Title: 84.443/543 Advanced Inorganic Chemistry
184.443/543Advanced Inorganic Chemistry
2Course Web Site
- http//faculty.uml.edu/ndeluca/84.334/
- Important links to
- course syllabus
- tentative class schedule
3The d orbitals
4Unusual Aspects of Inorganic Compounds
- The use of d orbitals enables transition metals
to form quadruple bonds. Sigma (s) bonds can be
formed using p orbitals, or the dz2 orbitals.
5Unusual Aspects of Inorganic Compounds
- Pi (p) bonds can be formed using the dxz and dyz
orbitals.
6Unusual Aspects of Inorganic Compounds
- In addition, face-to-face overlap is possible
between the dxy orbitals on each metal. This
forms a delta (d) bond.
7Unusual Aspects of Inorganic Compounds
- The existence of d bonds is usually determined by
measuring bond lengths and magnetic moments.
Re2Cl82- has a quadruple bond between the metal
atoms.
8Unusual Aspects of Inorganic Compounds
- The coordination number for transition metals can
be greater than 4, with coordination numbers of 6
being quite common. In addition, 4-coordinate
metal complexes need not be tetrahedral.
9Unusual Aspects of Inorganic Compounds
- When inorganic compounds have tetrahedral
geometry, it may be quite different from organic
compounds. P4 has tetrahedral geometry, but
lacks a central atom.
10Unusual Aspects of Inorganic Compounds
- Cluster compounds, in which there are metal-metal
bonds can be formed. The structure of Mn2(CO)10
has the two Mn atoms directly bonded to each
other.
11Unusual Aspects of Inorganic Compounds
- Cage compounds lack a direct metal-metal bond.
Instead, the ligands serve to hold the complex
together.
12Unusual Aspects of Inorganic Compounds
- Organic molecules may bond to transition metals
with s bonds or p bonds. If p bonded, some
unusual sandwich compounds may result.
13Quantum Numbers
n principal quantum n 1, 2, 3, etc. Determines the major part of the energy of the electron
l angular momentum quantum 0,1,2n-1 Describes angular dependence and contributes to the energy
ml magnetic quantum -l0l Describes the orientation in space. (ex. px, py or pz)
ms Spin quantum 1/2 or -1/2 Describes orientation of the electrons magnetic moment in space
14Common Orbital Designations
s p d f
l 0 1 2 3
In the absence of a magnetic field, the p
orbitals (or d orbitals) are degenerate, and have
identical energy.
15Wave Functions of Orbitals
- Wave functions can be factored into two angular
components (based on ? and f), and a radial
component (based on r).
16Angular Functions
- The angular functions, based on l and ml ,
provide the probability of finding an electron at
various points from the nucleus. These functions
provide the shape of the orbitals and their
spatial orientation.
17The d-orbitals
18Radial Functions
- Radial functions are determined by the quantum
numbers n and l, and are used to determine the
radial wave probability function (4pr2R2). - R is the radial function, and it describes the
electron density at different distances from the
nucleus. r is the distance from the nucleus.
19Radial Functions
- Radial functions are used to determine the
probablity of finding an electron in a specific
subshell at a specified distance from the
nucleus, summed over all angles.
20Radial Wavefunctions
- The radial wave functions for hydrogenic orbitals
have some key features
21Radial Wavefunctions
- Key features
- 1. All s orbitals have a finite amplitude at the
nucleus. - 2. All orbitals decay exponentially at
sufficiently great distances from the nucleus.
22Radial Wavefunctions
- Key features
- 3. As n increases, the functions oscillate
through zero, resulting in radial nodes.
23Radial Nodes
- Radial nodes represent the point at which the
wave function goes from a positive value to a
negative value. They are significant, since the
probability functions depend upon ?2, and the
nodes result in regions of zero probability of
finding an electron.
24Radial Nodes
- For a given orbital,
- the number of radial nodes n- l -1
25p orbitals
- The radial wave functions of p orbitals show a
zero amplitude at the nucleus. - The result is that
- p orbitals are less penetrating than s orbitals.
26Radial Probability Functions
- Radial probability functions (4pr2?2 or 4pr2R2 )
are the product of the blue and green functions
graphed for a 1s orbital.
27Radial Probability Functions
- The orange line represents the probability of
finding an electron in a 1s orbital as a function
of distance from the nucleus.
28Radial Probability Functions
- Note the zero probability at the nucleus (since
r0). The most probable distance from the
nucleus is the Bohr radius, ao 52.9 pm.
29Radial Probability Functions
- The probability falls off rapidly as the
distance from the nucleus increases. - For a 1s orbital, the probability is near zero
at a value of r 5ao.
30Radial Probability Functions
- In a 1 electron atom, the 2s and 2p orbitals
are degenerate. In multi-electron atoms, the 2s
orbital is lower in energy than the 2p orbital.
31Radial Probability Functions
- On average, the electrons in the 2s orbital
will be farther from the nucleus than those in
the 2p orbital. Yet, electrons in the 2s orbital
have a higher probability of being near the
nucleus due to the inner maximum. -
32Radial Probability Functions
- The net result is that the energy of electrons
in the 2s orbital are lower than that of
electrons in the 2p orbitals. -
33The d orbitals
34The f orbitals
35The Aufbau Principle
- The loss of degeneracy in multi-electron atoms
or ions results in electron configurations that
cannot be predicted based solely on the values of
quantum numbers. - The aufbau (building up) principle provides
rules for obtaining electron configurations.
