Electron on Helium Surface: Difference between revisions
(New page: An electron close to the surface of liquid helium experiences an attractive force due to the electrostatic polarization of the helium and a repulsive force due to the exclusion principle(h...) |
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\begin{cases} | \begin{cases} | ||
-\frac{Q^2e^2}{z} &\mbox{if} \qquad z>0\\ | -\frac{Q^2e^2}{z} &\mbox{if} \qquad z>0\\ | ||
\infty &\mbox{if} \qquad else | |||
\end{cases} | \end{cases} | ||
</math> | </math> | ||
Note: the potential is infinite when <math>z<=0</math> because the cannot penetrate the helium surface. | |||
(a) Solve the | |||
(a) Solve the Schrödinger equation. Find the Eingenenergies and Eigenvalues. | |||
(b) An electric field is turned on at t=0 which produces the perturbation: | (b) An electric field is turned on at t=0 which produces the perturbation: | ||
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== Solution...== | == Solution...== | ||
(a) Solve the Schrödinger equation. | |||
<math> H = -\frac{\hbar^2}{2m}\nabla^2 + V(z) </math> | |||
The Schrödinger equation for when <math>z>0</math> is: | |||
<math> | |||
\left[ | |||
\frac{\hbar^2}{2m} \left( | |||
\frac{\partial ^2}{\partial x^2} + | |||
\frac{\partial ^2}{\partial y^2} + | |||
\frac{\partial ^2}{\partial z^2} \right) | |||
-\frac{Q^2e^2}{z} | |||
\right] \psi (\mathbf{r}) | |||
= E\psi (\mathbf{r}) | |||
</math> | |||
Using separation of variables: | |||
<math> \psi (x,y,z) = X(x)Y(y)Z(z) </math> | |||
For X and Y we get place waves. | |||
<math> X(x)Y(y) = Ae^{i(k_x x + k_y y)} </math> | |||
This corresponds to motion parallel to the helium surface. | |||
For z-component the Schroedinger equation becomes: | |||
<math> | |||
\left[ | |||
\frac{\hbar^2}{2m}\frac{\partial ^2}{\partial z^2} - | |||
\frac{Q^2e^2}{z} | |||
\right] Z(z) = | |||
</math> | |||
This has the same form as the hydrogin atom with l=0 (s-wave). Since similar equations have similar solutions, the solution to the z-component is: | |||
<math> Z(z) = zR_{n0}(z) </math> | |||
where | |||
<math> | |||
R_{10} = \left( \frac{1}{a_0} \right) ^{3/2} z e^{ -\frac{z}{a_0} } | |||
</math> | |||
<math> | |||
R_{20} = \left( \frac{1}{2a_0} \right) ^{3/2} | |||
\left( 2-\frac{z}{a_0} \right) e^{ -\frac{z}{2a_0} } | |||
</math> | |||
The total wave function and energies are: | |||
<math> \psi = Ae^{i(k_x x + k_y y)}zR_{n0}(z) </math> | |||
<math> | |||
E_{k_xK_yK_z} = \frac{\hbar^2}{2m} | |||
\left( k_x^2 + k_y^2 \right) -\frac{Q^4e^4m}{2\hbar^2n^2} | |||
</math> | |||
where n = 1,2,... is the quantum number for the z-direction | |||
and the bohr radius has become | |||
<math> a_0 = \frac{\hbar^2}{mQ^2e^2} </math> | |||
(b) Turn on electric field at t=0. | |||
The electric field introduces a perturbation to the hamiltonian: | |||
<math> V_t = eE_0ze^{t/\tau} </math> | |||
From expression 2.1.10 in [http://wiki.physics.fsu.edu/wiki/index.php/Phy5646#Formalism Time Dependent Perturbation] Section of the PHY5646 page: | |||
<math>\begin{align} | |||
P_{1 \rightarrow 2}(t \rightarrow \infty) | |||
&= |\langle n|\psi(t)\rangle|^2 | |||
\\ | |||
&= \left|\frac{1}{i\hbar}\int_{0}^{\infty}dt' | |||
