Understanding the Electronic Structure of Atoms and the Pauli Exclusion Principle, Schemes and Mind Maps of Physics

How the solutions of the Schrödinger equation for atoms can be characterized by four quantum numbers: n, β, m, and ms. It introduces the Pauli exclusion principle, which states that two identical fermions cannot occupy the same state, and discusses how it applies to the electronic structure of atoms, including the ground state of helium and lithium. The document also touches upon the filling of subshells in the periodic table and the combination of angular momenta.

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116
Chapter 7. Atomic Physics
Notes:
Most of the material in this chapter is taken from Thornton and Rex, Chapter 8.
7.1 The Pauli Exclusion Principle
We saw in the previous chapter that the hydrogen atom could be precisely understood by
considering the Schrödinger equation, including the electrostatic potential energy that
accounts for the interaction between the nucleus and the electron. We then discovered
that the family of stationary states, which are the solutions of the Schrödinger equation
can be completely characterized by three quantum numbers
n,, and m
. However, we
also found that the state of the electron is further characterized by its intrinsic spin, which
acts in a way akin to the angular momentum in that it provides an extra magnetic moment
and is quantized similarly. But comparisons between the
ˆ
S
and
ˆ
L
operators should
probably not be pushed too far, as for the electron the spin is half-integer with
s=1 2
independent of any other parameter, while
0n1
and always an integer. As a
result, the states of the hydrogen can only be fully specified by combining the previous
three quantum numbers for the solutions of the Schrödinger equation and the magnetic
spin quantum number
ms
, forming the
foursome. As we will now discover
there is another very important aspect of the spin that is absolutely essential for
understanding the structure of many-electron atoms.
Although it would be in principle possible to solve the Schrödinger equation for more
complicated atoms, the presence of several interaction terms between the different
electrons makes the problem analytically intractable and basically impossible to solve.
The exact determination of the stationary states, their energy, angular momentum, etc.
must then be accomplished using computers. It is, however, possible to qualitatively
understand the structure of many-electron atoms using the results obtain for the study of
the hydrogen atom and another fundamental principle that we owe to the Austrian
physicist Wolfgang Pauli (1900-1958).
The so-called Pauli exclusion principle, which stems from Pauli’s efforts to explain the
structure of the periodic table, can be stated as follows
Two identical fermions cannot occupy the same state.
Remember that fermions have half-integer spins; the electron with
s=1 2
is therefore
one. As Pauli initial enunciation of his principle in 1925 happened as he was studying the
atomic structure, it can then stated more specifically for atomic electrons with
No two electrons in an atom can share the same set of quantum numbers
n,,m,ms
( )
.
pf3
pf4
pf5
pf8

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Chapter 7. Atomic Physics

Notes:

  • Most of the material in this chapter is taken from Thornton and Rex, Chapter 8.

7.1 The Pauli Exclusion Principle

We saw in the previous chapter that the hydrogen atom could be precisely understood by

considering the Schrödinger equation, including the electrostatic potential energy that

accounts for the interaction between the nucleus and the electron. We then discovered

that the family of stationary states, which are the solutions of the Schrödinger equation

can be completely characterized by three quantum numbers (^) n , , and m. However, we

also found that the state of the electron is further characterized by its intrinsic spin, which

acts in a way akin to the angular momentum in that it provides an extra magnetic moment

and is quantized similarly. But comparisons between the

S and

L operators should

probably not be pushed too far, as for the electron the spin is half-integer with s = 1 2

independent of any other parameter, while 0 ≤  ≤ n − 1 and always an integer. As a

result, the states of the hydrogen can only be fully specified by combining the previous

three quantum numbers for the solutions of the Schrödinger equation and the magnetic

spin quantum number (^) m s

, forming the (^) n ,, m , m s

( ) foursome.^ As we will^ now^ discover

there is another very important aspect of the spin that is absolutely essential for

understanding the structure of many-electron atoms.

Although it would be in principle possible to solve the Schrödinger equation for more

complicated atoms, the presence of several interaction terms between the different

electrons makes the problem analytically intractable and basically impossible to solve.

