Title: Electrons
1Electrons the early years
2Electromagnetic Radiation
- Radiant energy that travels through space at the
speed of light in a vacuum.
3Wave particle duality
4 Light as a wave
- Waves have 3 primary characteristics
- 1. Wavelength distance between two peaks in a
wave. - 2. Frequency number of waves per second that
pass a given point in space. - 3. Speed speed of light is 2.9979 ? 108 m/s.
5Wavelength and frequency are inversely
proportional
- ? ? c
- ? frequency s?1 hertz (Hz)
- ? wavelength (m)
- c speed of light (m/s)
6Light as a particlePhotoelectric Effect
The photoelectric effect occurs when photons of
sufficient energy actually kick electrons off of
the surface being struck by light.
7Light as a particleMax Planck
Transfer of energy is quantized, and can only
occur in discrete units, called quanta.
8Plancks Constant
- ?E change in energy, in J
- h Plancks constant, 6.626 ? 10?34 J s
- ? frequency, in s?1
- ? wavelength, in m
9Light as a particleEnergy and Mass (Einstein)
- E mc2
- E energy
- m mass
- c speed of light
10Particles as wavesDeBroglie
11Particles as wavesDeBroglie
12Particles as wavesDeBroglie
- For a generic particle (not EMR)
13deBroglies Equation
- ? wavelength, in m
- h Plancks constant, 6.626 ? 10?34 J s
- m mass, in kg
- ? velocity, in m/s
14Explaining the electron
- Continuous spectrum Contains all the
wavelengths of light. - Line spectrum Contains only some of the
wavelengths of light.
15Explaining the electron
- When a sample of an elemental gas is electrified
it emits electromagnetic radiation
16Explaining the electron
- When viewed through a diffraction grating, each
element produces a distinctive line spectrum
17Hydrogens Line Spectrum(Balmer series visible)
18Hydrogens Line SpectrumUV, Visible, Infrared)
19The Bohr Model
The electron in a hydrogen atom moves around the
nucleus only in certain allowed circular orbits
(quantized energy states.)
20The Bohr Model
Orbits are determined by distance from nucleus
where orbit circumference is a whole number
multiple of the deBroglie wavelength.
21The Bohr Model
22How does Plancks Theory support Bohrs
quantized orbit
- The Hydrogen Electron Visualized as a Standing
Wave Around the Nucleus
23The Bohr Model
The energy of the orbits increases with distance
from the nucleus. Ground State The lowest
possible energy state for an atom (n 1).
24The Bohr Model
An electron can absorb energy and jump from its
ground state to a higher energy orbit (excited
state).
25The Bohr Model
Electrons will not remain in an excited
state. Electrons emit energy in the form of
photons so that they can return to the ground
state. These photons make up the line spectrum.
26The Bohr Model
The frequency of the lines depends on the size of
the jump.
27The Bohr Model
- E energy of the levels in the H-atom
- z nuclear charge (for H, z 1)
- n an integer
28Energy Changes in the Hydrogen Atom
- ?E Efinal state ? Einitial state
- ?E -2.178x 10-18J 1/nf2 1/ni2
29Quantum Model
30Quantum Mechanics
- Based on the wave properties of the atom
- ? wave function
- mathematical operator
- E total energy of the atom
- A specific wave function is often called an
orbital.
31Heisenberg Uncertainty Principle
- x position
- mv momentum
- h Plancks constant
- The more accurately we know a particles
position, the less accurately we can know its
momentum.
32Lets say you have a room with flies
flying around in it
33The flies are not just anywhere in the room. They
are inside boxes in the room.
34You know where the boxes are, and you know the
flies are inside the boxes, but
35you dont know exactly where the flies are inside
the boxes
36The room is an atom The flies are electrons The
boxes are orbitals
37The room is an atom The flies are electrons The
boxes are orbitals
Science has determined where the orbitals are
inside an atom, but it is never known precisely
where the electrons are inside the orbitals
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39Hey, where am I?
40Probability Distribution
- square of the wave function (?2)
- probability of finding an electron at a given
position -
41Quantum Numbers (QN)
- 1. Principal QN
- (n 1, 2, 3, . . .) - related to size and
energy of the orbital. - Defines an energy level or shell
42Quantum Numbers (QN)
- 2. Angular Momentum QN
- (l 0 to n ? 1) - relates to shape of the
orbital. - n and l together define a sublevel or subshell
43- Letters are also used to represent the 2nd
quantum number
l letter
0 s
1 p
2 d
3 f
44Quantum Numbers (QN)
- 3. Magnetic QN
- (ml l to ? l ) - relates to orientation of
the orbital in space relative to other orbitals.
45Quantum Numbers (QN)
- 4. Electron Spin QN (ms ½ , ? ½) - relates
to the spin states of the electrons.
46Pauli Exclusion Principle
- In a given atom, no two electrons can have the
same set of four quantum numbers (n, l, ml , ms). - Therefore, an orbital can hold only two
electrons, and they must have opposite spins.
47So what are the sizes and shapes of orbitals?
48The area where an electron can be found, the
orbital, is defined mathematically, but we can
see it as a specific shape in 3-dimensional space
49z
y
x
50z
y
The 3 axes represent 3-dimensional space
x
51z
y
For this presentation, the nucleus of the atom is
at the center of the three axes.
x
52The 1s orbital is a sphere, centered around the
nucleus
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55The 2s orbital is also a sphere.
56The 2s electrons have a higher energy than the
1s electrons. Therefore, the 2s electrons are
generally more distant from the nucleus, making
the 2s orbital larger than the 1s orbital.
571s orbital
582s orbital
59Dont forget an orbital is the shape of
the space where there is a high probability of
finding electrons
60Dont forget an orbital is the shape of
the space where there is a high probability of
finding electrons
The s orbitals are spheres
61There are three 2p orbitals
62The three 2p orbitals are oriented perpendicular t
o each other
63z
This is one 2p orbital (2py)
y
x
64z
another 2p orbital (2px)
y
x
65z
the third 2p orbital (2pz)
y
x
66Dont forget an orbital is the shape of
the space where there is a high probability of
finding electrons
67Dont forget an orbital is the shape of
the space where there is a high probability of
finding electrons
This is the shape of p orbitals
68z
y
x
69z
2px
y
x
70z
2px and 2pz
y
x
71z
The three 2p orbitals, 2px, 2py, 2pz
y
x
72once the 1s orbital is filled,
73the 2s orbital begins to fill
74once the 2s orbital is filled,
75the 2p orbitals begin to fill
76each 2p orbital intersects the 2s orbital and the
1s orbital
77each 2p orbital gets one electron before pairing
begins
78once each 2p orbital is filled with a pair of
electrons, then
79the 3s orbital gets the next two electrons
80the 3s electrons have a higher energy than 1s,
2s, or 2p electrons,
81so 3s electrons are generally found further from
the nucleus than 1s, 2s, or 2p electrons
82D orbitals
83f orbitals