84.443/543 Advanced Inorganic Chemistry - PowerPoint PPT Presentation

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84.443/543 Advanced Inorganic Chemistry

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Title: 84.443/543 Advanced Inorganic Chemistry


1
84.443/543Advanced Inorganic Chemistry
2
Course Web Site
  • http//faculty.uml.edu/ndeluca/84.334/
  • Important links to
  • course syllabus
  • tentative class schedule

3
The d orbitals
4
Unusual 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.

5
Unusual Aspects of Inorganic Compounds
  • Pi (p) bonds can be formed using the dxz and dyz
    orbitals.

6
Unusual 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.

7
Unusual 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.
8
Unusual 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.

9
Unusual 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.

10
Unusual 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.

11
Unusual Aspects of Inorganic Compounds
  • Cage compounds lack a direct metal-metal bond.
    Instead, the ligands serve to hold the complex
    together.

12
Unusual 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.

13
Quantum 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
14
Common 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.
15
Wave Functions of Orbitals
  • Wave functions can be factored into two angular
    components (based on ? and f), and a radial
    component (based on r).

16
Angular 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.

17
The d-orbitals
18
Radial 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.

19
Radial 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.

20
Radial Wavefunctions
  • The radial wave functions for hydrogenic orbitals
    have some key features

21
Radial 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.

22
Radial Wavefunctions
  • Key features
  • 3. As n increases, the functions oscillate
    through zero, resulting in radial nodes.

23
Radial 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.

24
Radial Nodes
  • For a given orbital,
  • the number of radial nodes n- l -1

25
p 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.

26
Radial Probability Functions
  • Radial probability functions (4pr2?2 or 4pr2R2 )
    are the product of the blue and green functions
    graphed for a 1s orbital.

27
Radial Probability Functions
  • The orange line represents the probability of
    finding an electron in a 1s orbital as a function
    of distance from the nucleus.

28
Radial 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.

29
Radial 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.

30
Radial 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.

31
Radial 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.

32
Radial 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.

33
The d orbitals
34
The f orbitals
35
The 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.

36
The 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).

37
Electron Configurations
38
Electron 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.

39
Electron 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.

40
Shielding
  • 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.

41
Shielding
  • 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.

42
Slaters 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.

43
Slaters 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

44
Slaters 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

45
Problem Zeff
  • Use Slaters rules to estimate the effective
    nuclear charge of Cl and Mg.

46
Periodic 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.

47
Ionization 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.

48
Ionization energy

49
Ionization energy

50
Ionization energy

51
Electron 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.

52
Electron 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.

53
Trends Electron Affinity
54
Trends- 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.

55
Electron 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.

56
Atomic 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.

57
Atomic Radii
58
Atomic Size
59
Atomic 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
60
Atomic 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.

61
Ionic 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.

62
Ionic Radii
  • Cations are always smaller than their neutral
    atom, since removal of an electron causes an
    increase in the effective nuclear charge.

63
Ionic Radii
  • Anions are always larger than their neutral
    atom, since additional electrons greatly decrease
    the effective nuclear charge.

64
Ionic Radii
  • For isoelectronic cations, the more positive
    the charge, the smaller the ion.
  • For isoelectronic anions, the lower the
    charge, the smaller the ion.

65
Ionic 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.
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