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Tentative material to be covered for Exam 2 (Wednesday, October 27) Chapter 16 Quantum Mechanics and the Hydrogen Atom 16.1 Waves and Light 16.2 Paradoxes in Classical Physics 16.3 Planck, Einstein, and Bohr 16.4 Waves, Particles, and the Schroedinger Equation 16.5 The Hydrogen Atom Chapter 17 Many-Electron Atoms and Chemical Bonding 17.1 Many-Electron Atoms and the Periodic Table 17.2 Experimental Measures of Orbital Energies 17.3 Sizes of Atoms and Ions 17.4 Properties of the Chemical Bond 17.5 Ionic and Covalent Bonds 17.6 Oxidation States and Chemical Bonding Chapter 18 Molecular Orbitals, Spectroscopy, and Chemical Bonding 18.1 Diatomic Molecules 18.2 Polyatomic Molecules 18.3 The Conjugation of Bonds and Resonance Structures 18.4 The Interaction of Light with Molecules 18.5 Atmospheric Chemistry and Air Pollution

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Page 1: PowerPoint Presentation€¦ · PPT file · Web view · 2005-03-08Chapter 17 Many-Electron Atoms and ... Times Comic Sans MS Symbol Blank Presentation PowerPoint Presentation PowerPoint

Tentative material to be covered for Exam 2 (Wednesday, October 27)

Chapter 16 Quantum Mechanics and the Hydrogen Atom

16.1 Waves and Light16.2 Paradoxes in Classical Physics16.3 Planck, Einstein, and Bohr16.4 Waves, Particles, and the Schroedinger Equation16.5 The Hydrogen Atom

Chapter 17 Many-Electron Atoms and Chemical Bonding

17.1 Many-Electron Atoms and the Periodic Table17.2 Experimental Measures of Orbital Energies17.3 Sizes of Atoms and Ions17.4 Properties of the Chemical Bond17.5 Ionic and Covalent Bonds17.6 Oxidation States and Chemical Bonding

Chapter 18 Molecular Orbitals, Spectroscopy, and Chemical Bonding

18.1 Diatomic Molecules18.2 Polyatomic Molecules18.3 The Conjugation of Bonds and Resonance Structures18.4 The Interaction of Light with Molecules18.5 Atmospheric Chemistry and Air Pollution

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Chapter 16 Quantum Mechanics and the Hydrogen Atom

16.1 Waves and LightAtomic Spectra I

16.2 Paradoxes in Classical PhysicsUltraviolet Catastrophe Photoelectric effect

16.3 Planck, Einstein, and BohrPlanck’s Constant, Quanta and PhotonsBohr AtomAtomic Spectra II

16.4 Waves, Particles, and the Schroedinger EquationSchroedinger Equation (Wave Equation)

16.5 The Hydrogen AtomSizes and Shapes of OrbitalsElectron Spin

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Review of the development of the Bohr atom

A Movie from the Mechanical Universe

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Schroedinger: If electrons are waves, their postion and motion in space must obey a wave equation.

Solutions of wave equations yield wavefunctions, , which contain the information required to describe ALL of the properties of the wave.

Provides a picture of the electronic distributions of the electrons about an the nucleus of an atom and about the connected nuclei of a molecule.

Schroedinger thinking about his equation.

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Particles are out, waves are in. But the mathematics of waves is very complex!

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Wavefunctions and orbitalsObital: defined by the quantum numbers n, l and ml Orbital is a wavefunctionOrbital is a region of space occupied by an electronOrbitals has energies, shapes and orientation in space

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Quantum Numbers (QN)

Principal QN:

n = 1, 2, 3, 4……

Angular momentum QN:

l = 0, 1, 2, 3…. (n -1)

Rule: l = (n - 1)

Magnetic QN:

ml = …-2, -1, 0, 1, 2, ..

Rule: -l….0….+l

Shorthand notation for orbitalsRule: l = 0, s orbital; l = 1, p orbital; l = 2, d orbital

l = 3, f orbital1s, 2s, 2p, 3s, 3p, 4s, 4p, 4d, etc.

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Recall the gaps between the energy levels of the H atom. Big initial gap and then smaller and smaller gaps.

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The energy of an orbital of a hydrogen atom or any one electron atom only depends on the value of n

shell = all orbitals with the same value of nsubshell = all orbitals with the same value of n and l

an orbital is fully defined by three quantum numbers, n, l, and ml

Each shell of QN = n contains n subshells

n = 1, one subshelln= 2, two subshells, etc

Each subshell of QN = l, contains 2l + 1 orbitals

l = 0, 2(0) + 1 = 1l = 1, 2(1) + 1 = 3

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Sizes, Shapes, and orientations of orbitals

n determines size; l determines shapeml determines orientation

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Nodes in orbitals: s orbitals: 1s no nodes, 2s one node, 3s two nodes

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Nodes in orbitals: 2p orbitals:

angular node that passes through the nucleus

Orbital is “dumb bell” shaped

Important: the + and - that is shown for a p orbital refers to the mathematical sign of the wavefunction,

not electric charge!

