The paradox defined by Heisenberg’s uncertainty principle and also the wavelike nature of subatomic corpuscle such together the electron do it difficult to use the equations of timeless physics to explain the motion of electrons in atoms. Scientists essential a new approach the took the wave behavior of the electron right into account. In 1926, an Austrian physicist, Erwin Schrödinger (1887–1961; Nobel prize in Physics, 1933), developed wave mechanics, a mathematical an approach that defines the relationship in between the movement of a fragment that exhibits wavelike properties (such together an electron) and its allowed energies.
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Erwin Schrödinger (1887–1961)
Schrödinger’s unconventional technique to atomic theory was typical of his unconventional method to life. The was well known for his intense dislike that memorizing data and also learning indigenous books. Once Hitler pertained to power in Germany, Schrödinger escaped come Italy. He then operated at Princeton college in the united States yet eventually relocated to the academy for progressed Studies in Dublin, Ireland, wherein he continued to be until his retirement in 1955.
Although quantum mechanics uses innovative mathematics, you perform not require to recognize the math details to follow our discussion of its basic conclusions. We focus on the nature of the wavefunctions that are the remedies of Schrödinger’s equations.
Wavefunctions
A wavefunction (Ψ) is a mathematical duty that relates the place of one electron in ~ a given point in space (identified by x, y, and also z coordinates) to the amplitude the its wave, which coincides to that energy. Hence each wavefunction is associated with a specific energy E. The properties of wavefunctions acquired from quantum mechanics room summarized here:
A wavefunction supplies three variables to describe the position of one electron. A 4th variable is usually required to fully describe the place of objects in motion. 3 specify the position in space (as v the Cartesian coordinates x, y, and also z), and one mentions the time in ~ which the thing is in ~ the specified location. Because that example, if you to be the captain that a ship trying to intercept an opponent submarine, friend would need to know its latitude, longitude, and depth, as well as the time in ~ which it to be going come be at this place (Figure (PageIndex1)). For electrons, we have the right to ignore the time dependence since we will certainly be using standing waves, which by an interpretation do not change with time, to define the place of one electron.

The major Quantum Number
The principal quantum number (n) speak the average relative street of one electron native the nucleus:
As n rises for a provided atom, therefore does the average distance of one electron native the nucleus. A negatively charged electron that is, top top average, closer come the positively charged nucleus is attractive to the nucleus more strongly 보다 an electron that is farther the end in space. This means that electron with greater values that n are less complicated to remove from one atom. All wavefunctions that have the exact same value that n are claimed to constitute a major shell since those electron have comparable average distances from the nucleus. As you will certainly see, the primary quantum number n synchronizes to the n provided by Bohr to explain electron orbits and by Rydberg to explain atomic power levels.
The Azimuthal Quantum Number
The second quantum number is often called the azimuthal quantum number (l). The value of l defines the shape of the region of room occupied by the electron. The allowed values that l count on the value of n and also can selection from 0 to n − 1:
For example, if n = 1, l can be just 0; if n = 2, l have the right to be 0 or 1; and so forth. For a given atom, every wavefunctions that have the same values that both n and l kind a subshell. The areas of room occupied by electrons in the exact same subshell usually have the same shape, yet they are oriented differently in space.
Example(PageIndex1): n=4 shell Structure
How many subshells and orbitals are had within the primary shell with n = 4?
Given: value that n
Asked for: number the subshells and also orbitals in the principal shell
Strategy:
given n = 4, calculate the enabled values that l. Indigenous these allowed values, counting the variety of subshells. For each allowed value that l, calculate the allowed values of ml. The sum of the number of orbitals in every subshell is the number of orbitals in the primary shell.See more: How Many Tablespoons Is 6 Oz, Convert 6 Ounces To Tablespoons
Solution:
A We recognize that l have the right to have every integral worths from 0 come n − 1. If n = 4, climate l deserve to equal 0, 1, 2, or 3. Because the covering has four values that l, that has 4 subshells, every of which will contain a different variety of orbitals, depending upon the enabled values of ml.
B for l = 0, ml deserve to be only 0, and also thus the l = 0 subshell has only one orbital. Because that l = 1, ml can be 0 or ±1; thus the l = 1 subshell has three orbitals. For l = 2, ml deserve to be 0, ±1, or ±2, so over there are 5 orbitals in the l = 2 subshell. The last enabled value of l is l = 3, for which ml deserve to be 0, ±1, ±2, or ±3, bring about seven orbitals in the l = 3 subshell. The total variety of orbitals in the n = 4 primary shell is the amount of the number of orbitals in each subshell and also is same to n2 = 16