Lecture notes: CHEM103
Spring 2008 – September 30, 2008
GOAL: UNDERSTAND THE NATURE OF ELECTRONS
HOW? BY THE UNDERSTANDING THE INTERACTIONS OF
LIGHT WITH MATTER
OBJECTIVES FOR TODAY:
0)
NOTE ABOUT LAB THIS
WEEK!
1)
REVIEW:
particle-wave duality
a.
light as a wave,
including proof
2)
Light as a particle
a.
Maxwell Planck
& blackbody radiation: quantum mechanics
b.
Line spectra of
gases and in the sun
c.
Proof of particle
nature from Einstein
3)
Bohr & “solar
system” model of the atom
4) Electrons ALSO behave as waves (duality): MORE quantum mechanics
5)
everything PARTICLE as WAVES: the DeBroglie equation: EVEN MORE quantum
mechanics
6) emission
and absorption of light by atoms: INTERACTION OF LIGHT W/ MATTER
7)
calculating electron energy changes in atomic transitions USING Planck &
Rydberg
The nature of light:
particle-wave duality

1) light
can be described as a WAVE: using the concepts of wavelength & frequency

Proof
that light behaves as a wave:
Examples: diffraction

interference
now: combine diffraction
& interference (2 slit experiment)

INTERACTIONS
BETWEEN LIGHT AND MATTER, continued…
2) light can be described as a
PARTICLE – can be counted individually:
Maxwell Plank
and “blackbody radiation”
http://ephysics.physics.ucla.edu/physlets/eblackbody.htm
NOW: “CLASSICAL
MECHANICS VS. QUANTUM MECHANICS”
Planck’s
idea…
you
can’t break up energy into inifinitely small bits, but must take it in pieces.
(Analogy: gaining potential
energy (height) by climbing the stairs, instead of walking up a ramp.)
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Eradiation = n × h × n
h =
6.626×10-34 J·sec (Planck’s constant)
“nu” =
frequency (Hz or seconds-1)
(AND n = 0, 1, 2, 3… the
number of steps OR “QUANTA”)
SO: h×n describes the energy of ONE
photon (Planck’s constant x
photon frequency)
…and we can write:
Ephoton = h × n
EXAMPLE: SUN
RADIATES LIGHT; EARTH RADIATES LIGHT…
http://ephysics.physics.ucla.edu/greenhouse/HTML/greenhouse.htm

Calculate
the amount of energy in a photon with a wavelength of 500 nm:
“ …with a wavelength of 12 mm:
c =
l × n (speed = wavelength x
frequency)
Ephoton = h × n
combine these…
LINE SPECTRA
(EMITTED AND ABSORBED)
note: this is very different than
“blackbody radiation”

Emission lines for different materials
Different
colors = different wavelengths;
Different wavelengths = different
frequencies
Different frequencies
= different energies, but only at specific values!

“Frauenhofer
lines” in the solar spectrum
What does this mean?
Light is being absorbed
at specific energies.
Conservation
of energy tells us the energy must go somewhere!
WHERE? Into the atoms; but specifically into the electrons
– SO THESE INTERACT!
Remember: from this point forward,
it is the electrons that
define chemical properties!
AND, for electrons,
location doesn’t matter – ENERGY is everything!
FINALLY:
PROOF THAT THIS SOLUTION REALLY WORKS!
Albert
Einstein’s interpretation of the photoelectron effect (1905)
http://www.xmission.com/~locutus/applets/Photoelectric.html
http://ephysics.physics.ucla.edu/photoelectric/HTML/photoelectric.htm

KEY IDEA: NUMBER
OF PHOTONS (INTENSITY) IS LESS IMPORTANT THAN ENERGY OF PHOTONS (FREQUENCY);
ONCE THRESHOLD FREQUENCY IS EXCEEDED,
THEN INTENSITY MATTERS
SO WE GO BACK
TO THE ATOM & ELECTRONIC “STRUCTURE”
Neils Bohr
and the Hydrogen Atoms (1911)
(a
postdoctoral student of JJ Thomson AND Rutherford)
http://galileo.phys.virginia.edu/classes/252/Bohr_Atom/Bohr_Atom.html
THEORY: Electrons “orbit” the nucleus much like
planets orbit the sun – but the attraction different!
(Why is this a
problem?)

THE SOLUTION: just like light,
the
orbital velocities (angular momentum) of these electron orbits are
QUANTIZED!
(ONLY CERTAIN
SOLUTIONS TO THE PROBLEM ALLOWED!)
BUT THIS ONLY
WORKS IF ELECTRONS ARE A WAVE, JUST LIKE LIGHT…
How this
helps with Bohr’s quantum electron orbits – a way to think about it…
http://mutuslab.cs.uwindsor.ca/schurko/molspec/animations/bird_concordia/HydrogenSpectrum_2.htm