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Nodes in orbitals: 3d orbitals:

two angular nodes that passes through the

nucleus

Orbital is “four leaf clover” shaped

d orbitals are important for metals

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The fourth quantum number: Electron Spin

ms = +1/2 (spin up) or -1/2 (spin down)

Spin is a fundamental property of electrons, like its charge and mass.

(spin up)

(spin down)

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Electrons in an orbital must have different values of ms

This statement demands that if there are two electrons in an orbital one must have ms = +1/2

(spin up) and the other must have ms = -1/2 (spin down)

This is the Pauli Exclusion Principle

An empty orbital is fully described by the three quantum numbers: n, l and ml

An electron in an orbital is fully described by the four quantum numbers: n, l, ml

and ms

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Chapter 17 Many-Electron Atoms and Chemical Bonding

17.1 Many-Electron Atoms and the Periodic Table

17.2 Experimental Measures of Orbital Energies17.3 Sizes of Atoms and Ions17.4 Properties of the Chemical Bond17.5 Ionic and Covalent Bonds17.6 Oxidation States and Chemical

Bonding

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Chapter 17 The Many Electron AtomGoal: Construct the periodic table based

on quantum numbers

(1) Solve the wave equation exactly for the H atom

(2) Use the exact orbitals for the H atom as a starting approximation for the many electron atom

(3) Quantum numbers obtained for H atom used to describe the many electron atom

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The orbital approximation for a many electron atom:

The electrons are described by the same four quantum numbers as the H atom, but the energies of the orbits depend on both n and l (but not on ml)

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Ground state electron configuration of a many electron atom: Governs reactivity under normal condition

Imagine a bare nucleus of charge +ZImagine empty orbitals surrounding the nucleus

Fill the orbital with Z electrons for the neutral atom

Two Principles:Aufbau principle: fill lowest energy orbital firstPauli exclusion principle: each electron must have

four different quantum numbers (maximum of 2 electrons in an orbital).

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The energy of an orbital of a hydrogen atom or any one electron atom only depends on the value of n

shell = all orbitals with the same value of nsubshell = all orbitals with the same value of n and l

an orbital is fully defined by three quantum numbers, n, l, and ml

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Relative orbital energies for the multielectron atom.

The energy of an orbital of a multielectron atom depends on n and l (but not ml)

2s < 2p

3s < 3p <3d

Note energy levels are getting closer together for n = 3This means that factors ignored may have to be considered

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Constructing the periodic table by filling orbitals with electrons.

Construction of the first row of the periodic table.Electron configurations.

Aufbau: Fill 1s orbital firstPauli: no more than two

electrons in the 1s orbitalThe basis of the octet rule:

filling a shell1s subshell filled with 2He

= stable electron core given symbol [He].

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Filling the orbitals of 3Li, 4Be and 5B

Aufbau: Fill 1s orbital first, then 2s, then 2p

Pauli: no more than two electrons in the 1s orbital.

2s subshell filled with 4Be.

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Filling the orbitals of 6C and 7N. The need for a third rule (Hund’s rule):

When electrons occupy orbitals of the same energy, the lowest energy state corresponds to the configuration with the greatest number of orbitally and spin unpaired electrons. This avoids electron-electron repulsion and lowers the atom’s energy

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Filling the orbitals of 8O, 9F and 10Ne

Filling the 2p subshell produces another stable configuration of electrons which serves as the core shell of the third row: symbol [Ne]

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Orbital shells and the building up of the periodic

table

A shell is a set of orbitals with the same value of n

and l for a H atom.

The Ar atom has shells as shown in the profile of electron density as a

function of distance from the nucleus

These are the valence electrons of the Lewis

structures

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SummaryFrom 1H to 10Ne.

No new features from 11Na to 18Ar.

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The ionization energy (IE) of an atom is the minimun energy required to remove an electron from an atom.

X(g) X+(g) + e-

Periodic trends ionization energies of the representative elements: What are the correlations

across and down?

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The electron affinity (EA) of an atom is the energy change which occurs when an atom gains an electron.

X(g) + e- Xe- (g) Electron affinities of the representative elements:

What are the correlations across and down?

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Periodic properties of atomic radius:What are the correlations?

General Rule: The size of an atom decreases in a row as the nuclear charge increases and the size of an atom increases in a column as the nuclear charge increases

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Electronegativity (EN): a measure of the ability of an atom to attract electrons

to itself in competition with other atoms

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Practice Exam for Chapter 16 will go up tonight or tomorrow

Slide show for Exam 2 is up in Persuasion

Working on getting back your answer sheets for Exam 1

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Bond lengths

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