e^{\frac{i}{\hbar}(E_2 - E_1)t'} | |||
\langle \psi_{n=2}|V_{t'}| \psi_{n=1}\rangle\right|^2 | |||
\\ | |||
&= \frac{e^2E_0^2}{\hbar^2} | |||
\frac{1}{\omega_{21}^2 + \frac{1}{\tau}} | |||
\left| \langle \psi_{n=2}(z) | z | \psi_{n=1}(z) \rangle \right|^2 | |||
\end{align}</math> | |||
<math>\begin{align} | |||
\langle \psi_{n=2}(z) | z | \psi_{n=1}(z) \rangle | |||
&= \langle zR{20} | z | zR_{10} \rangle | |||
\\ | |||
&= \int_{0}^{\infty} dz z^3 e^{ \frac{3}{2} \frac{z}{a_0}} \left( 2 - \frac{z}{a_0} \right) | |||
\left[ \frac{1}{ \left( \int_{0}^{\infty} dz z^2 e^{\frac{-2z}{a_0}} \right)^{1/2} | |||
\left( \int_{0}^{\infty} dz z^2 \left(2 - \frac{z}{a_0} \right)^2 e^{\frac{-z}{a_0}} \right)^{1/2} | |||
} \right] | |||
\end{align}</math> | |||
where the quantity inside the brackets is the normalization for <math> \psi_1 </math> and <math> \psi_2 </math>, respectively. | |||
let <math> x = \frac{z}{a_0} </math> | |||
<math>\begin{align} | |||
\langle \psi_{n=2}(z) | z | \psi_{n=1}(z) \rangle | |||
&\rightarrow | |||
a_0 \int_{0}^{\infty} dx x^3 e^{ \frac{3}{2} x } \left( 2 - x \right) | |||
\left[ \frac{1}{ \left( \int_{0}^{\infty} dx x^2e^{-2x} \right)^{1/2} | |||
\left( \int_{0}^{\infty} dx x^2 \left( 2 - x \right)^2 e^{ -x } \right)^{1/2} | |||
} \right] | |||
\\ | |||
&= a_0 \frac{3}{2} \sqrt{2}{81} | |||
\end{align}</math> | |||
So the probablity of a transition from ground state to the first excited state is: | |||
<math> | |||
P_{1 \rightarrow 2} = \frac{e^2E_0^2}{\hbar^2} \frac{1}{ \omega_{21}^2 + \frac{1}{\tau^2} } \frac{2^{11}}{3^{8}} | |||
</math> |
Latest revision as of 19:51, 26 April 2010
An electron close to the surface of liquid helium experiences an attractive force due to the electrostatic polarization of the helium and a repulsive force due to the exclusion principle(hard core). To a reasonable approximation for the potential when helium fills the space where :
Note: the potential is infinite when because the cannot penetrate the helium surface.
(a) Solve the Schrödinger equation. Find the Eingenenergies and Eigenvalues.
(b) An electric field is turned on at t=0 which produces the perturbation:
If the electron is initially in its ground state, find the probability makes a transition to its first excited state for times .
Solution...
(a) Solve the Schrödinger equation.
The Schrödinger equation for when is:
Using separation of variables:
For X and Y we get place waves.
This corresponds to motion parallel to the helium surface.
For z-component the Schroedinger equation becomes:
This has the same form as the hydrogin atom with l=0 (s-wave). Since similar equations have similar solutions, the solution to the z-component is:
where
The total wave function and energies are:
where n = 1,2,... is the quantum number for the z-direction and the bohr radius has become
(b) Turn on electric field at t=0.
The electric field introduces a perturbation to the hamiltonian:
From expression 2.1.10 in Time Dependent Perturbation Section of the PHY5646 page:
where the quantity inside the brackets is the normalization for and , respectively.
let
So the probablity of a transition from ground state to the first excited state is: