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Transcript
Chapter 7 Lecture
Lecture Presentation
Chapter 7
The QuantumMechanical Model
of the Atom
----Revised by Wang
Sherril Soman
Grand Valley State University
© 2014 Pearson Education, Inc.
The Nature of Light: Its Wave Nature
• Light: a form of electromagnetic radiation
Composed of perpendicular oscillating waves,
one for the electric field, and
one for the magnetic field
• All electromagnetic waves move through
space at the same, constant speed.
3.00 × 108 m/s = the speed of light
© 2014 Pearson Education, Inc.
Speed of Energy Transmission
© 2014 Pearson Education, Inc.
Characterizing Waves
• The amplitude is the height of the wave.
– The amplitude is a measure of light intensity.
The larger the amplitude, the brighter the light.
crest
trough
© 2014 Pearson Education, Inc.
Characterizing Waves
• The wavelength (l) is a measure of the
distance covered by the wave.
Wavelength (l)
© 2014 Pearson Education, Inc.
Characterizing Waves
• The frequency (n) is the number of waves (the
number of cycles) that pass a point in a given
period of time.
– Units are hertz (Hz) or cycles/s = s−1 (1 Hz = 1 s−1).
• The total energy is proportional to,
the amplitude of the waves, and
the frequency.
© 2014 Pearson Education, Inc.
The Relationship Between
Wavelength and Frequency
speed, m/s
frequency,
/s (or Hz)
wavelength, m
Example 7.1 Wavelength and Frequency
Calculate the wavelength (in nm) of the red light emitted by a
barcode scanner that has a frequency of 4.62 × 1014 s–1.
© 2014 Pearson Education, Inc.
Color
• The color of light is determined by its
wavelength or frequency.
• White light is a mixture of all the colors
of visible light.
– A spectrum
– Red Orange Yellow Green Blue Indigo
Violet
• When an object absorbs some of the
wavelengths of white light and reflects
others, it appears colored. The observed
color is predominantly the colors
reflected.
© 2014 Pearson Education, Inc.
Amplitude and Wavelength
© 2014 Pearson Education, Inc.
The Electromagnetic Spectrum
• Visible light comprises only a small fraction of
all the wavelengths of light, called the
electromagnetic spectrum.
© 2014 Pearson Education, Inc.
Continuous Spectrum
© 2014 Pearson Education, Inc.
Thermal Imaging using Infrared Light
© 2014 Pearson Education, Inc.
Using High-Energy Radiation
to Kill Cancer Cells
During radiation therapy, a tumor is
targeted from multiple directions in order to
minimize the exposure of healthy cells, while
maximizing the exposure of cancerous cells.
© 2014 Pearson Education, Inc.
Electromagnetic wave – particles or
waves ?
© 2014 Pearson Education, Inc.
Electromagnetic wave – particles or
waves ?
© 2014 Pearson Education, Inc.
Einstein’s Explanation
• Einstein proposed that the light energy was
delivered to the atoms in packets, called quanta
or photons.
• The energy of a photon of light is directly
proportional to its frequency.
– Inversely proportional to its wavelength
– The proportionality constant is called Planck’s
Constant, (h), and has the value 6.626 × 10−34 J ∙ s.
© 2014 Pearson Education, Inc.
Einstein’s Explanation
Example 7.2 Photon Energy
A nitrogen gas laser pulse with a wavelength of 337 nm contains
3.83 mJ of energy. How many photons does it contain?
© 2014 Pearson Education, Inc.
Spectra
• When atoms or molecules absorb energy, that
energy is often released as light energy,
– Fireworks, n
– eon lights, etc.
Na
© 2014 Pearson Education, Inc.
K
Li
Ba
Emission Spectra
© 2014 Pearson Education, Inc.
Indication of energy level of electrons
 Electrons in atoms are at discrete energy
levels.
 The energy difference between the high
level and the low level equals to the emitted
photon energy.
© 2014 Pearson Education, Inc.
Rydberg’s Spectrum Analysis
Johannes Rydberg (1854–1919)
• Rydberg analyzed the spectrum of
hydrogen and found that it could be
described with an equation that involved an
inverse square of integers.
© 2014 Pearson Education, Inc.
Rutherford’s Nuclear Model
• The atom contains a tiny dense center called the
nucleus.
• The nucleus is essentially the entire mass of
the atom.
• The nucleus is positively charged .
• The electrons move around in the empty space of
the atom surrounding the nucleus.
© 2014 Pearson Education, Inc.
Problems with Rutherford’s Nuclear Model
of the Atom
• Electrons are moving charged particles.
• According to classical physics, moving charged
particles give off energy.
• Therefore, electrons should constantly be giving
off energy.
– This should cause the atom to glow!
• The electrons should lose energy, crash into the
nucleus, and the atom should collapse!
– But it doesn’t!
© 2014 Pearson Education, Inc.
The Bohr Model of the Atom
Neils Bohr (1885–1962)
• Bohr’s major idea was that the energy of the atom
was quantized, and that the amount of energy in
the atom was related to the electron’s position in
the atom.
– Quantized means that the atom could only have very
specific amounts of energy.
© 2014 Pearson Education, Inc.
Bohr Model of H Atoms
© 2014 Pearson Education, Inc.
Bohr Model of H Atoms
photonener gy  E  E final  Einitial
 1

