DeldotB
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Homework Statement
Suppose that two neutrinos are created in the sun - call the states |{ \nu_1}\rangle and |{ \nu_2}\rangle.
(Among many other things) I am asked to show that once the neutrinos have propigated a distance x after a time t, the states satisfy:
|{ \nu_1}(x,t)\rangle = e^{i \phi_1} | \nu_1(0,0) \rangle
|{ \nu_2}(x,t)\rangle = e^{i \phi_2} | \nu_2(0,0) \rangle
Where \phi_{1,2} = k_ix-E_it/ \hbar where k_i= \sqrt{2m_iE/ \hbar^2}
Homework Equations
Schrodinger Equation
The Attempt at a Solution
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This seems very simple, but I am missing a factor:
Solving the time independent schrodinger equation yields: | \nu_1 (0,0) \rangle = e^{-ikx} where k= \sqrt{2mE/ \hbar^2}.
Tagging on time dependence yields: | \nu_1 (t) \rangle = e^{-ikx} e^{-iEt/ \hbar}= e^{-iEt/ \hbar} | \nu_1 (0,0) \rangle.
So my question is: I tagged on the time dependence factor (from solving the time dependent s.e) and I got e^{-iEt/ \hbar} | \nu_1 (0,0) \rangle. But the problem states after the neutrinos have propigated a distance x after a time t. But isn't the "distance x" tied up in | \nu_1 (0,0) \rangle = e^{-ikx} ?
Why are the solutions of the form |{ \nu_1}(x,t)\rangle = e^{i (k_ix-E_it/ \hbar)} | \nu_1(0,0) \rangle instead of just |{ \nu_1}(x,t)\rangle = e^{iE_it/ \hbar} | \nu_1(0,0) \rangle?
I hope this makes sense. Thanks in advance!