36The Aufbau Principle
- 1. The lowest values of n and l are filled first
to minimize energy. - 2. The Pauli Exclusion Principle requires that
each electron in an atom must have a unique set
of quantum numbers. - 3. Hunds Rule requires that electrons in
degenerate orbitals will have the maximum
multiplicity (or highest total spin).
37Electron Configurations
38Electron Configurations
- Klechkowskys Rule states that filling proceeds
from the lowest available value of n l. - When two combinations have the same sum of n
l, the orbital with a lower value of n is filled
first.
39Electron Configurations
- The electron configurations of Cr and Cu in the
first row of the transition metals defy all
rules, as do many of the lower transition
elements.
40Shielding
- The energy of an orbital is related to its
ability to penetrate the area near the nucleus,
and its ability to shield other electrons from
the nucleus. - The positive charge affecting a specific
electron is called the effective nuclear charge,
or Zeff.
41Shielding
- Zeff Zactual S
- or
- Zeff Zactual s
- Where S or s is the shielding factor.
- Both the value of n and l (orbital type) play a
significant role in determining the shielding
factor.
42Slaters Rules
- 1. The electronic structure of atoms is written
in groupings - (1s)(2s, 2p)(3s, 3p)(3d)(4s, 4p)(4d)(4f )
- 2. Electrons in higher groupings do not shield
those in lower groups.
43Slaters Rules- Calculation of S
- 3. For ns or np electrons
- a) electrons in the same ns and np as the
electron being considered contribute .35,
except for 1s, where .30 works better. - b) electrons in the n-1 group contribute .85
- c) electrons in the n-2 group or lower (core
electrons) contribute 1.00
44Slaters Rules- Calculation of S
- 4. For nd or nf electrons
- a) electrons in the same nd or nf levelas the
electron being considered contribute .35 - b) electrons in the groups to the left
contribute 1.00
45Problem Zeff
- Use Slaters rules to estimate the effective
nuclear charge of Cl and Mg.
46Periodic Trends
- Zeff increases across a period. This is due to
the addition of protons in the nucleus,
accompanied by ineffective shielding for the
added electrons. As a result, the valence
electrons experience a greater nuclear charge on
the right side of the periodic table. -
47Ionization energy
- Ionization energy is the energy required to
remove an electron from a mole of gaseous atoms
or ions. - An(g) energy ? A(n1)(g) e-
- Ionization energy increases going across a
period, and sometimes decreases slightly going
down a group.
48Ionization energy
49Ionization energy
50Ionization energy
51Electron Affinity
- Electron affinity has several definitions.
Originally, it was defined as the energy released
when an electron is added to a mole of gaseous
atoms or ions. - A(g) e- ? A-(g) energy
- Under this definition, the elements in the
upper right part of the periodic table (O, F)
have relatively high (and positive) electron
affinities.
52Electron Affinity
- Your text still uses this basic definition, but
defines electron affinity as the energy change
for the reverse process. - A-(g) ? A(g) e- EA ?U
- The values of electron affinity are the same,
with positive values for elements that readily
accept an additional electron.
53Trends Electron Affinity
54Trends- Electron Affinity
- The electron affinity of fluorine is less
negative than expected. This may be due to
additional electron-electron repulsion when an
electron is added to such a small atom.
55Electron Affinity
- There are no real trends in electron affinity.
The affinities of group IA metals are slightly
positive, near zero for group IIA, and then
increase in groups IIIA and IVA. They drop (but
remain positive) for group VA, and then increase
through group VIIA. The values are negative for
the noble gases.
56Atomic Radii
- The determination of atomic radii is difficult.
The method used depends upon the nature of the
elemental structure (metallic, diatomic, etc.).
As a result, comparisons across the table are not
straightforward. - In general, size decreases across a period due
to the increase in effective nuclear charge, and
increases going down a group due to increasing
values of n.
57Atomic Radii
58Atomic Size
59Atomic Radii
- A close examination of the radii of elements in
periods 5 and 6 shows values which defy the
trends.
Group 4 (4B) Group 5 (5B) Group 11 (1B)
Zr 145 pm Nb 134 pm Ag 134 pm
Hf 144 pm Ta 135 pm Au 134 pm
60Atomic Radii
- There is a large decrease in atomic size
between La (169pm) and Hf (144 pm). This is due
to the filling of the f orbitals of the
Lanthanide series. As a result, the elements Hf
and beyond appear to be unusually small. - The decrease in size is called the lanthanide
contraction, and is simply due to the way
elements are listed on the table.
61Ionic Radii
- Determining the size of ions is problematic.
Although crystal structures can be determined by
X-ray diffraction, we cannot determine where one
ion ends and another begins. -
62Ionic Radii
- Cations are always smaller than their neutral
atom, since removal of an electron causes an
increase in the effective nuclear charge. -
63Ionic Radii
- Anions are always larger than their neutral
atom, since additional electrons greatly decrease
the effective nuclear charge. -
64Ionic Radii
- For isoelectronic cations, the more positive
the charge, the smaller the ion. - For isoelectronic anions, the lower the
charge, the smaller the ion.
65Ionic Radii
Determining ionic radii is extremely difficult.
Ionic size varies with ionic charge,
coordination number and crystal structure. Past
approaches involved assigning a reasonable
radius to the oxide ion. Calculations based on
X-ray data and electron density maps provide
results where cations are 14pm larger and anions
14pm smaller than previously found.