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The Oxford Solid State Basics

Steven H. Simon

Chapter 6

What Holds Solids Together: Chemical Bonding - all with Video Answers

Educators


Chapter Questions

02:02

Problem 1

Chemical Bonding
(a) Qualitatively describe five different types of chemical bonds and why they occur.

D Describe which combinations of what types of atoms are expected to form which types of bonds (make reference to location on the periodic table).
D. Describe some of the qualitative properties of materials that have these types of bonds.
(Yes, you can just copy the table out of the chapter summary, but the point of this exercise is to learn the information in the table!)
(b) Describe qualitatively the phenomenon of van der Waals forces. Explain why the force is attractive and proportional to $1 / R^{7}$ where $R$ is the distance between two atoms.

Lottie Adams
Lottie Adams
Numerade Educator
01:57

Problem 2

Covalent Bonding in Detail*
(a) Linear Combination of Atomic Orbitals:
In Section $6.2 .2$ we considered two atoms each with a single atomic orbital. We called the orbital $|1\rangle$ around nucleus 1 and $|2\rangle$ around nucleus 2 . More generally we may consider any set of wavefunctions $|n\rangle$ for $n=1, \ldots, N$. For simplicity, let us assume this basis is orthonormal $\langle n \mid m\rangle=\delta_{n, m}$ (More generally, one cannot assume that the basis set of orbitals is orthonormal. In Exercise $6.5$ we properly consider a non-orthonormal basis.)
Let us write a trial wavefunction for our ground state as
$$
|\Psi\rangle=\sum_{n} \phi_{n}|n\rangle
$$
This is known as a linear combination of atomic orbitals, LCAO, or tight binding (it is used heavily in numerical simulation of molecules).
We would like to find the lowest-energy wavefunction we can construct in this form, i.e., the best approximation to the actual ground-state wavefunction. (The more states we use in our basis, generally, the more aocurate our results will be.) We claim that the ground state is given by the solution of the effective Schroedinger equation
$$
\mathcal{H} \phi=E \phi
$$
where $\phi$ is the vector of $N$ coefficients $\phi_{n}$, and $\mathcal{H}$ is the $N$ by $N$ matrix
$$
\mathcal{H}_{n, m}=\langle n|H| m\rangle
$$
with $H$ the Hamiltonian of the full system we are considering. To prove this, let us construct the energy
$$
E=\frac{\langle\psi|H| \psi\rangle}{\langle\psi \mid \psi\rangle}
$$
D Show that minimizing this energy with respect to each $\phi_{n}$ gives the same eigenvalue equation, Eq. 6.13. (Caution: $\phi_{n}$ is generally complex! If you are not comfortable with complex differentiation, write everything in terms of real and imaginary parts of each $\phi_{n}$.) Similarly, the second eigenvalue of the effective Schroedinger equation will be an approximation to the first excited state of the system.
(b) Two-orbital covalent bond
Let us return to the case where there are only two orbitals in our basis. This pertains to a case where we have two identical nuclei and a single electron which will be shared between them to form a covalent bond. We write the full Hamiltonian as
$$
H=\frac{\mathrm{p}^{2}}{2 m}+V\left(\mathrm{r}-\mathrm{R}_{1}\right)+V\left(\mathrm{r}-\mathrm{R}_{2}\right)=K+V_{1}+V_{2}
$$
where $V$ is the Coulomb interaction between the electron and the nucleus, $R_{1}$ is the position of the first nucleus and $R_{2}$ is the position of the second nucleus. Let $\in$ be the energy of the atomic orbital around one nucleus in the absence of the other. In other words
$$
\begin{aligned}
&\left(K+V_{1}\right)|1\rangle=\epsilon|1\rangle \\
&\left(K+V_{2}\right)|2\rangle=\epsilon|2\rangle
\end{aligned}
$$
Define also the cross-energy element
$$
V_{\text {cross }}=\left\langle 1\left|V_{2}\right| 1\right\rangle=\left\langle 2\left|V_{1}\right| 2\right\rangle
$$
and the hopping matrix element
$$
t=-\left\langle 1\left|V_{2}\right| 2\right\rangle=-\left\langle 1\left|V_{1}\right| 2\right\rangle
$$
These are not typos!
D. Why can we write $V_{\text {cross }}$ and $t$ equivalently using either one of the expressions given on the righthand side?

