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1.6: First attempts to model the H atom

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    339540
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    Hydrogen Atoms Models

    Model 1: The Rutherford model

    The Coulomb force that exists between oppositely charge particles means that a positive nucleus and negative electrons should attract each other, and the atom should collapse. To prevent the collapse, the electron was postulated to be orbiting the positive nucleus. The Coulomb force (discussed below) is used to change the direction of the velocity, just as a string pulls a ball in a circular orbit around your head or the gravitational force holds the moon in orbit around the Earth. The origin for this hypothesis that suggests this perspective is plausible is the similarity of the gravity and Coulombic interactions. The expression for the force of gravity between two masses (Newton's Law of gravity) is

    \[F_{gravity} \propto \dfrac{m_1m_2}{r^2}\label{1.8.1}\]

    with

    • \(m_1\) and \(m_2\) representing the mass of object 1 and 2, respectively and
    • \(r\) representing the distance between the objects centers

    The expression for the Coulomb force between two charged species is

    \[F_{Coulomb} \propto \dfrac{Q_1Q_2}{r^2}\label{1.8.2}\]

    with

    • \(Q_1\) and \(Q_2\) representing the charge of object 1 and 2, respectively and
    • \(r\) representing the distance between the objects centers

    However this analogy has a problem too. An electron going around in a circle is constantly being accelerated because its velocity vector is changing. A charged particle that is being accelerated emits radiation. This property is essentially how a radio transmitter works. A power supply drives electrons up and down a wire and thus transmits energy (electromagnetic radiation) that your radio receiver picks up. The radio then plays the music for you that is encoded in the waveform of the radiated energy.

    Figure 1.png
    The classical death spiral of an electron around a nucleus.

    Model 2A: The Classical Bohr Atom (Electron as a Particle)

    The Bohr model is an early attempt to predict the allowed energies for single-electron atoms such as \(H\), \(He^{+}\), \(Li^{2+}\), \(Be^{3+}\), etc. Although Bohr's reasoning relies on classical concepts and hence, is not a correct explanation, the reasoning is interesting, and so we examine this model for its historical significance.

    Bohr_Theory_of_the_Atom_.jpg
    Bohr atom with an electron revolving around a fixed nucleus.

    In 1911, Niels Bohr introduced his theory on the hydrogen atom. It assumed three main points.

    1. Electrons move in circular orbitals.
    2. Electrons are confined by Coulombic force
    3. The wave nature of particles leads to quantization of energy levels of an atom.

    Calculation of the orbits requires two assumptions.

    Assumption 1: The electron is held in a circular orbit by electrostatic attraction

    The Coulombic force of the attraction between the proton and electron can be written as

    \[F_{coulombic} = \dfrac {e^2}{4\pi \epsilon_0 r^2} \label{BHeq1}\]

    where \(e\) is the charge of the electron, \(\epsilon_0\) is the perimittivity of free space, and \(r\) is the radius of the electron orbit. The Coulombic force is counterbalanced by centrifugal force

    \[F_{centrifugal} = m_e \cdot \dfrac {v^2}{r} \label{BHeq2}\]

    where \(m_e\) is the mass of the electron, and \(v\) is the speed of the electron.

    Assumption 2: The angular momentum is quantized

    Bohr assumed that angular momentum of the electron was quantized (more below)

    \[L = m_e vr = \dfrac {nh}{2\pi} \label{BH0}\]

    Setting Equations \ref{BHeq1} and \ref{BHeq2} equal to each other and solving for \(r\) and introducing Equation \ref{BH0}, the radius of the electron's orbit, gives

    \[r = \dfrac {\epsilon_0 h^2 n^2}{\pi m_e e^2}\]

    The symbol \(\hbar\) is more commonly used in quantum mechanics, which is equivalent to \(\dfrac {h}{2\pi}\), so the equation for the radius of the orbit can be written as

    \[r = \dfrac {4\pi \epsilon_0 \hbar^2 n^2}{m_e e^2} \label{BA1}\]

    Using \(n\) = \(1\), you get an \(r\) value of \(5.29 \times 10^{-11} m\). So Equation \ref{BA1} can be rewritten as

    \[r = n^2 a_o \label{BA2}\]

    where

    \[a_o = \dfrac {4\pi \epsilon_0 \hbar^2 }{m_e e^2} = 5.29 \times 10^{-11} m\]

    \(a_o\) is often called the Bohr radius (i.e. radius of an unexcited hydrogen atom).

    Example \(\PageIndex{2}\): Quantized Orbits

    A hydrogen atom is in its first excited state (\(n = 2\)). Using the Bohr theory of the atom, calculate the radius of the orbit.

