diff --git a/src/lecture_1.md b/src/lecture_1.md index d7db62e8d94cf3b01ce8bc97a41db00a4efbce20..9c49766fcd2d5760e20aeaee37e9ef4525195ef6 100644 --- a/src/lecture_1.md +++ b/src/lecture_1.md @@ -19,7 +19,7 @@ Exercises: 2.3, 2.4, 2.5, 2.6, 2.8 After this lecture you will be able to: - Explain quantum mechanical effects on the heat capacity of solids (Einstein model) - - Compute occupation number, energy and heat capacity of a bosonic particle + - Compute the expected particle number, energy, and heat capacity of a quantum harmonic oscillator (a single boson) - Write down the total thermal energy of a material ### Einstein model @@ -133,7 +133,7 @@ $g(\omega)$ is the _density of states_: the number of normal modes found at each - Describe the concept of reciprocal space and allowed momenta - Write down the total energy of phonons given the temperature and the dispersion relation - - Estimate heat capacity due to phonons in high temperature and low temperature regimes + - Estimate heat capacity due to phonons in high temperature and low temperature regimes of the Debye model #### Reciprocal space, periodic boundary conditions Each normal mode can be described by a _wave vector_ ${\bf k}$. A wave vector represents a point in _reciprocal space_ or _k-space_. We can find $g(\omega)$ by counting the number of normal modes in k-space and then converting those to $\omega$. diff --git a/src/lecture_3.md b/src/lecture_3.md index c68aa827dd1c3d9bf34e48a6ed277b699ef034f5..b5a913c5dd0c9a7652a821fc7b42a04b1824a0cb 100644 --- a/src/lecture_3.md +++ b/src/lecture_3.md @@ -149,7 +149,7 @@ Therefore if each atom has a single electron in the outermost shell, these atoms - Explain the origins of interatomic forces - Compute vibrational spectra of small molecules in 1D - - Write down Hamiltonians and equations of motion of bulk materials (but not yet solve them) + - Formulate Hamiltonians and equations of motion of bulk materials (but not yet solve them) ## Adding repulsion