D. Show that the eigenvalues of our Schroedinger equation Eq. $6.13$ are given by
$$
E=\epsilon+V_{\text {eross }} \pm|t|
$$
D. Argue (perhaps using Gauss's law) that $V_{\text {cross }}$ should roughly cancel the repulsion between nuclei, so that, in the lower eigenstate the total energy is indeed lower when the atoms are closer together.
p. This approximation must fail when the atoms get sufficiently close. Why?

Anand Jangid
Anand Jangid
Numerade Educator
01:58

Problem 3

LCAO and the Ionic-Covalent Crossover
For Exercise 6.2.b consider now the case where the atomic orbitals $|1\rangle$ and $|2\rangle$ have unequal energies $\epsilon_{0,1}$ and $\epsilon_{0,2}$. As the difference in these two energies increases show that the bonding orbital becomes more localized on the lower-energy atom. For simplicity you may use the orthogonality assumption $\langle 1 \mid 2\rangle=0 .$ Explain how this calculation can be used to describe a crossover between covalent and ionic bonding.

Natalie Johns
Natalie Johns
Numerade Educator
04:02

Problem 4

Ionic Bond Energy Budget
The ionization energy of a sodium atom is about $5.14 \mathrm{eV}$. The electron affinity of a chlorine atom is about $3.62 \mathrm{eV}$. When a single sodium atom bonds with a single chlorine atom, the bond length is roughly $0.236 \mathrm{~nm}$. Assuming that the cohesive energy is purely Coulomb energy, calculate the total energy released when a sodium atom and a chlorine atom come together to form a $\mathrm{NaCl}$ molecule. Compare your result to the experimental value of $4.26 \mathrm{eV}$. Qualitatively account for the sign of your error.

Naresh Bagrecha
Naresh Bagrecha
Numerade Educator
14:05

Problem 5

LCAO Done Right*
(a) * In Exercise $6.2$ we introduced the method of linear combination of atomic orbitals. In that exercise we assumed that our basis of orbitals is orthonormal. In this exercise we will relax this assumption.
Consider now many orbitals on each atom (and potentially many atoms). Let us write
$$
|\psi\rangle=\sum_{i=1}^{N} \phi_{i}|i\rangle
$$
for an arbitrary number $N$ of orbitals. Let us write the $N$ by $N$ overlap matrix $\mathcal{S}$ whose elements are
$$
\mathcal{S}_{i, j}=\langle i \mid j\rangle
$$
In this case do not assume that $\mathcal{S}$ is diagonal.
Using a similar method as in Exercise 6.2, derive the new "Schroedinger equation"
with the same notation for $\mathcal{H}$ and $\phi$ as in Exercise 6.2. This equation is known as a "generalized eigenvalue problem" because of the $\mathcal{S}$ on the right-hand side.
(b) ** Let us now return to the situation with only two atoms and only one orbital on each atom but such that $\langle 1 \mid 2\rangle=\mathcal{S}_{1,2} \neq 0$. Without loss of generality we may assume $\langle i \mid i\rangle=1$ and $S_{1,2}$ is real. If the atomic orbitals are s-orbitals then we may assume also that $t$ is real and positive (why?).
Use Eq. $6.14$ to derive the eigenenergies of the system.

Susan Hallstrom
Susan Hallstrom
Numerade Educator
01:57

Problem 6

Van der Waals Bonding in Detail*
(a) Here we will do a much more precise calculation of the van der Waals force between two hydrogen atoms. First, let the positions of the two nuclei be separated by a vector $\mathbf{R}$, and let the vector from nucleus 1 to electron 1 be $\mathbf{r}_{1}$ and let the vector from nucleus 2 to electron 2 be $\mathbf{r}_{2}$ as shown in the following figure.

