Introduction
Neil Bohr was a Danish physicist
who put forward a theory in 1913 regarding the atomic structure of the atom
known as the Bohr’s atomic model. His ideas were quite different from the
classical model in fact, he was one of the first scientist to use the quantum
model. In his experiment he used the Hydrogen atom (Z= 1) to describe the
atomic structure of the atom.
Once Einstein extended planks idea
of energy quantization to the electromagnetic radiation other physicist made
the similar strides. Neil Bohr was constantly searching for the exact structure
of the atom. In his mind he constantly faces following questions.
If an atom has positively charged
protons and negatively charged electrons, why are they stable? Why don’t they
collide with each other despite being positively charged? What are these
emission spectra lines that we see of different types of elements and why they
emit different colors?
Bohr then tried to answer this
question with his model extending the idea of energy quantization and said that
potential energy of electron in the Hydrogen atom is also quantized. The
postulates of his model are as follows.
- The electrons revolve around the nucleus in a fix energy level which are called as shells.
- He said that each electron in different energy levels have different energies. An electron can move from one energy level to another energy level when it absorbs or emit photon. ΔEelectron = Ephoton
OR ΔE = hf = Ei − Ef
- The energy levels are represented by integers like (n = 1, 2, 3….). The shells are also be named as (K, L, M…), the lowest energy level is also called as ground state.
- He also put forward the mathematical formula for Angular momentum,
ℓ = angular momentum
n = principal quantum number
h = Planck’s constant
π = 3.14
LIMITATIONS OF THE BOHR’S ATOMIC MODEL
- Because it considers electrons to have both a known radius and orbit, it infringes the Heisenberg Uncertainty Principle.
- The Bohr Model gives an inaccurate value for the orbital angular momentum of the lowest energy state.
- It has a terrible track record when it comes to predicting the spectra of heavier elements.
- The relative intensities of spectral lines are not predicted.
- Fine and hyperfine structure in spectral lines is not explained
- It doesn't account for the Zeeman Effect.
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