Unit I On-a-Page

Principles and Definitions

If you have had Dr. Toggerson or Dr. Bourgeois for Physics 131, you are familiar with a distinction made between principles and definitions. The are the fundamental rules of the Universe that describe how things work. Concepts which are , on the other hand, simply describe a quantity. For example,

\vec{p} = m \vec{v}

is the definition of momentum for a massive particle; this equation offers no deep foundational insights into how the universe works. We physicists simply noted that the quantity m\vec{v} came up a lot, and we gave it a name \vec{p}. In order to describe how the Universe works, principles often involve multiple definitions. Note that sometimes a principle or definition has an equation, while other times it is just stated in words! This point connects to Physics Goals 1 and 2 for this course.

To help acquaint those of you who may not be used to this distinction and to help organize the huge amount of factual information in this particular unit, I will list the principles for this unit. You can quickly see how short this list is.

Principles for This Unit

  • “Waves are shy” – Quantum objects like light and electrons exist/propagate as waves. They only really behave in a particle-like manner when they interact/are observed.
  • Since quantum objects exhibit both wave and particle properties, we need to be able to move back and forth between the two pictures – As you can see in the table below, both waves and particles have two independent properties. The goal is to move between them.
    Wave Properties Particle Properties
    Amplitude \leftarrow \; \psi^2 \propto P, N \; \rightarrow Probability of being at a location / Number of particles
    Wavelength  \leftarrow \; p = \frac{h}{\lambda} \; \rightarrow Momentum
  • A confined wave must “fit in the box” – Thus, we must have an integer number of half-waves. For a nice symmetrical box, or box-like molecule, the wave will evenly fit in the box  n \left( \frac{\lambda}{2} \right) = L . However, even in situations such as atoms where the electron is more strongly attracted to the nucleus, we will have an integer number of half waves.
  • Energy must be conserved  \Delta E = Q

Other Basic Properties You Should Know

  • The SI prefixes from nano- (n) to Giga- (G)
  • Light in a vacuum always travels at the speed of light c=299792458 \, \frac{\mathrm{m}}{\mathrm{s}}
  • The A is independent of wavelength \lambda
  • Free electrons have zero potential energy; all bound electrons, having lower energy than this, have negative potential energy.
A Venn-diagram showing the different sciencesIn chemistry, you probably saw the conversion between energy and wavelength for photons done through the equation  E = \frac{hc}{\lambda} . We will NOT consider that as a principle to begin analyses / solving problems. The reason is that, in chemistry, you only consider converting between energy and wavelength for photons. We want to think about BOTH photons AND electrons. It turns out that  E = \frac{hc}{\lambda} ONLY works for photons, while  p = h / \lambda works for both photons and electrons! Thus, we consider  p = h/\lambda to be our principle. Many students get tripped up by applying  E = \frac{hc}{\lambda} to electrons. Don’t fall into this trap!

 

Instructor’s Note

 

The ideas in this unit can be connected in many different ways. One possible useful way to organize such information is in a “concept map” like the one shown below. The map is also available at this link.

In this map:

  • UMass maroon bubbles are big ideas.
  • Yellow bubbles apply to massless particles, such as light.
  • Green bubbles apply to massive particles, such as electrons.

I recommend printing a copy for use in class!

A concept map of all of the ideas in Unit 1

License

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Physics 132: What is an Electron? What is Light? by Roger Hinrichs, Paul Peter Urone, Paul Flowers, Edward J. Neth, William R. Robinson, Klaus Theopold, Richard Langley, Julianne Zedalis, John Eggebrecht, and E.F. Redish is licensed under a Creative Commons Attribution 4.0 International License, except where otherwise noted.

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