs. Place the density around 10^78 gm/cm^3. The article is reliable in regards to particle physics. If one accepts TOE. However its calculations are based on a far older inflationary model. Still doubt that would be enough for time dilation. Assuming we have a magic telescope to allow us to be an outside observer lol.
I think the problem is that there isn't any way to compare relative time dilation between two different points in time.jalak7 said:When cosmic background radiation was created the time flow throughout the universe was pretty much the same everywhere, right? So if we made a clock based on that and called it a universal clock, then would the flow of time in the early universe be slower relative to the universal clock than time flow is today, because of the difference in gravity?
timmdeeg said:To my understanding even much higher matter density of the universe in the past wouldn't cause gravitational time dilation, because in contrast to Schwarzschild metric the gravitational potential in the FRW model is isotropic. May be this wording isn't correct. What I mean is that as long as we keep the picture that the redshift is due to expansion the density plays no role.
Hi Mordred, the cosmological redshift/time dilation is directly related to the scale factor and to the special relativistic Doppler formula in the empty case, resp. Thus we fortunately don't have to care about things like time slices, energy density and a certain epoch. Indirectly yes, as the dynamics depend on energy density, pressure and lambda.Mordred said:If a particular De-Sitter (matter removed) time slice has no gravity wells to cause a redshift. That lack of dilation cannot be seen in another time slice. So the only measurable difference in regards to redshift would be due to expansion. Also keep in mind the universal energy-density at any time after the inflationary epoch is not enough to cause a dilation.
I think the distinction proper time vs. coordinate time is not related to how in which epoch the universe develops. As soon as there is a distance, there is relativity, means there is proper time, which is invariant and coordinate time, which isn't.petm1 said:I would think that in the early universe time ticked at the same rate for all clocks, coordinate time was the only time. As the duration of the universe increased the difference between coordinate time of the universe and the proper time of matter began to differ as they aged at about the same rate. The simultaneous moment of coordinate time, one clock for the universe, as compared with the simultaneous motion of a single clock within it.
I am not sure, what you want to say. Perhaps this is of some help. Coordinate/proper time is not related to density.petm1 said:At some point in the smaller denser hotter past all the makings for all of our clocks were local and ticking at the same rate.
The main evidence for the slower flow of time in the early universe comes from the observed cosmic microwave background radiation. This radiation is believed to be the leftover energy from the Big Bang and its pattern closely matches that of a blackbody, indicating a uniform and hot early universe. The fact that the cosmic microwave background has a uniform temperature across the sky also suggests that the universe was expanding and cooling at a consistent rate, which is a key factor in determining the speed of time.
Albert Einstein's theory of relativity states that time is relative and can be affected by factors such as gravity and velocity. In the early universe, both of these factors were much stronger compared to the present day. This means that time would have passed at a slower rate in the early universe due to the high gravitational forces and the rapid expansion of space.
Based on our current understanding of physics, time is an essential component of the universe and cannot be completely different in different regions or eras. However, the rate at which time flows can vary based on the conditions present. Therefore, while time may have been slower in the early universe, it still existed and followed the laws of physics.
Unfortunately, there is no direct way to measure the flow of time in the early universe as we cannot observe it directly. However, by studying the cosmic microwave background and other astrophysical phenomena, scientists can make precise calculations and predictions about the rate of time in the early universe.
Entropy is a measure of disorder and is closely related to the flow of time. In the early universe, the high energy and high temperatures meant that the universe was in a state of low entropy, meaning it was highly ordered. As the universe expanded and cooled, the entropy increased, indicating that time was passing. This concept is known as the second law of thermodynamics and helps us understand the direction of time's flow in the early universe and beyond.