Integration questions for my astoronomy class

AI Thread Summary
The discussion focuses on integration techniques needed for an astronomy class, specifically integrating from a defined range with a complex function involving Hubble's constant and cosmological parameters. The user expresses confusion about how to approach the integration process, particularly with the given differential equation. A suggested method involves a variable substitution to simplify the integration, referencing trigonometric identities to facilitate the calculation. The conversation emphasizes the importance of understanding the integration steps and transformations to solve such problems effectively. Mastering these integration techniques is crucial for success in astronomy-related coursework.
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Hi, I have to do a lot of integration questions for my astoronomy class but I'm not really sure how to! for example how do u integrate from a number let's say a = 0, to a = 1/(1+z)... and dt = \frac{da}{H_0 \left(\frac{\Omega_{m,0}}{a} + a^2 \Omega_{\Lambda,0}\right)^{\frac{1}{2}}}

I've done a different kind of simple integration but i have no idea how this works,. thanks!
 
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dt = \frac{da}{H_0 \left(\frac{\Omega_{m,0}}{a} + a^2 \Omega_{\Lambda,0}\right)^{\frac{1}{2}}}

Is this what you mean ?
 
To integrate \frac{du}{(a^2 + b^2 u^2)^{-\frac{1}{2}}}
make the variable change
\frac{bu}{a} = tan v
and remember that
1 + tan^2 v = sec^2 v
 
yest mentz its that one
 
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