Title: Qualitative introduction to quantum theory
1Qualitative introduction to quantum theory
BS1030, Chemistry for Life Scientists November
11, 2008
- Prof. Judith Klein-Seetharaman
- School of Biological Sciences
- j.klein-seetharaman_at_rhul.ac.uk
2Overview
- Today Study of atomic structure - from classical
mechanics to quantum theory - Energy is quantized
- Wave-particle duality
- Next week Application of quantum theory to
describe atomic structure - The uncertainty principle
- The Schroedinger equation
- Quantum numbers
- Atomic orbitals
- Third week Bonding and shapes of molecules
- Types of bonds
- MO theory
Atkins Jones Chapter 1.1-1.6
Atkins Jones Chapter 1.7-1.22
Atkins Jones Chapter 23
3Atomic Structure
4Atomic Structure
- Dalton featureless spheres
- J.J. Thomson discovery of the electron as the
first sub-atomic particle (neg. charge) - Robert Millikan determined the charge of the
electron - But atom is neutral
- J.J. Thomson atom is a blob of a positively
charged jelly with electrons like raisins - Ernest Rutherford shoot positive charges from
atoms against a thin platinum foil - What do you expect to find? In JJ Thomsons
model? In alternative models?
5Shooting alpha particles on a thin foil
1 in 20,000 is deflected with very large angle
Most go through
6Rutherfords Atom Model
- Nucleus many times smaller than itself with
electrons occupying the rest of the space - What are the electrons doing in the atom?
7The answer came from
8(No Transcript)
9The answer came from
- The study of light emitted by heated atoms
10The answer came from
- The study of light emitted by heated atoms
11What is light?
- electromagnetic radiation
- Oscillating electric and magnetic fields
traveling at the speed of light - of cycles is frequency
- 1Hz s-1
- One cycle per second
- Amplitude
- Wavelength
l v c
Wavelength x Frequency speed of light
12What is the speed of light
- In vacuum 2.998 108 m/s
- Radar waves leave earth, bounce off the moon and
come back in 2.5 seconds (478,000 miles)
13Short or long wavelength?
14What is the wavelength of red?of blue?which
frequency?other waves?
15Continuous Spectrum
16Atomic spectra
17There are patterns in the lines
- First Joseph Balmer, a swiss school teacher in
1885 - Then Johann Rydberg, a swedish spectroscopist
18What does it mean?
19What does it mean?
- The electrons in an atom can only have certain
energies. - Energy is quantized.
20Next puzzle black body radiation
21Next puzzle black body radiation
- With increasing temperature, the total energy
emitted increases and the maximum intensity
shifts to shorter wavelengths.
22Stefan-Boltzmann Law
Wiens Law
23Can you determine the temperature on the surface
of the sun?
24A red giant is a late stage in the evolution of a
star. The average wavelength maximum is 700nm.
- What is the temperature of the star?
25What is the wavelength emitted by the human body?
26Why does the wavelength shift with T?
- Classical physics puts no restriction on how
small a quantum can be transferred between matter
and radiation - Thus, classical physics says any hot body should
emit any wavelength - Even a human body would glow in the dark
- There would be no darkness
- Something is wrong! Ultraviolet catastrophe
27Plancks answer
E hn
- Energy exchange between matter and radiation is
quantized - Low frequencies, not enough energy to stimulate
oscillations - hPlanck constant
- Can reproduce Wiens and Stefan-Boltzmann laws
perfectly
28The nail in the coffin Photoelectric effect
- No electrons are ejected if the frequency of the
radiation is below a threshold value
characteristic of the metal. - Immediate ejection of electrons however low the
intensity of the radiation. - The kinetic energy of the ejected electrons
increases linearly with the frequency of the
incident radiation.
29Einsteins explanation
- Einstein proposed that electromagnetic radiation
consists of particles, which were later called
photons - Each photon is a packet of energy
- Questions
- A. What is the energy of a photon e.g. of blue
light? - B. Why kinetic energy linear?
30Bohr Frequency Condition
- The frequency in a line spectrum of an atom
arises from transition between two energy levels
31Light is also waves
- Best evidence Diffraction
32From waves to particles back to waves
- Line spectrum of atoms
- Bohrs frequency condition
- Black body radiation
- Plancks quantization of energy
- Photoelectric effect
- Einsteins particle interpretation
- Diffraction
- Clearly a wave-related property
33Wave-Particle Duality
- In the wave model, the intensity of the radiation
is proportional to the square of the amplitude of
the wave. - In the particle model, the intensity is
proportional to the number of photons present.
34Generalization to all particles
- French scientist Louis de Broglie proposed that
all particles should have wavelike properties
35The wave-like behavior of electrons can be
experimentally observed
36Electron Microscope
- Electrons have wavelengths suitable to image
biological samples down to near-atomic resolution
37The Dr. Jekyll Mr. Hyde of Physics
The Electron Wave Particle
38Crime Scene Investigators
Ernest Rutherford New Zealand Physicist
(1871-1937) Nobel Prize in Chemistry 1908
Max Planck German Physicist (1858-1947) Nobel
Prize in Physics 1918
Albert Einstein German Physicist
(1879-1955) Nobel Prize in Physics 1921
Robert Millikan American Physicist
(1868-1953) Nobel Prize in Physics 1923
Niels Bohr Danish Physicist (1885-1962) Nobel
Prize in Physics 1922
Joseph John Thomson British Physicist
(1856-1949) Nobel Prize in Physics 1906
39Now you (should) know
- Why we need quantum mechanics
- That Energy is quantized
- That matter shows particle/wave duality
- What are characteristics of particles
- What are characteristics of waves
- How to calculate energies, frequencies,
wavelengths