Let us now write the Hamiltonian for both atoms (assuming fixed positions of nuclei, i.e., using BornOppenheimer approximation) as
$$
\begin{aligned}
H &=H_{0}+H_{1} \\
H_{0} &=\frac{\mathbf{p}_{1}^{2}}{2 m}+\frac{\mathbf{p}_{2}^{2}}{2 m}-\frac{e^{2}}{4 \pi \epsilon_{0}\left|\mathbf{r}_{1}\right|}-\frac{e^{2}}{4 \pi \epsilon_{0}\left|\mathbf{r}_{2}\right|} \\
H_{1} &=\frac{e^{2}}{4 \pi \epsilon_{0}|\mathbf{R}|}+\frac{e^{2}}{4 \pi \epsilon_{0}\left|\mathbf{R}-\mathbf{r}_{1}+\mathbf{r}_{2}\right|} \\
&-\frac{e^{2}}{4 \pi \epsilon_{0}\left|\mathbf{R}-\mathbf{r}_{1}\right|}-\frac{e^{2}}{4 \pi \epsilon_{0}\left|\mathbf{R}+\mathbf{r}_{2}\right|}
\end{aligned}
$$
Here $H_{0}$ is the Hamiltonian for two non-interacting hydrogen atoms, and $H_{1}$ is the interaction between the atoms.
Without loss of generality, let us assume that $\mathbf{R}$ is in the $x$ direction. Show that for large $\mathbf{R}$ and small $\mathrm{r}_{i}$, the interaction Hamiltonian can be written as
$$
H_{1}=\frac{e^{2}}{4 \pi \epsilon_{0}|\mathbf{R}|^{3}}\left(z_{1} z_{2}+y_{1} y_{2}-2 x_{1} x_{2}\right)+\mathcal{O}\left(1 / R^{4}\right)
$$
where $x_{i}, y_{i}, z_{i}$ are the components of $\mathrm{r}_{1}$. Show that this is just the interaction between two dipoles.
(b) Perturbation Theory:
The eigenvalues of $H_{0}$ can be given as the eigenvalues of the two atoms separately. Recall that the eigenstates of hydrogen are written in the usual notation as $|n, l, m\rangle$ and have energies $E_{n}=$ $-\mathrm{Ry} / n^{2}$ with $\mathrm{Ry}=m e^{4} /\left(32 \pi^{2} \epsilon_{0}^{2} \hbar^{2}\right)=e^{2} /\left(8 \pi \epsilon_{0} \alpha_{0}\right)$ the Rydberg (here $l \geqslant 0,|m| \leqslant l$ and $n \geqslant$
$l+1)$. Thus the eigenstates of $H_{0}$ are written as $\left.\mid n_{1}, l_{l}, m_{1} ; n_{2}, l_{2}, m_{2}\right)$ with energies $E_{n_{1}, n_{2}}=$ $-\mathrm{Ry}\left(1 / n_{1}^{2}+1 / n_{2}^{2}\right)$. The ground state of $H_{0}$ is $|1,0,0 ; 1,0,0\rangle$.
D Perturbing $H_{0}$ with the interaction $H_{1}$, show that to first order in $H_{1}$ there is no change in the ground-state energy. Thus conclude that the leading correction to the grotund-state energy is proportional to $1 / R^{6}$ (and hence the force is proportional to $1 / R^{7}$ ).
D Recalling second-order perturbation theory show that we have a correction to the total energy given by
$$
\delta E=
$$
$\sum_{n_{1}, n_{2}} \begin{aligned}&|<1,0,0 ; 1,0,0| H_{1} \mid n_{1}, l_{l}, m_{1} ; n_{2}, l_{2} \\&l_{1}, l_{2} \atop m_{1}, m_{2}\end{aligned}$ $$ \begin{array}{l}\text { E0,0 }-E_{n_{1}, n_{2}} \\ \text { Show that the force must be attractive. }\end{array} $$
(c)*Bounding the binding eneryy:
First, show that the numerator in this expression is zero if either $n_{1}=1$ or $n_{2}=1$. Thus the smallest $E_{n_{1}, n_{2}}$ that appears in the denominator is $E_{2,2}$. If we replace $E_{n_{1}, n_{2}}$ in the denominator with $E_{2,2}$ then the $|\delta E|$ we calculate will be greater than than the $|\delta E|$ in the exact calculation. On the other hand, if we replace $E_{n_{1}, n_{2}}$ by 0 , then the $|\delta E|$ will always be less than the $\delta E$ of the exact calculation.
D Make these replacements, and perform the remaining sum by identifying a complete set. Derive the bound
at the force must be attractive.
$g$ the binding energy:
that the numerator in this expression
her $n_{1}=1$ or $n_{2}=1$. Thus the small-
that appears in the denominator is $E_{2,2}$.
the exact calculation. On the other
replace $E_{n_{1}, n_{2}}$ by 0, then the $|\delta E|$ will
ws than the $\delta E$ of the exact calculation.
ese replacements, and perform the re-
by identifying a complete set. Derive

Anand Jangid
Anand Jangid
Numerade Educator