Angular frequency of a matter patter

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SUMMARY

The discussion centers on the angular frequency (\(\omega\)) in the de Broglie relation \(E = \hbar \cdot \omega\) and its behavior under varying conditions, particularly in different gravitational fields and electromagnetic environments. Participants explore whether \(\omega\) is a constant or an average, especially in the context of spin-1/2 particles and their probability amplitude functions (\(\Psi\)). The conversation also touches on practical examples, such as tunneling through a square potential barrier, to illustrate how the wave vector changes in different regions.

PREREQUISITES
  • Understanding of quantum mechanics concepts, particularly de Broglie relations
  • Familiarity with wave functions and probability amplitude functions in quantum physics
  • Knowledge of electromagnetic fields and their influence on particle behavior
  • Basic grasp of potential barriers and quantum tunneling phenomena
NEXT STEPS
  • Study the implications of gravitational redshift on angular frequency in quantum mechanics
  • Investigate the effects of varying electromagnetic fields on wave functions
  • Learn about quantum tunneling and its mathematical representation through wave vectors
  • Explore advanced topics in quantum field theory related to particle behavior in non-uniform fields
USEFUL FOR

Physics students, quantum mechanics researchers, and anyone interested in the behavior of matter particles in varying fields will benefit from this discussion.

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By the de Broglie relations: E = [tex]\hbar * \omega[/tex]

Is the angular frequency ([tex]\omega[/tex]) in this equation an average or is it a constant? In other words, does the angular frequency (or the wavenumber, k) for a matter particle change, for instance, in differing gravitational fields, such as we see for a photon with gravitational redshift?
 
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I can restate the question in a related way.

Assume a spin-1/2 particle is described by a probability amplitude function ([tex]\Psi[/tex]) with angular frequency ([tex]\omega[/tex]) or wavenumber (k). The probability amplitude distribution for that particle exists within a volume of space-time. Assume that within that volume of space-time, there is an electromagnetic field that varies significantly in strength over that volume. How does that varying electromagnetic field affect the wavenumber/angular frequency of the particle's probability amplitude distribution?
 
Er... I have almost no clue on what you're getting at here.

Let's look at a less "exotic" example, shall we? Something that every single physics undergraduate does - tunneling through a square potential barrier. Look at the wave vector as it goes through the various regions. Does it change?

Zz.
 

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