Matter, Measurements and Problem Solving

Download Report

Transcript Matter, Measurements and Problem Solving

Chapter 6
Electronic Structure of Atoms
SC 131 CHEM 1
Chemistry: The Central Science
CM Lamberty
Quantum Mechanics: A Theory

Smallness of atoms and subatomic particles




Traditional observations not possible



Size of e- <10-9 of 10-9 of a gram
Speck of dust contains as many e- as there have been
people on Earth since beginning
Dtm chemical and physical properties
e- do not move in regular patterns
e- observed behave differently than those not observed.
Quantum-mechanical model


Model to explain how e- exist in atoms and dtm
properties
Explain WHY some M, some NM, why noble gases are
inert, etc.
The Nature of Light

Wave Nature of Light


The Electromagnetic Spectrum


Radio (low E) to Gamma rays (high E)
Interference and Diffraction


Properties of waves
Ways waves may interact
The Particle Nature of Light
Photoelectric effect
 photons

The Wave Nature of Matter

Light is electromagnetic
radiation


Wave composed of
oscillating mutually
perpendicular electric and
magnetic fields
Speed of light (vacuum)
3.00x108 m/s

Amplitude


Vertical height of crest
Determines the
intensity of light
07_01-01UN.JPG
07_01.JPG
The Wave Nature of Matter

Wavelength


Distance between adjacent crests
Frequency
Number of cycles passing a point in given
period of time
 Cycles per second (s-1). 1 Hertz = 1 cycle/s
 Frequency directly proportional to speed,
inverse to wavelength

n= c
l
Wavelength and Amplitude
07_02.JPG
The Electromagnetic Spectrum




Includes ALL wavelengths of EM radiation
10-15m (gamma) - 105m (radio waves)
Short wavelength has greater E
Gamma (g) rays




Most energetic, shortest
Produced by sun and stars and unstable atomic nuclei
Damage to biological molecules
X-rays



Longer wavelength than gamma
Pass through many substances that block visible
Can damage biological molecules
The Electromagnetic Spectrum

Ultraviolet




Visible





Component of sunlight for suntan/sunburn
Carries enough E to damage biological mq
excessive exposure skin cancer, cataracts
Violet (short l, high E) - red (longer l, lower E)
Violet, blue, green, yellow, orange, red
Causes certain mq in eye to change shape resulting in
vision
Color we see is reflected, others absorbed
Infrared


Heat from hot object
Night vision goggles
The Electromagnetic Spectrum

Microwaves
Longer wavelengths
 Used for radar and microwave ovens
 Efficiently absorbed by water and can heat


Radio waves
Longest wavelength
 Transmit signals responsible for FM and AM
radio, cellular phones, TV, etc

Interference and Diffraction

Interference
How waves add together
 Constructive or destructive


Diffraction
How waves bend to move around/though
object
 Diffraction of light through 2 slits
 Interference pattern

Interference and Diffraction
07_06.JPG
07_07.JPG
The Particle Nature of Light


Light initially thought of as wave
Photoelectric effect





Metals emit e- when light shines on them
Series of tests did not follow EM theory
Einstein: packets of light E = hn
h is Planck’s constant
Photons




Our name for packets of light
Sometimes called quantum of light
E = hc
l
Light is “lumpy”
Light is shower of particles each having e of hn
Wave-particle duality of light
Atomic Spectroscopy & Bohr Model
Study of the EM radiation absorbed and
emitted by atoms
 Atom absorbs E (heat, light, electricity)
and remits the E as light

Each element emit light of characteristic color
 Each with several distinct wavelengths


Emission spectrum
Each element has its own emission spectrum
 Discrete lines not continuous

Atomic Spectroscopy & Bohr Model
07_10.JPG
Atomic Spectroscopy & Bohr Model

Johannes Rydberg
Simple equation to predict wavelength of H
 1/l = R(1/m2-1/n2)


Neils Bohr
His model: e- travel around nucleus in circular
orbits.
 These orbits can exist only as specific fixed
distances from nucleus
 E of each orbit was fixed or quantized
 Stationary states
 Only when e- made a transition that radiation
emitted or absorbed

The Wave Nature of Matter

Louis de Broglie
Wave nature of electrons
 Diffraction pattern
 de Broglie relation l = h/mn


Heisenberg

Uncertainty Principle: cannot simultaneously
observe both the wave nature and the particle
nature of the electron
Quantum Mechanics and the Atom

Schrodinger
Orbital, probability distribution map showing
where the electron is likely to be found
 Wave function


Quantum Numbers used to specify each
orbital or location of electron for an atom.
Quantum Mechanics and the Atom

Principle quantum number, n
Integer that dtm overall size and E of orbital
 n= 1,2,3…


Angular quantum number, l
Integer that dtm shape of orbital
 l = 0,1,2,…(n-1)


Magnetic quantum number, ml
Integer that dtm orientation of orbital
 ml = -l to +l (-l, …, -1, 0, 1,…, l)

Quantum Mechanics and the Atom
07_16-02UN.JPG
Atomic Spectroscopy Explained
07_17.JPG
07_18.JPG
The Shapes of Atomic Orbitals

Shape important b/c covalent chemical
bonds depend upon sharing of electrons
and occupy these orbitals
Shapes of the overlapping orbitals dtm shape
of molecule
 Shape dtm primarily by l the angular
momentum quantum number

l=0
 l=1
 l=2
 l=3

s orbital
p orbital
d orbital
f orbital
The Shapes of Atomic Orbitals

s orbitals
07_20.JPG
07_22.JPG
The Shapes of Atomic Orbitals

p orbitals
2 lobes
 Node at nucleus
 Orbitals are orthogonal to one another

The Shapes of Atomic Orbitals

d orbitals
5 3d orbitals
 4 are cloverleaf with 4 lobes
 5th is 2-lobed with donut (see p. 266)

Electron Configurations



Electron configuration
Ground state
Electron spin and Pauli Exclusion Principle





Direction of arrow represents electron spin
Direction does not affect value
Direction is quantized either up or down
Spin Quantum Number, ms
+1/2 (up) or -1/2 (down)
Electron Configurations

Pauli Exclusion Principle

No two electrons can have the same four quantum
numbers
Electron Configurations




Sublevel Energy Splitting in Multielectron Atoms
E(s) < E(p) < E(d) < E(f)
Sheilding
Effective nuclear charge
Electron Configuration of Sulfur