B Calculating the age of the universe with the Hubble constant

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Discussion Overview

The discussion revolves around the calculation of the age of the universe using the Hubble constant (Ho) and the implications of the universe's expansion rate. Participants explore the relationship between distance, velocity, and the changing nature of the Hubble constant over time.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants express uncertainty about using 1/Ho to determine the age of the universe, noting that the velocity of galaxies changes over time according to Hubble's Law.
  • There is a discussion about the distinction between velocities being constant with respect to time for a given galaxy versus varying with distance for different galaxies.
  • One participant questions whether the assumption of constant velocity since the Big Bang implies that recession speeds are constant with respect to distance.
  • Another participant clarifies that while the distance to galaxies increases at different rates today, the concept of constant expansion refers to the velocity of a specific galaxy being constant since the Big Bang.
  • Participants discuss the implications of Hubble's "constant" not being truly constant over time, suggesting that it decreases linearly as time progresses.
  • There is mention of ongoing advancements in measurement tools, such as the E-ELT and the CODEX experiment, aimed at measuring the accelerated expansion of the universe with high precision.

Areas of Agreement / Disagreement

Participants generally agree that the Hubble constant is not truly constant over time and that the relationship between distance and recession speed is complex. However, there are competing views regarding the implications of these concepts and the assumptions made in calculations.

Contextual Notes

Participants acknowledge limitations in their assumptions and the need for precision in measurements, particularly regarding the changing nature of the Hubble constant and its implications for understanding the universe's age.

Who May Find This Useful

This discussion may be of interest to those studying cosmology, astrophysics, or anyone curious about the dynamics of the universe's expansion and the methodologies used to measure it.

anonymous24
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Hello,
When we assume the universe is expanding at a constant rate, we could say the age of the universe is 1/Ho. but I always feel unsure about that because 1/Ho is the distance over the velocity. However, the velocity changes over time, that is, when something is closer to us, the move slower and when they are further, they move faster according to Hubble's Law. So my question is how can we assume the velocity is constant while it's accelerating ? Thank you in advance.
 
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anonymous24 said:
Hello,
When we assume the universe is expanding at a constant rate, we could say the age of the universe is 1/Ho. but I always feel unsure about that because 1/Ho is the distance over the velocity. However, the velocity changes over time, that is, when something is closer to us, the move slower and when they are further, they move faster according to Hubble's Law. So my question is how can we assume the velocity is constant while it's accelerating ? Thank you in advance.

Do not confuse "constant or not with respect to time" with "constant or not with respect to distance". When we assume a constant rate, the velocities with respect to us are constant with respect to time but it is true that the velocities of galaxies at different distances are different. But if you pick a given galaxy, we take its velocity to have been constant since the Big Bang. Of course, this approximation of constant velocities is far from what is actually going on and must taken with a huge grain of salt. Even in a universe with constant Hubble parameter, there are subtle effects to take into account.
 
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nrqed said:
Do not confuse "constant or not with respect to time" with "constant or not with respect to distance". When we assume a constant rate, the velocities with respect to us are constant with respect to time but it is true that the velocities of galaxies at different distances are different. But if you pick a given galaxy, we take its velocity to have been constant since the Big Bang. Of course, this approximation of constant velocities is far from what is actually going on and must taken with a huge grain of salt. Even in a universe with constant Hubble parameter, there are subtle effects to take into account.
Thank you for your reply. However, there is one point I'm not so sure about. You mentioned we assume the velocity with respect to us of a given galaxy is constant with respect to time, does it imply that it is moving away from us with constant velocity since the big bang? If so, how does this not imply that the velocity is also constant with respect to distance, i.e. as it certainly gets further away from us. Thank you.
 
anonymous24 said:
does it imply that it is moving away from us with constant velocity since the big bang?
That is exactly the meaning of "constant expansion".
anonymous24 said:
If so, how does this not imply that the velocity is also constant with respect to distance, i.e. as it certainly gets further away from us.
"with respect to distance" compares two different objects at different distance but at the same time. The distance to something that is now 10 billion light years away from us increases faster today than the distance to something 5 billion light years away.
 
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mfb said:
That is exactly the meaning of "constant expansion"."with respect to distance" compares two different objects at different distance but at the same time. The distance to something that is now 10 billion light years away from us increases faster today than the distance to something 5 billion light years away.
Thank you so much, that clears up a lot of my confusion. I just have one last question that does it mean the recession speed against distance from our Earth diagram (gradient = Ho) changes over time? like it will look really different a thousand years in the future? Thank you. Is it also why Hubble Constant changes over time?
 
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anonymous24 said:
Thank you so much, that clears up a lot of my confusion. I just have one last question that does it mean the recession speed against distance from our Earth diagram (gradient = Ho) changes over time? like it will look really different a thousand years in the future? Thank you. Is it also why Hubble Constant changes over time?
That's right. Hubble's "constant" is a misnomer as it is not at all a constant with respect to time. In a constant rate expansion universe, the formula age of universe = ##1/H_0## remains valid at all times which shows that as time passes, Hubble's "constant" has to change. It actually decreases linearly with time in such a universe. A thousand years would be too short to notice the variation (unless much much more precise measurement tools are made available) but, say, in a billion years it would be clear that ##H_0## would have decreased.
 
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nrqed said:
That's right. Hubble's "constant" is a misnomer as it is not at all a constant with respect to time. In a constant rate expansion universe, the formula age of universe = ##1/H_0## remains valid at all times which shows that as time passes, Hubble's "constant" has to change. It actually decreases linearly with time in such a universe. A thousand years would be too short to notice the variation (unless much much more precise measurement tools are made available) but, say, in a billion years it would be clear that ##H_0## would have decreased.
Thank you so much, it's really clear to me now.
 
nrqed said:
A thousand years would be too short to notice the variation (unless much much more precise measurement tools are made available)
Those tools are under construction. The E-ELT (first light expected 2024) will have a mirror as large as the 20 largest existing telescopes combined. The CODEX experiment there plans to directly measure the accelerated expansion of the universe within a few years. The idea is simple: measure the redshift of some galaxies, repeat the measurements a few years later. The challenge is the required precision, the redshift has to be measured with a precision of 1 part in a billion.
Reference
 
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mfb said:
Those tools are under construction. The E-ELT (first light expected 2024) will have a mirror as large as the 20 largest existing telescopes combined. The CODEX experiment there plans to directly measure the accelerated expansion of the universe within a few years. The idea is simple: measure the redshift of some galaxies, repeat the measurements a few years later. The challenge is the required precision, the redshift has to be measured with a precision of 1 part in a billion.
Reference
That's fascinating, thanks for the info!
 

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