where $m_e$ is the free electron mass. This is expected because the free elctrons are not subject to a potential
where $m_e$ is the free electron mass. This is expected because the free electrons are not subject to a potential
#### Question 5.
If the dispersion relation is parabolic, so in the free electron model.
The effective mass is given by the curvature of the dispersion. Therefore, if the dispersion has a constant curvature, the effective mass is the same for all $k-$values. This is the case for the purely parabolic dispersion $\epsilon(k)\propto^2$ of the free electron model
## Exercise 1: Lattice vibrations
#### Question 1.
The group velocity is given by
\begin{align}
v_g(k)&=\frac{\partial \omega(k)}{\partial k}\\
&= a \sqrt{\frac{\kappa}{m}}\cos(\frac{ka}{2}) \frac{\sin(ka/2)}{|\sin(ka/2)|},
\end{align}
which can be written as
$$
v_g = a \sqrt{\frac{\kappa}{m}}
\begin{cases}
&\cos(\frac{ka}{2}), 0<ka<\pi\\
&-\cos(\frac{ka}{2}), -\pi<ka<0
\end{cases}
v_g(k)=\frac{\partial \omega(k)}{\partial k} = a \sqrt{\frac{\kappa}{m}}\cos(\frac{ka}{2}) \text{sign}(k),
$$
where $\text{sign}(k)$ represents the sign of $k$.
=\frac{2L}{a \pi} \frac{1}{\sqrt{4\kappa / m - \omega^2}},
$$
where we substituted back the dispersion relation.
#### Question 3.
...
...
@@ -109,29 +100,40 @@ Hint: The group velocity is given as $v = \frac{d\omega}{dk}$, draw a coordinate
#### Question 1.
For the energy we have: $$\langle E \rangle = \int \hbar \omega g(\omega) (n_{BE}(\hbar \omega) + \frac{1}{2})d\omega$$ with $g(\omega)$ being the DOS calculated in exercise 1 and $n_{BE}(\hbar \omega) = \frac{1}{e^{\hbar\omega/k_BT}-1}$.
For the energy we have:
$$
U = \int \hbar \omega g(\omega) (n_{BE}(\hbar \omega) + \frac{1}{2})d\omega
$$
with $g(\omega)$ the density of states calculated in exercise 1 and $n_{BE}(\hbar \omega) = \frac{1}{e^{\hbar\omega/k_BT}-1}$ the Bose-Einstein distribution.
#### Question 2.
For the heat capacity we have: $$C = \frac{d \langle E \rangle}{d T} = \int g(\omega) \hbar\omega \frac{d n_{BE}(\hbar \omega)}{d T}d\omega$$
For the heat capacity we have:
$$
C = \frac{d U }{d T} = \int g(\omega) \hbar\omega \frac{d n_{BE}(\hbar \omega)}{d T}d\omega
$$
## Exercise 3: Next-nearest neighbors chain
#### Question 1.
The Schrödinger equation is given by: $|\Psi\rangle = \sum_n \phi_n |n\rangle$ such that we find $$ E\phi_n = E_0\phi_n - t\phi_{n-1} - t\phi_{n+1} - t'\phi_{n-2} - t'\phi_{n+2}$$
The Schrödinger equation is $H|\Psi\rangle = E|\Psi\rangle$. The wavefunction is $|\Psi\rangle = \sum_m \phi_m |m\rangle$. By calculating $\langle n |H|\Psi\rangle$, we find