The exact determination of the stationary states, their energy, angular momentum, etc.

must then be accomplished using computers. It is, however, possible to qualitatively

understand the structure of many-electron atoms using the results obtain for the study of

the hydrogen atom and another fundamental principle that we owe to the Austrian

physicist Wolfgang Pauli (1900-1958).

The so-called Pauli exclusion principle , which stems from Pauli’s efforts to explain the

structure of the periodic table, can be stated as follows

Two identical fermions cannot occupy the same state.

Remember that fermions have half-integer spins; the electron with s = 1 2 is therefore

one. As Pauli initial enunciation of his principle in 1925 happened as he was studying the

atomic structure, it can then stated more specifically for atomic electrons with

No two electrons in an atom can share the same set of quantum numbers n ,, m , m s

( ).

The structure of atoms and that of the periodic table can be explained with this principle

and the further assumption that atomic electrons tend to occupy the lowest available

energy states.

To see how this works, let us consider the next simplest atom after hydrogen, i.e., helium.

The helium atom (He) is composed of a nucleus made of two protons and two neutrons

for a total charge of + 2 e (a neutron has the same mass as a proton but no charge) and

two electrons. As was the case for the hydrogen atom we can expect that the lowest

energy state for an electron will consists of a 1s wave function with the electron spin

quantum number either 1 2 or − 1 2 , i.e., n ,, m , m s

( ) =^ (^1 ,^0 ,^0 ,^ ±^1 2 ).^ The second

electron is also likely to occupy a similar state, but because of the Pauli exclusion

principle, which forbids two electrons from occupying the exact same state, the quantum

numbers can only be n ,, m , m s

( ) =^ (^1 ,^0 ,^0 ,^ ^1 2 ) ;^ note^ the opposite sign^ of^ m s

for the two

electrons. We are thus left with the picture of the helium atom having its two electrons in

1s states, where one electron has its spin “up” and the other its spin “down.” The

complete ground state of the helium atom is then denoted by 1 s

2

, where the ending

superscript specifies the number of electrons in the given state (in this case, 1 s).

What would be the electronic structure for the next simplest atom, i.e., Lithium (Li),

which contains three electrons (and a nucleus made of three protons and four neutron)? It

should now be clear that the Pauli exclusion principle will forbid the lowest atomic state

to be something like 1 s

3

, since this would imply that two electrons would have to share

the same m s

number (i.e., the ending superscript cannot be greater than two for a n s

orbital). To minimize energy two electrons will still occupy the inner shell 1 s

2

, while the

third one will reside on the next unoccupied orbital with favourable energy. In this case

the next available lowest-energy electron state is 2s. The lithium atom ground state is

therefore 1 s

2

2 s

1

. One would be justified to ask why couldn’t the ground configuration be

1 s

2

2 p

1

instead? Indeed, this appears to be supported by the fact that our solution for the

hydrogen atom asserted that s and p orbitals for a given n^ number have the same energy

E

n

. The answer lies with the consideration of the precise shapes of the different orbitals.

An s orbital is said to be more penetrating than a p orbital. That is, the radial wave

function for  = 0 is more concentrated closer to the nucleus than that for  = 1. This

implies that an electron on a 2p orbital in the lithium atom is more likely to have the

nuclear charge of + 3 e screened by the two electrons on the 1s orbitals and “feel” an

effective charge of  + e. On the other hand, an electron on the more penetrating 2s

orbital is not as screened and will see more of the nuclear charge (i.e., the effective

charge is greater than + e ), which results in a lower potential energy due to its stronger

interaction with the nucleus. The 1 s

2

2 s

1

state is thus of lower energy than the 1 s

2

2 p

1

state and the correct choice for the ground state of lithium.

