2.5.3.2. Electron Shells

As a simple model, an atom may be considered to be a positively charged nucleus surrounded by shells of negatively charged electrons. The shells are termed K, L, M, and N (starting from the innermost, most strongly bound shell). More accurately, an atom consists of a nucleus surrounded by electrons that occupy volumes of space (orbitals) around it (Figure 2.5.3.2) only some of which are spherical.

Figure 2.5.3.2. Actual probability distributions for electron clouds, which are considered as shells in this discussion. Electron Shells

Each electron has several quantum numbers that uniquely define it and specify the shell it may occupy. The quantum numbers are:

 

Number

Name

Permitted Values

Defines

Notes

n

principal quantum number

positive integers (1,2,3...)

electron shell

(1=K, 2=L, 3= M...)

Principle binding energy.

l

azimuthal quantum number

integers from 0 to (n-1)

electron cloud shape (0=sphere, 1=dumbbell...)

Orbital angular momentum. Chemists follow the conventions of optical spectroscopy using letters rather than numbers to indicate the value of l: sharp (l = 0), principal, (l = 1), diffuse (l = 2), and fundamental (l = 3).

m

magnetic quantum number

-l to +l (including 0)

electron shell orientation when in a magnetic field

In the absence of an external magnetic field, the magnetic number has no meaning and will be ignored in the subsequent discussion.

s

spin quantum number

± ½

electron spin direction

Clockwise or counterclockwise.

j

inner precession

l ± ½, except j ¹ 0 - ½

total angular momentum

As noted under permitted values, for s orbitals (with l = 0), j can only be +½ (a vector sum is always positive). The value of j is important for determining what transitions are possible between electron shells.

The Pauli exclusion principle states that no two electrons can have the same quantum numbers. This constraint specifies the maximum number of electrons per level as 2n². Shells specified by the quantum numbers are labeled as shown on the following table.

 

K

LI

LII

LIII

MI

MII

MIII

MIV

MV

NI

NII

NIII

NIV

NV

NVI

NVII

n

1

2

2

2

3

3

3

3

3

4

4

4

4

4

4

4

l

0

0

1

1

0

1

1

2

2

0

1

1

2

2

3

3

s

j

½

½

½

½

½

½

½

etc.

 


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Copyright 1997-2003, James H. Wittke

Last update: 01/18/2006 01:47 PM.