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9.8 Option - From quanta to quarks: 2. de Broglie: The electron is a wave!

Syllabus reference (October 2002 version)
2. The limitations of classical physics gave birth to quantum physics
Students learn to: Students:

Extract from Physics Stage 6 Syllabus (Amended October 2002) © Board of Studies, NSW.
[Edit 14 Aug 08]

Prior learning: Preliminary modules 8.2, 8.3, 8.4.

Background: The Bohr model of the atom was a great step forward but couldn't explain the problem of why the electron didn't spiral into the nucleus with catastrophic results. De Broglie could explain that phenomenon. A new era in science had begun.

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describe the impact of De Broglie’s proposal that any kind of particle has both wave and particle properties

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solve problems and analyse information using: lamda=h/mv

lamda=h/mv expanded

Note the size of this wavelength is very short. It is this short wavelength that makes the use of electrons in the electron microscope so effective in producing high resolution images of objects with fine detail.

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define diffraction and identify that interference occurs between waves that have been diffracted

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describe the confirmation of de Broglie’s proposal by Davisson and Germer

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explain the stability of the electron orbits in the Bohr atom using De Broglie‘s hypothesis

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gather, process, analyse and present information and use available evidence to assess the contributions made by Heisenberg and Pauli to the development of atomic theory

Sample information

The contribution made by Heisenberg and Pauli to the development of atomic theory was significant in that they took the ideas of others and developed a theoretical basis for describing why these things happened through mathematics. Werner Heisenberg developed the mathematical theory of quantum mechanics because he was unhappy with the mixed classical and quantum model of Bohr's that was used to explain the hydrogen atom. Pauli took the quantum mechanical model that was in its entirety theoretical and applied it to the hydrogen atom and was theoretically able to derive the Rhydberg constant and to develop Balmer's equation. This was the first time in the history of atomic physics where the theoretical preceded the supporting observation.

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