Calculating Age of Universe Using Redshift: 0.6

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SUMMARY

The discussion focuses on calculating the age of the universe at a redshift of 0.6, given that the current age is 13.4 billion years. Participants clarify that to find the age at this redshift, one must first determine the scale factor using the formula z = (a0/a) - 1. The Friedmann equation is essential for understanding the relationship between the scale factor and time, with a(t) being proportional to t^(2/3) in a matter-dominated universe. This approximation allows for the calculation of the universe's age at different redshifts.

PREREQUISITES
  • Understanding of redshift and its implications in cosmology
  • Familiarity with the Friedmann equation and its components
  • Knowledge of scale factors in cosmological models
  • Basic grasp of power laws and their application in physics
NEXT STEPS
  • Study the Friedmann equation in detail to understand its application in cosmology
  • Learn about the scale factor and its role in calculating cosmic distances
  • Explore the concept of redshift and its significance in measuring the universe's expansion
  • Investigate the implications of a matter-dominated universe on cosmic evolution
USEFUL FOR

Astronomy students, cosmologists, and anyone interested in understanding the calculations behind the age of the universe and redshift effects.

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Hi i am confused as to how to calculate the age of the universe with redshift
say for example

The age of the universe now is 13.4 billion years old (and a critical universe).
How do i find the age of the universe if it was a redshift at say 0.6??

Do i have to find the scale factor first?
I am not very sure, please help!
 
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You need to know the ratio of the scale factors. z=(a0/a)-1 where a is the scale factor then and a0 is the scale factor now.
 
how do i get that? do i have to integrate first
 
No. To a good approximation the universe has been matter dominated all of it's history. What does a(t) look like as a function of t in this case?
 
so how would that work then?
 
What does a(t) look like as a function of t in a matter dominated universe? You can look it up, it's a power law.
 
to the power of 4
 
Nope. Use the Friedmann equation. H^2 is proportional to rho. If a(t)=t^n. H is proportional to 1/t. rho is proportional to 1/a(t)^3. So 1/t^2 is proportional to 1/a(t)^3. So a(t) is proportional to t^(2/3).
 
I'm sorry I'm not an expert on this I don't usually take science courses... but are u saying I'm gna take a(t)= k * t^(2/3) . and that gives me the answer?
 
  • #10
Yes. Since z=(a0/a)-1, this gives z=(t0/t)^(2/3)-1. (t0 is the age of the universe and t is time at redshift z. It's an approximation but it should do. You are asking some pretty hard questions for a non-science course person. What's the course?
 

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