Expanding Universe: Doubts & Questions

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Discussion Overview

The discussion revolves around the concept of the expanding universe, specifically questioning whether both space and time intervals are expanding, the rate of this expansion, and the implications of these ideas on local observations and relativistic effects. Participants explore theoretical and observational aspects of cosmic expansion, touching on models and implications in both general and special relativity.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants assert that only space is expanding, while others suggest that this expansion leads to an implicit time expansion due to the increased time taken for objects to reach each other.
  • There is a discussion on the rate of expansion, with references to Hubble's law, and the observation that local gravitational forces counteract cosmic expansion, making it imperceptible at small scales.
  • One participant questions how time expansion could be experimentally or observationally determined, leading to a distinction between special and general relativistic effects.
  • Another participant elaborates on relativistic time dilation, discussing the implications of time dilation in gravitational fields and relative motion, while questioning the concept of universal time expansion.
  • There are speculative ideas about how time dilation might affect the motion of stars in galaxies and the potential relationship between spacetime warping and the shapes of galaxies.
  • Some participants reference models likening the expansion of the universe to objects on an inflating balloon, emphasizing that expansion becomes significant only on large scales.

Areas of Agreement / Disagreement

Participants generally agree that only space is expanding, but there is no consensus on the implications of this expansion for time or how it can be observed. Multiple competing views remain regarding the nature of time dilation and its effects.

Contextual Notes

Limitations include unresolved questions about the observational methods for measuring time expansion, the dependence on definitions of time and space, and the complexities of gravitational influences on local scales.

Who May Find This Useful

This discussion may be of interest to those exploring cosmology, general and special relativity, and the implications of cosmic expansion on local observations and theoretical models.

arroy_0205
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I have certain doubts about the notions of expanding universe:

1. Are both space and time intervals expanding or only the space interval expanding? According to FRW model, only space is expanding. Is that correct?

2. At what rate is this expansion taking place? When I talk to my friend, I do not find him moving away from me with time. Does that mean the expansion rate is very small?
 
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1) As far as i know only space is expanding, however because things in that 'bit' of space would be moving and thus things move away from each other, you get a sort of implicit time expansion too because things take longer to get to each other. This reinforces the idea of spacetime as inseperable
2) Expansion roughly follows hubble's law which is v = H d where v is the velocity of expansion, H is the Hubble parameter (not constant with time, thus accelerating universe) and d is the distance between two things. The reason you don't see your friend moving away from you is cosmic expansion is almost completely countered in the gravity well of the galaxy let alone the Earth. Basically gravitational forces ensure this doesn't happen on the local scale but it can be observed in between clusters and such.

Some links:
http://en.wikipedia.org/wiki/Hubble's_law
http://en.wikipedia.org/wiki/Freidmann_equation
 
Experimentally or observationally how does one know if time is expanding or not?
 
Depends. If its special relativistic time dilation, you dont. If its due to general relativistic effects then you can measure the potential well you are in (or the acceleration you are under) and do the maths and work it out.

EDIT: Sorry saw you said observationally. Erm...i think you can measure your local curveture but I am not sure (for GR effects)
 
arroy_0205 said:
2. At what rate is this expansion taking place? When I talk to my friend, I do not find him moving away from me with time. Does that mean the expansion rate is very small?

This is a time effect. Have you ever noticed that when you spend a lot of time with a friend, you slowly drift apart and become disillusioned from each other? :biggrin:
 
1). The only type of time dilation that I am aware of is due to relativistic effects, such as the the slightly slower frequency of clocks at rest in a gravitational field when compared to clocks in free fall, or the slightly slower frequency of clocks, when traveling at great speed relative to an observer. The only thing we can say with certainty is that the speed of light is constant. If intervals of time were expanding everywhere as you suggested, then we could say that activities were slowing down everywhere, but slowing down with respect to what? Some grand clock outside of time and space, A hyperspacetime clock perhaps? Everything within this time expansion, including a beam of light would automatically be accelerated, so for our velocity of light to remain constant, space would necessarily have to expand to allow for the slower time. It seems to me that this theory would break down when taken to the extreme... when time stops with respect to our hyperspacetime clock and space is infinitely large. This may sound rediculous, and some like Brian Greene in The Fabric of the Cosmos argue that Einstein's results only pertain when the expansion of space has been subtracted out, and that objects beyond our cosmic horizon can recede at greater than light speed, but what if we extended this idea of spacetime dilation to the large scale example of widely spaced clusters of stars traveling along the spiral arms around the massive center of a distant galaxy. Wouldn't this time dilation cause the tangential velocity of stars to increase as they moved outward from the massive center of the galaxies, as was the case for our accelerated beam of light in expanding space. Could this warping of spacetime caused by expansion, which amplifys velocity over time produce the mysterious Archemedian spiral shape we see when looking at spiral galaxies. Shapes that according to Milgrom violate Newton's first law, F=ma? If so, then the rate of expansion could roughly be estimated by rolling the galaxy along one of its spiral arms and measuring the slope of the line created by it's center. Physicists have used several more accurate ways to calculate the overall expansion rate using observations of the intensity of light from quasars to determine distance and the doppler shift of the wavelength of light from distant stars to determine their speed. Many attribute this expansion to a dark energy that acts between massive, distant objects on a grand scale and is much less than the force of gravity.
2). According to Brian Greene's book, Only on the largest of scales is the expansion of space able to overcome the gravitational and stronger electromagnetic forces. Therefore the expansion of the universe is similar to coins affixed to an inflating balloon or poppy seeds within or on a rising muffin. In this model, the size of the seeds is fixed, but the expansion of space continues to accelerate, until eventually distant objects loose their ability to communicate to each other as the expansion of space between them reaches the speed of light. This is what I referred to earlier as the cosmic horizon.
 
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