Using Hubble parameter defn to change integration variable from t to a

In summary, the given integral can be solved by using the Hubble parameter definition and rearranging to find dt. Then substituting this into the original integral and simplifying, we can use the substitution method to integrate with respect to a and arrive at the final expression for r1 in terms of a, using the Hubble parameter definition.
  • #1
ck99
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Homework Statement



r1 = tt1 1/a(t) dt

Use the Hubble parameter definition to change from t to a, if a(t) = a and a(t1) = 1

Homework Equations



Hubble parameter H = a' / a where a' = da/dt

The Attempt at a Solution



Start with Hubble parameter definition, and rearrange to find dt

aH = da/dt

dt = 1/aH da

Substitute this into the original integral to get

r1 = a1 (1/a) (1/aH) da

Simplify, because

(1/aH)(1/a) = 1/(a2H) = 1/(aa') (from Hubble parameter defn)

So r1 = a1 1/(aa') da

I'm not sure if this is the right approach, and if it is, how do I integrate this expression with respect to a when it has an a' term in it? I think my effort is all wrong, because it does not help me at all with the second part of the question :(

Any help much appreciated!
 
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  • #2

Your approach is correct so far! To integrate the expression with respect to a, you can use the substitution method. Let u = aa'. Then du = a'da. Substituting this into the integral, we get:

r1 = ∫1 1/u du

Integrating, we get:

r1 = ln(u) + C

Substituting back for u, we get:

r1 = ln(aa') + C

Since we know that a(t1) = 1, we can substitute this in to get:

r1 = ln(aa') - ln(1) = ln(aa')

To solve for a, we can take the exponential of both sides:

e^r1 = aa'

a = e^r1 / a'

This gives us the final expression for r1 in terms of a, using the Hubble parameter definition.

Hope this helps!
 

1. What is the Hubble parameter definition?

The Hubble parameter, denoted as H(t), is a measure of the rate at which the universe is expanding at any given time. It is defined as the ratio of the velocity of a galaxy or other astronomical object to its distance from us.

2. How is the Hubble parameter used to change the integration variable from t to a?

The Hubble parameter can be used to change the integration variable from t (time) to a (scale factor) in cosmological calculations. This is done by using the relation a = 1/(1+z), where z is the redshift, and substituting it into the equation for H(t).

3. Why is it necessary to change the integration variable when using the Hubble parameter definition?

Changing the integration variable from t to a allows for a more intuitive understanding of cosmological calculations. The scale factor, a, represents the size of the universe at a given time, and using it instead of time allows for a better understanding of the expansion and evolution of the universe.

4. What is the significance of using the Hubble parameter definition in cosmology?

The Hubble parameter is a crucial tool in cosmology as it provides important information about the expansion rate and age of the universe. It is also used in calculations related to the Big Bang theory and the evolution of the universe over time.

5. How is the Hubble parameter related to the Hubble constant?

The Hubble constant, denoted as H0, is the current value of the Hubble parameter at the present time. It is used to measure the expansion rate of the universe at the current moment. The Hubble parameter is related to H0 through the equation H(t) = H0/a, where a is the scale factor at the present time.

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