    Solution
    This is a straightforward application of Equation \ref{BA2} with \(n=2\). \[ r_2 = 2^2 a_o = 4 a_o = 4 (5.29 \times 10^{-11} m) = 2.12 \times 10^{-10}\;m\] The dimensions of atoms are often expressed in nanometers (\(1\, nm = 10^{-9}\, m\)) or angstroms (\(1\, Å = 10^{-10}\,m\)). So the radius of this excited hydrogen atom is 0.212 nm or 2.12 Å.
    Fgure 2.png
    Energy levels predicted by the Bohr model. Electron transitions and their resulting wavelengths for hydrogen. Energy levels are not to scale. from Stephen Lower.

    The total energy of any system can be denoted by

    \[E = T + V\]

    the summation of the systems kinetic and potential energy, respectively. Setting the system to be an electron allows for the total energy of the electron in a Hydrogen atom to be calculated. In this case, the kinetic energy is

    \[T = \dfrac{ m_e v^2}{2}\]

    and

    \[V = - \dfrac {e^2}{4\pi \epsilon_0 r}.\]

    Thus,

    \[E = \dfrac{m_e v^2}{2} - \dfrac {e^2}{4\pi \epsilon_0 r}\]

    By substituting \(m_e v^2\) by equating \(F_{coulombic}\) and \(F_{centrifugal}\), and plugging in the Bohr radius for \(r\) (Equation \(\ref{BA1}\)) results in

    \[E_n = \dfrac {-m_e e^4}{8\epsilon^2_0 h^2} \cdot \dfrac {1}{n^2} \label{R1}\]

    or

    \[E_n = -R \dfrac {1}{n^2} \label{BA5}\]

    where \(R\) is the Rydberg constant, which is sometimes referred to as \(R_\infty\) or \(R_H\).

    The energy of an orbital is negative indicating that the negatively charged electron is bound by the positive nucleus, and therefore it requires energy to free the electron from the atom. When assuming the nuclear mass is infinite compared to the mass of the electron, the value of \(R_\infty\) is \(109737 cm^{-1}\) or \(13.6\, eV\). When properly taking the nuclear mass into account, \(R_H\) is \(109677 cm^{-1}\).

    Example \(\PageIndex{3}\): Quantized Energies

    A hydrogen atom is in its first excited state (\(n = 2\)). Using the Bohr theory of the atom, calculate the energy of the electron in this orbit.

    Solution
    This is a straightforward application of Equation \ref{BA5} with \(n=2\). \[ E_n = -R \dfrac {1}{2^2} = \dfrac{R}{4} = \dfrac{13.6\, eV}{4} = 3.4 \,eV\] The electron is higher in the Coloumbic well and hence requires less energy to remove.

    State-to-state Transitions

    A Hydrogen atom emits radiation when the e- makes a transition from a higher energy orbit (state, orbital) to a lower one. Alternatively, the electron can absorb a photon by "jumping" (changing) from one quantum state to another.

    AtomicLineSpEm.png

    For emission, the conservation of energy in the absorption transition would look like

    \[ E_{n_i} + hv = E_{n_f} \]

    and similarly for emission transition

    \[ E_{n_i} - hv = E_{n_f} \label{emission} \]

    where the energy of the state is a function of the \(n_i\) and \(n_f\) integers for the initial and final states. For emission, we can now expand Equation \ref{emission} using Equation \ref{R1}

    \[\nu=\dfrac{E_{n_i}-E_{n_f}}{h}=\dfrac{e^4 m_e}{8\epsilon_{0}^{2} h^3}\left ( \dfrac{1}{n_{f}^{2}}-\dfrac{1}{n_{i}^{2}}\right ) \label{1.8.23}\]

    Note

    Note

    It is important to differentiate the energy of a photon \( E =hv \) corresponding to a wave that propagates with speed \(c\), frequency \(v\) and wavelength \(\lambda\) and the transition energy between 2 states \(E_{n_f} - E_{n_i} =\Delta E \). Given that a transition (absorption pr emission) occurs when the change in Energy \( \Delta E\) equals the energy of a photon, we can write Equation \ref{emission}.

    We can now identify the Rydberg constant \(R_H\) and it is not phenomenological, but can be expressed in terms of basic physical constants on the right hand side of Equation \(\ref{1.8.23}\)

    \[ \begin{align*} R_H &= \dfrac {m_ee^4}{8 \epsilon ^2_0 h^3 } \\[4pt] &\approx 2.19 \times 10^{-18} J \end{align*}\]

    and in terms of wavenumbers using the \(c=\lambda \nu\) relationship

    \[ \begin{align*} R_H &= \dfrac {m_ee^4}{8 \epsilon ^2_0 h^3c } \\[4pt] &\approx 109,737 \,cm^{-1} \end{align*}\]

    A demo of both wavelength and particle like Bohr atoms: http://www.walter-fendt.de/html5/phe...hrmodel_en.htm

    Contributions and Attributions

    Adapted by Valeria D. Kleiman


    This page titled 1.6: First attempts to model the H atom is shared under a not declared license and was authored, remixed, and/or curated by Delmar Larsen.