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Transcript
Tentative material to be covered for Exam 2
(Wednesday, October 27)
Chapter 16
Quantum Mechanics and the Hydrogen Atom
16.1
16.2
16.3
16.4
16.5
Waves and Light
Paradoxes in Classical Physics
Planck, Einstein, and Bohr
Waves, Particles, and the Schroedinger Equation
The Hydrogen Atom
Chapter 17
Many-Electron Atoms and Chemical Bonding
17.1
17.2
17.3
17.4
17.5
17.6
Many-Electron Atoms and the Periodic Table
Experimental Measures of Orbital Energies
Sizes of Atoms and Ions
Properties of the Chemical Bond
Ionic and Covalent Bonds
Oxidation States and Chemical Bonding
Chapter 18
Molecular Orbitals, Spectroscopy, and Chemical Bonding
18.1
18.2
18.3
18.4
18.5
Diatomic Molecules
Polyatomic Molecules
The Conjugation of Bonds and Resonance Structures
The Interaction of Light with Molecules
Atmospheric Chemistry and Air Pollution
Chapter 16
Quantum Mechanics and the Hydrogen Atom
16.1
Waves and Light
Atomic Spectra I
16.2
Paradoxes in Classical Physics
Ultraviolet Catastrophe
Photoelectric effect
16.3
Planck, Einstein, and Bohr
Planck’s Constant, Quanta and Photons
Bohr Atom
Atomic Spectra II
16.4
Waves, Particles, and the Schroedinger Equation
Schroedinger Equation (Wave Equation)
16.5
The Hydrogen Atom
Sizes and Shapes of Orbitals
Electron Spin
Review of the development of the Bohr
atom
A Movie from the Mechanical Universe
Schroedinger: If electrons are
waves, their postion and motion
in space must obey a wave
equation.
Solutions of wave equations yield
wavefunctions, Y, 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.
Particles are out, waves are in. But the mathematics of waves is very
complex!
Wavefunctions and orbitals
Obital: defined by the quantum numbers n, l and ml
Orbital is a wavefunction
Orbital is a region of space occupied by an electron
Orbitals has energies, shapes and orientation in space
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
orbitals
Rule: l = 0, s orbital; l
= 1, p orbital; l = 2, d
orbital
l = 3, f orbital
1s, 2s, 2p, 3s, 3p, 4s, 4p,
4d, etc.
Recall the gaps between the energy levels of the H atom. Big initial
gap and then smaller and smaller gaps.
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 n
subshell = 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 subshell
n= 2, two subshells, etc
Each subshell of QN = l,
contains 2l + 1 orbitals
l = 0, 2(0) + 1 = 1
l = 1, 2(1) + 1 = 3
Sizes, Shapes, and orientations of orbitals
n determines size; l determines shape
ml determines orientation
Nodes in orbitals: s orbitals: 1s no nodes, 2s one node, 3s
two nodes
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!
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
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)
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
Chapter 17
17.1
17.2
17.3
17.4
17.5
17.6
Many-Electron Atoms and
Chemical Bonding
Many-Electron Atoms and the
Periodic Table
Experimental Measures of Orbital
Energies
Sizes of Atoms and Ions
Properties of the Chemical Bond
Ionic and Covalent Bonds
Oxidation States and Chemical
Bonding
Chapter 17 The Many Electron Atom
Goal: 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
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)
Ground state electron configuration of a many
electron atom: Governs reactivity under normal
condition
Imagine a bare nucleus of charge +Z
Imagine empty orbitals surrounding the nucleus
Fill the orbital with Z electrons for the neutral atom
Two Principles:
Aufbau principle: fill lowest energy orbital first
Pauli exclusion principle: each electron must have four
different quantum numbers (maximum of 2 electrons in
an orbital).
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 n
subshell = all orbitals with the same value of n and l
an orbital is fully defined by three quantum numbers, n, l, and ml
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 = 3
This means that factors ignored
may have to be considered
Constructing the periodic table by filling orbitals with
electrons.
Construction of the first row of the periodic table.
Electron configurations.
Aufbau: Fill 1s orbital first
Pauli: no more than two
electrons in the 1s orbital
The basis of the octet rule:
filling a shell
1s subshell filled with 2He =
stable electron core given
symbol [He].
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.
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 electronelectron repulsion and
lowers the atom’s energy
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]
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
Summary
From 1H to
10Ne.
No new
features
from 11Na to
18Ar.
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?
The electron affinity (EA) of an atom is the energy change which
occurs when an atom gains an electron.
X(g) + eXe- (g)
Electron affinities of the representative elements:
What are the correlations across and down?
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
Electronegativity (EN): a measure of the
ability of an atom to attract electrons to
itself in competition with other atoms
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
Bond lengths