1

hn  2.18 10 J 

2
2
n

n
final
initial


 1
c
1 
18 
h  2.18 10 J

2
2 

l
n
n
initial 
 final
18
© 2014 Pearson Education, Inc.
Bohr Model of H Atoms
© 2014 Pearson Education, Inc.
Bohr Model of H Atoms
© 2014 Pearson Education, Inc.
Bohr Model of H Atoms
Example 7.7 Wavelength of Light for a Transition in the Hydrogen Atom
Determine the wavelength of light emitted when an electron in a
hydrogen atom makes a transition from an orbital in n = 6 to an
orbital in n = 5.
photonener gy   E  Einitial  E final
hn  2.18  10
h
c
l
18
 2.18  10
© 2014 Pearson Education, Inc.
 1

1

J

2
2
n

n
final
initial


18
 1
1 

J

n 2 n 2 
initial 
 final
Wave Behavior of Electrons
Louis de Broglie (1892–1987)
• de Broglie proposed that particles could have
wavelike character.
v, speed
Electron Diffraction
© 2014 Pearson Education, Inc.
Uncertainty Principle
• Heisenberg stated that the product of the
uncertainties in both the position and speed of a
particle was inversely proportional to its mass.
– x = position, x = uncertainty in position
– v = velocity, v = uncertainty in velocity
– m = mass
• This means that the more accurately you know
the position of a small particle, such as an
electron, the less you know about its speed, and
vice versa.
© 2014 Pearson Education, Inc.
Schrödinger’s Equation
• Schrödinger’s equation allows us to
calculate the probability of finding an
electron with a particular amount of energy
at a particular location in the atom.
• Solutions to Schrödinger’s equation
produce many wave functions, Y.
• A plot of distance versus Y 2 represents an
orbital, a probability distribution map of a
region where the electron is likely to be found.
© 2014 Pearson Education, Inc.
Solutions to the Wave Function, Y
• Calculations show that the size, shape, and
orientation in space of an orbital are
determined to be three integer terms in the
wave function.
– Added to quantize the energy of the electron.
• These integers are called quantum
numbers.
– Principal quantum number, n
– Angular momentum quantum number, l
– Magnetic quantum number, ml
© 2014 Pearson Education, Inc.
Principal Quantum Number, n
• Characterizes the energy level of the electron in
a particular orbital.
– Corresponds to Bohr’s energy level
• n can be any integer  1.
• n is also called principal shell.
© 2014 Pearson Education, Inc.
Angular Momentum Quantum Number, l
• The angular momentum quantum number
determines the shape of the orbital. It is
also called subshell.
• l can have integer values from 0 to (n – 1).
• Each value of l is called by a particular letter
that designates the shape of the orbital.
–
–
–
–
I =0, s,
I =1, p,
I =2, d,
I =3, f.
© 2014 Pearson Education, Inc.
Energy Levels and Sublevels
© 2014 Pearson Education, Inc.
?
Energy Levels and Sublevels
Example 7.5 Quantum Numbers I
What are the quantum numbers and names (for example, 2s, 2p) of
the orbitals in the n = 4 principal level?
© 2014 Pearson Education, Inc.
Magnetic Quantum Number, ml
• The magnetic quantum number is an integer
that specifies the orientation of the orbital.
– The direction in space the orbital is aligned
relative to the other orbitals
• Values are integers from −l to +l
– Including zero
– Gives the number of orbitals of a particular shape
• When l = 2, the values of ml are −2, −1, 0, +1, +2,
which means there are five orbitals with l = 2.
© 2014 Pearson Education, Inc.
Magnetic Quantum Number, ml
© 2014 Pearson Education, Inc.
n, l, ml
© 2014 Pearson Education, Inc.
n, l, ml
Example 7.6 Quantum Numbers II
These sets of quantum numbers are each supposed to specify an
orbital. One set, however, is erroneous. Which one and why?
a.n = 3; l = 0; ml = 0 b. n = 2; l = 1; ml = –1
c. n = 1; l = 0; ml = 0 d. n = 4; l = 1; ml = –2
© 2014 Pearson Education, Inc.
Describing an Orbital
• Each set of n, l, and ml describes one
orbital.
• Orbitals with the same value of n are in the
same principal energy level.
– Also called the principal shell
• Orbitals with the same values of n and l are
said to be in the same sublevel.
– Also called a subshell
© 2014 Pearson Education, Inc.
l = 0, the s Orbital
© 2014 Pearson Education, Inc.
l =1, p Orbitals
© 2014 Pearson Education, Inc.
l =2, d Orbitals
© 2014 Pearson Education, Inc.
l=3, f Orbitals
© 2014 Pearson Education, Inc.