Just as the orbitals are designated by letters depending on the values of the  quantum

number, e.g., s, p, d, f, etc., shells are associated to the different values of the principal

quantum number n. More precisely, levels of n = 1 , 2 , 3 , 4 , … are given the capital

letters K, L, M, N, … The aforementioned n ^ orbitals are then called subshells. It

Exercises

  1. Use Table 8.1 to determine the ground state configuration of potassium (K, consisting

of 19 protons and 20 neutrons).

Solution.

Potassium has 19 electrons, which we must place in subshells of increasing energy. The

K and L shells are successively filled without interruption and will use up

( 2 ) + ( 2 + 6 ) = 10 electrons (for the 1 s

2

  • 2 s

2

  • 2 p

6

( ) subshells).^ Likewise,^ the next 8

electrons will occupy the 3 s

2

and 3p

6

subshells, but Table 8.1 tells us that final lone

electron does not go to a 3d but a 4s orbital. The ground state configuration for potassium

is therefore 1 s

2

2 s

2

2 p

6

3 s

2

3 p

6

4 s

1

.

7.2 The Periodic Table

With the understanding of the electronic structure of atoms we acquired it is now

relatively easy to understand the structure of the periodic table, which was first

introduced by the Russian chemist Dmitri Ivanovich Mendeleev (1834-1907) in 186 9

(well before the advent of quantum mechanics). Figure 1 shows the table, with the

electronic configuration specified for every element.

The periodic table is organized in groups , along the different columns, for elements

sharing the same chemical properties. A careful look of any given column will show that

the corresponding elements all have the same or similar subshell status. That is, they all

have the same number of electrons occupying a given ^ subshell, irrespective of the n

number. The rows are known as periods and correspond to the filling of subshells. As one

goes from the first element on the left to the last on the right of a period, one or more than

one subshell can be successively filled. Periods are characterized by the number of shells

(or energy levels) of electrons surrounding the nucleus. Here is a brief description of

some important groups.

Group 1 - Alkalis

This group, to which hydrogen belongs, are characterized by having one s electron in the

outer subshell. Since s electrons tend to extend relatively far from the nucleus and,

furthermore, can easily be stripped off the atom (thus forming a positive ion of charge

  • 1 e ) these elements are highly reactive. Because of this tendency to give or share an

electron it is said that alkalis have a valence of + 1. This also results in them being good

electrical conductors. All elements in this group, except hydrogen, are refereed to as

alkali metals.

Group 2 - Alkaline Earths

Alkaline earths elements have their outer s subshell filled. Although we might assume

that they would then be more stable than alkalis, the fact that s orbitals are extended and

their electrons easily removed render them quite chemically reactive. They have a

valence of + 2 and are good electrical conductors.

Groups 3 to 12 – Transition Metals (or Transition Elements)

The three rows where the 3d, 4d, and 5d subshells are being filled (i.e., elements 21-30,

39 - 48, and 72-80) form the transition metals group. Several of these atoms (e.g., iron

(Fe), cobalt (Co), and nickel (Ni)) have strong magnetic moments due to the presence of

unpaired electrons in the d subshell. These electrons will see their spins aligned therefore

producing the ferromagnetic properties of the elements.

The rare earths elements consisting of the lanthanides (elements 58-71) and actinides

(elements 90-103) can also be included in this group. This is because these elements have

unpaired electrons in the f subshells (for n^ =^4 and n^ =^5 , respectively) leading also to

large magnetic moments.

Group 17 - Halogens

All elements of this group have five electrons in their outer p subshell, and therefore have

a valence of − 1. This characteristic renders them very chemically reactive; Fluorine (F)

is the most reactive element in existence. Halogens will especially bond efficiently with

alkalis, which have a valence of + 1 , to form compound such as NaCl.

Atoms in groups 13 to 16 are composed of metals (e.g., aluminum (Al), tin (Sn), and

bismuth (Bi)), non-metals (carbon (C), nitrogen (N), and oxygen (O)), and metalloids

(often semiconductors) exhibiting some properties of metals and non-metals (e.g., boron

(B), silicon (Si), Arsenic (As), and tellurium (Te)).

