.
History 181B:  Modern Physics
Class 23 (3/9/01)
The old quantum theory of atomic structure
Navigation
Home Schedule < Previous Class Next Class >
 
Outline Atomic models

     Empirical starting points:  constitution and construction

     Early proposals
          J.J. Thomson's
          Rutherford's

     A comment:  the model-making tradition

     Bohr's model
          How Bohr came to Rutherford
          Imposing a nonclassical stability condition on allowed orbits
          What are the experimental consequences?

Discrete spectra

     Background:  observations and apparatus
     Signatures of the chemical elements
     How are spectral lines produced?  Models of oscillating electrons

Returning to Bohr's model

     Hypotheses about light emission:  transitions between orbits
     Two quantization conditions, two fundamental principles
     What it explains:  spectra, the periodic table
     The correspondence principle

Names and terms 
Primary Secondary
J.J. Thomson (1856-1940), NP 1906
Ernest Rutherford (1871-1937), NP Chemistry 1908
Niels Bohr (1885-1962), NP 1922
orbits
discrete spectrum = line spectrum
prism
Balmer spectrum (of hydrogen)
DE = hn
J = n(h/2p) = n x "h-bar"
Hantaro Nagaoka (1865-1950)
Joseph (von) Fraunhofer (1787-1826)
Gustav Kirchhoff (1824-1887)
Robert Bunsen (1811-1899)
Copyright © Cathryn Carson 2001