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To recap. When an electron is bound to a nucleus (which is just a proton for Hydrogen), only a certain set of wavefunction are allowed. This is the so-called orbital model or cloud model of atoms (see Fig. "Cloud Model").

The cloud represents where we are more likely to find the electron.

These waves are quantized. For each wave we can calculate the energy of the electron. Because of the shape of the potential well, the formula for the energy is just

E_n = -\frac{E_1}{n^2}

As always, the integer n is 1,2,3,. . . If you compare this formula to the electron in a box, you see that it is inverted. This is special to the hydrogen atom. Note the very important minus sign. For the electron to be bound, the energy must be negative.

The ground state energy E_1 is a function of the masses and charges of the proton and electron. We know those, so this number is known as well. It is

E_1 = 13.6 ; \rm{eV}.

Spectroscopy

We now have the energy levels for the hydrogen atom (see Fig. "Energy Levels H").

The figure above is important to understand. The various levels of energy are also called states. If you have a hydrogen atom with the electron in level 2, we say that the atom is in the state n=2. We call that state the first excited state, since it is the first state above the ground state E_1.

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