Is There a Simple Equation for Hubble's Constant and Time in Astronomy?

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SUMMARY

The discussion centers on a simplified equation relating Hubble's constant (H(t)) and time in a matter-dominated Robertson-Walker universe. The equation derived is H(t) = H0*(t0/t), which follows from the Friedmann and continuity equations of general relativity. It is emphasized that this equation does not accurately reflect the universe's expansion at all times due to periods of radiation dominance and the transition to Lambda-dominance. Misinterpretations regarding the "speed of expansion of the universe" are also addressed, clarifying that H(t) does not imply a constant speed or size of the universe.

PREREQUISITES
  • Understanding of Hubble's constant and its significance in cosmology
  • Familiarity with the Friedmann equations in general relativity
  • Knowledge of the Robertson-Walker metric
  • Basic concepts of matter and radiation dominance in the universe
NEXT STEPS
  • Research the Friedmann equations and their implications in cosmology
  • Study the Robertson-Walker metric and its applications in cosmological models
  • Explore the concept of Lambda-dominance and its effects on cosmic expansion
  • Investigate common misconceptions about the expansion of the universe and Hubble's law
USEFUL FOR

Astronomers, astrophysicists, and students of cosmology seeking to deepen their understanding of Hubble's constant and the dynamics of the universe's expansion.

Ledsnyder
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I found an equation relating hubbles constant and time!It is highly simplified but helpful!

http://www.astronomycafe.net/qadir/q679.html


da/at = (2/3)*a0* (1/t0) * (t/t0)^-1/3

then dividing by a = a0 (t/t0)^2/3 you get

H(t) = H0*(t0/t)
 
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This is not simplified -- it is the explicit Hubble parameter as a function of time in a matter-dominated Robertson-Walker universe. It follows from the Friedmann and continuity equations of general relativity.
 
Maybe the simplification is in the fact that it does not always give the right numbers, because our real universe has not been and will not be all the time matter-dominated. It has been radiation dominated for a while in the past, and then kind of a balanced mix for a while. And lately it is gradually shifting over from matter dominance to Lambda-dominance.

The main trouble, though, is what you see if you follow the link. The author refers to this as "the speed of expansion of the universe".

The equation quoted is about H(t). It is not about "the speed of expansion of the universe." People often get confused, it seems to me, when they are told that the universe has a speed of expansion:

1. then they get the idea that it must have a definite known size (else how could it have a speed of expansion?)

2. and they get the idea that this imagined speed must be increasing because they have heard "acceleration" mentioned. (whereas H(t) has been and is expected to continue decreasing).

So they get a bunch of misconceptions that IMHO take root primarily because of careless language.
 

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