7.3 The Combination of Angular Momenta

We saw that transitions metals have high magnetic moments because of the effect of

unpaired electron’s spin. To understand how this comes about we must first understand

how angular momenta, orbital and intrinsic spin, combine or add up to form the total

angular momentum

J. We will consider the simple case for the combination of the spin

S and orbital angular momentum

L of a single electron. We first note that the two

momenta add vectorially

J =

L +

S. (^7.^1 )

We remember that both the orbital and spin angular momenta are quantized such that

L =  (  + 1 ), L

z

= m

S = s ( s + 1 ), S

z

= m s

and m j

j. From equations ( 7. 2 ) and ( 7. 3 ) we can write

J

z

= m

  • m s

( ), ( 7. 4 )

or m j

= m

  • m s

. It is important to realize that different values for m

, m s

, or m j

imply a

different orientation for the corresponding vectors. We therefore expect that there will be

several possibilities for both the orientation of the total angular momentum

J as well as

its magnitude J.

To get a better sense of this let us consider the case where  = 1 , m

= − 1 , 0 , and 1 , and

s = 1 2 , m s

= − 1 2 and 1 2. Considering equation ( 7. 4 ) tells us that the following values

for m j

are realized

m j

m

= 1

m s

1

2

m

= 0

m s

1

2

m

=− 1

m s

1

2

These values for the magnetic total quantum number can be grouped as follows to find

the realized values for j according to equation ( 7. 3 )

j =

, m j

j =

, m j

This result can be generalized to any pair of angular momenta of any kind (i.e., any

mixture of orbital, spin, or “intermediate” total angular momenta) with

J =

J

1

J

2

j 1

j 2

jj 1

  • j 2

m j

j ,

where successive values for J differ by 1. It can easily be verified that equations ( 7. 6 )

are verified when

J

1

L

1

and

J

2

S

1

Let us now come back to the case of a transition metal atom and see if we can better

understand its high magnetic moment relative to elements of other groups. For example,

we consider the case of titanium (Ti), which has the [ Ar] 3 d

2

4 s

2

electronic configuration

( [ Ar] means that the inner core of titanium corresponds to the filled electronic

configuration of argon, which is (^1) s

2

2 s

2

2 p

6

3 s

2

3 p

6

). The d subshell of titanium is thus

incomplete with only two electrons. For reasons that we will not discuss here, the ground

state for such an atom with two unpaired electron on an outer subshell is realized when i)

the spin is maximized, ii) the orbital angular momentum is also maximized, and iii) the

total angular momentum is minimized, while always keeping in mind that the Pauli

exclusion principle must be verified. The total spin is then

S =

S

1

S

2

, which implies that

s = 0 or 1. Because of the first rule above we choose s = 1. Likewise, the total orbital

angular momentum is

L =

L

1

L

2

with  1

2

= 2 and therefore  = 0 , 1 , 2 , 3 , and 4.

We may be tempted to choose  = 4 in order to maximize the orbital momentum, but this

would go against the Pauli exclusion principle since it implies that m  1

= m  2

(remember that  1

2

and s 1

= s 2

). We must therefore settle for  = 3 , which in turn

implies that the total angular momentum

J =

L +

S can span the values j = 2 , 3 , and 4.

Evidently,

J is minimized for j = 2 , which is a state possessing a significant magnetic

moment for m j

Finally, the state (or configuration) of an atom is expressed with the following notation

2 s + 1

L j

where 2 s + 1 is called the multiplicity of the state, and L is a capital letter used for the

orbital corresponding to . For example, the ground state of titanium we determined

earlier is defined with

3

F 2

Exercise

  1. Determined the notation for the ground state of carbon given that its configuration is

1 s

2

2 s

2

2 p

2

.

Solution.

We have two unpaired p electrons for which we maximize the spin with s = 1. The

possible values for the total orbital angular momentum are  = 0 , 1 , and 2 , with the

maximum allowed by the Pauli exclusion principle of  = 1. It follows that

j = 0 , 1 , and 2 , for a minimum of j = 0 and a ground state denoted by

3

P 0