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Limitations of Bohr Model: Explanation & Calculation

Kasturi Talukdar

Updated on 10th February, 2023 , 5 min read

Limitations of Bohr Model Overview

The Bohr model of the atom, proposed by Niels Bohr in 1913, is a simple and early model of atomic structure that explains the behavior of electrons as they revolve around a nucleus in fixed, circular orbits, each with a specific energy level. It introduced the concept of the atomic number and provided a basis for more advanced models of atomic structure.

Limitations of Bohr Model: What is Bohr's Model?

Bohr's Model of the Atom is a theoretical model of the structure of atoms that was proposed by Danish physicist Niels Bohr in 1913. According to this model, atoms consist of a small, positively charged nucleus surrounded by electrons that orbit the nucleus in well-defined energy levels, or shells. In the Bohr model, the electrons in an atom occupy distinct energy levels, and each energy level is associated with a specific orbital radius. Electrons are not allowed to occupy any energy level they wish, but only those energy levels that correspond to integer values of the angular momentum.

Limitations of Bohr Model

The limitations of Bohr model are as follows:

  1.  Electron orbits are fixed and circular, but electrons in real atoms are found to occupy cloud-like regions instead of fixed orbits.
  2. The model does not consider the behavior of electrons in high-energy states and the uncertainty principle, which states that it is not possible to determine both the position and velocity of an electron simultaneously.
  3. The Bohr model does not explain the origin of spectral lines and the electronic configuration of ions.
  4. The model assumes that electrons are in stable orbits and do not emit or absorb electromagnetic radiation, which is not entirely accurate.
  5. The model does not explain the behavior of electrons in complex atoms, such as atoms with multiple energy levels and valence electrons.
  6. The Bohr model does not explain the observed splitting of spectral lines in a magnetic field, known as the Zeeman effect.

Limitations of Bohr Model: Calculation

The Bohr model can be used to calculate the energy of an electron in a particular orbit and the frequency of light emitted or absorbed when an electron jumps between orbits. Here's a simple example:

Consider an electron in the first energy level (n=1) in a hydrogen atom. According to the Bohr model, the energy of an electron in a particular orbit is given by the equation:

E = -13.6 eV / n^2

where n is the energy level of the electron and eV (electron volts) is the unit of energy. Plugging in n = 1, we get:

E = -13.6 eV

To calculate the frequency of light emitted or absorbed when an electron jumps from one orbit to another, we use the equation:

ΔE = hf

whereΔE is the change in energy, h is Planck's constant, and f is the frequency of the light. We can rearrange this equation to solve for the frequency:

f = ΔE / h

So, for an electron moving from the n = 2 energy level to the n = 1 energy level, the change in energy is given by:

ΔE = E2 - E1 = (-13.6 eV / 4) - (-13.6 eV) = -13.6 eV / 4

And the frequency of the light emitted or absorbed is:

f = ΔE / h

Note that the value of Planck's constant is:

6.62 x 10^-34 Js.

This is a simple example of how the Bohr model can be used to calculate the energy of an electron in a particular orbit and the frequency of light emitted or absorbed when an electron jumps between orbits. The actual calculations in atomic physics can be much more complex, but the basic principles remain the same.

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Limitations of Bohr Model: Experiment

There is no single experiment that can be said to prove the Bohr model. However, a number of experiments in atomic physics have provided evidence for the principles outlined in the Bohr model, including:

  1. The study of spectral lines:The spectral lines of atoms provide evidence for the quantization of energy levels in atoms and for the idea that electrons can move between orbits by emitting or absorbing light.
  2. The measurement of the fine structure in atomic spectra: The fine structure of atomic spectra provides further evidence for the quantization of energy levels in atoms and helps to refine the ideas in the Bohr model.
  3. The study of hydrogen spectra: The spectral lines in the Balmer series of hydrogen were used to confirm the validity of the Bohr model and helped establish the concept of quantized energy levels in atoms.

These and other experiments provided crucial evidence for the validity of the Bohr model and helped lay the foundations for the development of modern atomic physics. However, it is important to note that the Bohr model is now considered a classical model and has been superseded by more sophisticated models that incorporate the principles of quantum mechanics.

Limitations of Bohr Model: Applications in Daily Life

The Bohr model has influenced the development of more advanced models of atomic structure that have practical applications in daily life. Some examples include:

  1. Medical imaging:X-ray technology uses the principles of the interaction between X-rays and electrons in atoms to produce images of bones and other internal structures.
  2. Radiation therapy: The understanding of atomic structure and electron arrangements is used in the design of radiation therapy to target cancer cells.
  3. Electronic devices: The understanding of electron behavior in atoms and their energy levels has led to the development of electronic devices such as transistors, computer chips, and other components of electronic devices.
  4. Chemistry: The concept of energy levels and electron configurations is central to the understanding of chemical reactions and the properties of substances.

Limitations of Bohr Model: Things to Remember

Here are a few key things to remember about the limitations of the Bohr Model:

  1. Only applies to hydrogen-like atoms: The Bohr law only applies to hydrogen-like atoms, which are single electron atoms, and does not accurately describe the behavior of electrons in more complex atoms with multiple electrons.
  2. Circular orbits assumption: The Bohr law assumes that electrons move in circular orbits around the nucleus, which is inconsistent with the principles of quantum mechanics, which state that electrons are described by wave functions.
  3. Ignores electron spin: The Bohr law does not take into account the spin of electrons, which is an important factor in determining the behavior of electrons in atoms.
  4. Does not account for electron-electron interactions: The Bohr law does not account for the interactions between electrons in an atom, which are crucial for determining the behavior of electrons in more complex atoms.
  5. Does not explain the stability of atoms: While the Bohr law provides a basic understanding of the energy levels of electrons in atoms, it does not fully explain the stability of atoms and why they do not collapse under their own electromagnetic forces.

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Frequently Asked Questions

What are the demerits of Bohr Model?

The specifics of the hydrogen and helium atomic spectra were beyond Bohr’s comprehension. He omitted to explain why spectral lines split in the presence of a magnetic field. He did not offer an explanation for the strength of the spectral lines.

What are the three main limitations of Bohr Model?

The 3 main limitations were: Bohr’s atomic model was unable to account for the Zeeman Effect (effect of magnetic field on the spectra of atoms). Additionally, the Stark effect was left unexplained (effect of electric field on the spectra of atoms). The spectra obtained from bigger atoms could not be explained by it.

Who founded the Bohr Model?

The Bohr model of the atom, proposed by Niels Bohr in 1913

What is the Bohr Model?

The Bohr model of the atom, proposed by Niels Bohr in 1913, is a simple and early model of atomic structure that explains the behavior of electrons as they revolve around a nucleus in fixed, circular orbits, each with a specific energy level.

What are the different atomic models?

The different atomic models proposed are: Plum Pudding Model by J.J.Thompson, Planetary Model by Ernest Rutherford, Bohr Model by Neils Bohr, and Electron Cloud Model.

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