Residue Theorem Applied to Calculating ψ(k,t)

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I have a doubt on this following procedure using the residue theorem:
Initially we have
ψ(k,t)=\frac{1}{2\pi}\int_{L_{\omega}}\frac{S(k,\omega)}{D(k,\omega)}e^{-i\omega t}d\omega
Then the author said using the residue theorem, we have
ψ(k,t)=-iƩ_{j}\frac{S(k,\omega_j(k))}{\partial D/ \partial \omega (k,\omega_j(k))}e^{-i\omega_j(k) t}
where S(k,\omega_j(k)), D(k,\omega_j(k)) are functions relating k and \omega.
What kind of residue theorem is the author using?
Thank you very much
 
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The "residue theorem" the author is using, the only one I know, is
"The integral of f(z) around a closed curve is 2\pi i times the sum of the residues at the poles of f inside the curve."
 
HallsofIvy said:
The "residue theorem" the author is using, the only one I know, is
"The integral of f(z) around a closed curve is 2\pi i times the sum of the residues at the poles of f inside the curve."

Hi,

Thanks for your reply.

I know residue theorem. I just can't relate the usage the author has displayed to the canonical form, like I found in Wiki or what you have said.

To be more specific, could you tell me how did you get the partial derivative of D w.r.t. ω in the denominator?
 
A pole occurs where D(k,\omega) = 0, at which point \omega = \omega_j(k). Locally the Taylor series for D is (for fixed k):
<br /> D(k,\omega) = (\omega - \omega_j(k))\frac{\partial D}{\partial \omega}(k,\omega_j(k)) + \dots
Thus close to \omega = \omega_j(k) (assuming S(k,\omega_j(k)) \neq 0) the integrand is approximately
<br /> \frac{S(k,\omega_j(k))}{(\omega - \omega_j(k))\frac{\partial D}{\partial \omega}(k,\omega_j(k))}e^{-i\omega_j(k)t}<br />
so the residue is
<br /> \frac{S(k,\omega_j(k))}{\frac{\partial D}{\partial \omega}(k,\omega_j(k))}e^{-i\omega_j(k)t}.<br />

I don't know where the minus sign in the original comes from; presumably the contour is being traversed clockwise instead of anticlockwise.
 
jollage said:
Hi,

Thanks for your reply.

I know residue theorem. I just can't relate the usage the author has displayed to the canonical form, like I found in Wiki or what you have said.

To be more specific, could you tell me how did you get the partial derivative of D w.r.t. ω in the denominator?
Suppose the function you are integrating has a simple pole at ##z_0##. If the function being integrated can be written in the form ##\frac{p(z)}{q(z)}##, with ##q(z_0)=0## and ##q'(z_0)\neq 0##, then its residue at the point ##z_0## is given by ##\frac{p(z_0)}{q'(z_0)}##.
 
pasmith said:
A pole occurs where D(k,\omega) = 0, at which point \omega = \omega_j(k). Locally the Taylor series for D is (for fixed k):
<br /> D(k,\omega) = (\omega - \omega_j(k))\frac{\partial D}{\partial \omega}(k,\omega_j(k)) + \dots
Thus close to \omega = \omega_j(k) (assuming S(k,\omega_j(k)) \neq 0) the integrand is approximately
<br /> \frac{S(k,\omega_j(k))}{(\omega - \omega_j(k))\frac{\partial D}{\partial \omega}(k,\omega_j(k))}e^{-i\omega_j(k)t}<br />
so the residue is
<br /> \frac{S(k,\omega_j(k))}{\frac{\partial D}{\partial \omega}(k,\omega_j(k))}e^{-i\omega_j(k)t}.<br />

I don't know where the minus sign in the original comes from; presumably the contour is being traversed clockwise instead of anticlockwise.

Thanks a lot, what you said makes sense.
 
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