Solving Normalization Factor for 1s Atomic Orbital of H

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Hi all! I hope somebody is able to help me on my way with this question.

I have been asked to show that the Normalization factor for the 1s atomic orbital of H is 1/(\Pi a_o^3)^\frac{1}{2}. The wavefunction is \psi(r) = N exp(-r / a_o)

I'm given dt = r^2 sin \Theta and dr d\Theta d\Phi and \int_{0}^{\infty}x^n e^a^x dx=n!/a^n+1

I must admit I'm clueless which direction to go. It was mentioned to me, that squaring the wavefunction is the first step, but I cannot arrive at the given constant. Am I starting off on the wrong foot?

Thanks for any input, in advance.

geronimo
 
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geronimo123 said:
Hi all! I hope somebody is able to help me on my way with this question.

I have been asked to show that the Normalization factor for the 1s atomic orbital of H is 1/(\Pi a_o^3)^\frac{1}{2}. The wavefunction is \psi(r) = N exp(-r / a_o)

I'm given dt = r^2 sin \Theta and dr d\Theta d\Phi and \int_{0}^{\infty}x^n e^ax dx=n!/a^n+1

I must admit I'm clueless which direction to go. It was mentioned to me, that squaring the wavefunction is the first step, but I cannot arrive at the given constant. Am I starting off on the wrong foot?

Thanks for any input, in advance.

geronimo
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Sorry about this - I don't know how it managed to post twice. It's my first time working with tex and I was having evident difficulties :) Thanks for the pointer!
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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