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At our QM intro our professor said that we derive uncertainty principle using the integral of plane waves ##\psi = \psi_0(k) e^{i(kx - \omega t)}## over wave numbers ##k##. We do it at ##t=0## hence ##\psi = \psi_0(k) e^{ikx}##
<br /> \psi = \int\limits_{-\infty}^{+\infty} \psi_0\!(k) \cdot e^{ikx} \, \textrm{d} k<br />
where ##\psi_0(k)## is a ##k##-dependent normalisation factor (please correct me if I am wrong). This dependency was said to be a Gaussian function
<br /> \psi_0(k)= \psi_0 e^{i(k-k_0)^2/4\sigma k^2}<br />
where ##\psi_0## is an ordinary normalisation factor (please correct me if I am wrong).
QUESTION 1: Why do we choose ##\psi_0(k)## as a gauss function? Why is this function so appropriate in this case?
QUESTION 2: I don't know how did our professor get a gauss function with an imagnary number ##i## in it. His gauss is nothing like the one on Wikipedia which is
<br /> f(x) = a e^{-(x-b)^2/2c^2}<br />
QUESTION 3: We used the first integral i wrote down to calculate the Heisenberg's uncertainty principle like shown below, but it seems to me that most of the steps are missing and this is the reason i don't understand this. Could anyone explain to me step by step how to do this.
<br /> \begin{split}<br /> \psi &= \int\limits_{-\infty}^{+\infty} \psi_0\!(k) \cdot e^{ikx} \, \textrm{d} k\\<br /> \psi &= \int\limits_{-\infty}^{+\infty} \psi_0 e^{i(k-k_0)^2/4\sigma k^2} \cdot e^{ikx} \, \textrm{d} k\\<br /> \psi &= \psi_0 2 \sqrt{\pi} e^{ik_0x} e^{-x/2 \sigma k^2}<br /> \end{split}<br />
I think this is connected to a Gaussian integral, but it doesn't look quite like it to me. Well in the end our professor just says that out of the above it follows that
<br /> \boxed{\delta x \delta k = \frac{1}{2}} <br />
I don't understand this neither. It was way too fast or me.
<br /> \psi = \int\limits_{-\infty}^{+\infty} \psi_0\!(k) \cdot e^{ikx} \, \textrm{d} k<br />
where ##\psi_0(k)## is a ##k##-dependent normalisation factor (please correct me if I am wrong). This dependency was said to be a Gaussian function
<br /> \psi_0(k)= \psi_0 e^{i(k-k_0)^2/4\sigma k^2}<br />
where ##\psi_0## is an ordinary normalisation factor (please correct me if I am wrong).
QUESTION 1: Why do we choose ##\psi_0(k)## as a gauss function? Why is this function so appropriate in this case?
QUESTION 2: I don't know how did our professor get a gauss function with an imagnary number ##i## in it. His gauss is nothing like the one on Wikipedia which is
<br /> f(x) = a e^{-(x-b)^2/2c^2}<br />
QUESTION 3: We used the first integral i wrote down to calculate the Heisenberg's uncertainty principle like shown below, but it seems to me that most of the steps are missing and this is the reason i don't understand this. Could anyone explain to me step by step how to do this.
<br /> \begin{split}<br /> \psi &= \int\limits_{-\infty}^{+\infty} \psi_0\!(k) \cdot e^{ikx} \, \textrm{d} k\\<br /> \psi &= \int\limits_{-\infty}^{+\infty} \psi_0 e^{i(k-k_0)^2/4\sigma k^2} \cdot e^{ikx} \, \textrm{d} k\\<br /> \psi &= \psi_0 2 \sqrt{\pi} e^{ik_0x} e^{-x/2 \sigma k^2}<br /> \end{split}<br />
I think this is connected to a Gaussian integral, but it doesn't look quite like it to me. Well in the end our professor just says that out of the above it follows that
<br /> \boxed{\delta x \delta k = \frac{1}{2}} <br />
I don't understand this neither. It was way too fast or me.