# Born-Oppenheimer approximation

The aim of this section is to study the quantum description of the molecular bond. We are going to limit the analysis to diatomic molecules. First of all we consider a molucule composed by two atomic nuclei A and B, whose positions are defined by vectors ${\displaystyle {\vec {R}}_{A}}$ and ${\displaystyle {\vec {R}}_{B}}$. The electrons positions are instead identified by ${\displaystyle {\vec {x}}_{i}}$. Both nuclei and electrons positions are refered to the center of mass of the two nuclei. The Hamiltonian we can write for a system like this is:

${\displaystyle {\hat {H}}={\hat {T_{N}}}+{\hat {T_{e}}}+U_{eN}+U_{ee}+U_{NN}}$

where ${\displaystyle {\hat {T_{N}}}}$ and ${\displaystyle {\hat {T_{e}}}}$ are the kinetic energies associated respectively to the nuclei and the electrons and ${\displaystyle U_{eN},U_{ee}}$ and ${\displaystyle U_{NN}}$ represent the Coulomb interactions. Now it's possible to isolate from this Hamiltonian an electron Hamiltonian:

${\displaystyle {\hat {H_{e}}}={\hat {T_{e}}}+U_{eN}+U_{ee}}$

This ${\displaystyle {\hat {H_{e}}}}$ is a function of the nuclei positions and we can obtain an eigenvalues equation for the electrons:

${\displaystyle {\hat {H_{e}}}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)\psi _{n}^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace ;\left\lbrace {\vec {x}}_{i}\right\rbrace \right)=E_{n}^{el}\psi _{n}^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace ;\left\lbrace {\vec {x}}_{i}\right\rbrace \right)}$

It's possible to demonstrate that solving this equation for the electrons Hamiltonian leads to a solution ${\displaystyle \psi }$ for the original complete eigenvalue equation which has the form:

${\displaystyle \psi =\sum _{n}\chi _{n}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)\psi _{n}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace ;\left\lbrace {\vec {x}}_{i}\right\rbrace \right)}$

where ${\displaystyle \chi _{n}}$ is a wave function depending only on the nuclei positions. Such an equation is difficult to solve, but it can be semplified through the Born-Oppenheimer adiabatic approximation. This model is based on the fact that the mass of the nucleus is much greater than the electron one (${\displaystyle m_{p}/m_{e}\approx 1800}$). Being so, we can state that electrons move way faster than nuclei. Hence we can assume that electrons follow the motion of the nuclei without changing the energy level they belong to. In other words, there is no energy exchange between nuclei and electrons. In this adiabatic approximation the solution ${\displaystyle \psi }$ becomes:

${\displaystyle \psi =\chi _{n}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)\psi _{n}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace ;\left\lbrace {\vec {x}}_{i}\right\rbrace \right)}$

The sum over the quantum number ${\displaystyle n}$ disappears, because of the impossibility for an electron to jump to an excited state. Now we can use theese results to write an equation for the total Hamiltonian:

${\displaystyle \left({\hat {T_{N}}}+U_{NN}+{\hat {H_{e}}}\right)\chi _{n}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)\psi _{n}^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace ;\left\lbrace {\vec {x}}_{i}\right\rbrace \right)=E_{tot}\chi _{n}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)\psi _{n}^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace ;\left\lbrace {\vec {x}}_{i}\right\rbrace \right)}$

At this point we can observe that ${\displaystyle {\hat {H_{e}}}}$ only acts on ${\displaystyle \psi ^{el}}$, which is actually an eigenstate of ${\displaystyle {\hat {H_{e}}}}$, so we can substitute ${\displaystyle {\hat {H_{e}}}}$ in the equation above with the corresponding eigenvalue ${\displaystyle E^{el}\left({\vec {R}}_{i}\right)}$. Moreover, again thanks to the greatness of nuclei masses in respect to electrons ones, we can assume that the application of the kinetic term ${\displaystyle {\hat {T_{N}}}}$ to the ${\displaystyle \psi ^{el}}$ component of the total wave function gives a negligible contribution, then we can consider that ${\displaystyle {\hat {T_{N}}}}$ acts only on ${\displaystyle \chi }$. Relying on this last approximation, it's possibile to semplify the ${\displaystyle \psi ^{el}}$ term in order to obtain an eigenvalues equation for the sole ${\displaystyle \chi }$ function:

${\displaystyle \left[{\hat {T_{N}}}+U_{NN}+E_{n}^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)\right]\chi \left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)=E_{tot}\chi \left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)}$

The last equation describes the nuclei dynamics and this means that the equations for ${\displaystyle \psi ^{el}}$ and ${\displaystyle \chi }$ are now uncoupled. ${\displaystyle E_{tot}}$ depends only on the distance between the nuclei:

${\displaystyle E_{tot}=E_{tot}\left(\left|{\vec {R}}_{A}-{\vec {R}}_{B}\right|\right)}$

Now we can redefine the quantity ${\displaystyle E^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)}$ considering that ${\displaystyle U_{NN}}$ is just a moltiplicative operator:

${\displaystyle E^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)=E_{n}^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)+U_{NN}}$

In other words, ${\displaystyle E^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)}$ is the eigenvalue for the operator ${\displaystyle {\hat {H}}_{e}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)+U_{NN}}$ corresponding to the eigenfunction ${\displaystyle \psi ^{el}}$. It's possible to plot ${\displaystyle E^{el}\left(\left\lbrace {\vec {R}}_{i}\right\rbrace \right)}$ in respect to the nuclear distance ${\displaystyle R=\left|{\vec {R}}_{A}-{\vec {R}}_{B}\right|}$:

In the graph, the value of the energy in correspondence of the ${\displaystyle x}$ axis is ${\displaystyle E_{A}+E_{B}}$, where ${\displaystyle E_{A}}$ and ${\displaystyle E_{B}}$ are the energy associated to the idrogenoid Hamiltonian for nucleus ${\displaystyle A}$ and ${\displaystyle B}$. It can be seen that there is an ${\displaystyle R_{min}}$ at which the energy is minimal. This is called dissociation energy and it's the energy that has to be given to the molecule in order to break the bond.