Understanding Classical Physics: The Role of Planck Constant

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SUMMARY

The discussion centers on the relationship between the Planck constant and classical physics, asserting that classical physics emerges when the Planck constant approaches zero. Specifically, as the Planck constant (h) tends to zero, the energy spacing (E = hv) also approaches zero, resulting in a continuous energy spectrum that negates quantization. This transition occurs at macroscopic scales, where the effects of quantum mechanics become negligible, similar to how special relativity becomes irrelevant at low speeds compared to the speed of light.

PREREQUISITES
  • Understanding of quantum mechanics principles
  • Familiarity with the Planck constant (h)
  • Knowledge of energy quantization (E = hv)
  • Basic concepts of special relativity (SR)
NEXT STEPS
  • Explore the implications of Planck's constant in quantum mechanics
  • Study the transition from quantum mechanics to classical physics
  • Investigate the relationship between energy spacing and wave intensity
  • Learn about the effects of special relativity at varying speeds
USEFUL FOR

Students of physics, educators in classical and quantum mechanics, and researchers exploring the foundational principles of physical theories.

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Classical physics can essentially be defined as the limit of quantum mechanics as the Planck constant tends to zero.
If the Planck constant tends to zero, it's obviously just getting smaller, so how would this describe classical physics?

Is this a way of explaining it?:

If energy spacing E = hv, and h --> 0, then E --> 0, which is essentially a continuous energy spectrum and quantization and discreteness goes away. Hence classical physics.


Thanks.
 
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It's about Planck's constant relative to the scale you're dealing with. If your scale is meters, Planck's constant is negligible and you get classical physics. If your scale is angstroms or smaller, Planck's constant is quite relevant and you get QM.

It's not unlike the relationship between SR and the speed of light. At low speeds, the speed of light is practically infinite, so you needn't worry about relativistic calculations. At speeds of, say, .8c, the speed of light becomes important.

If energy spacing E = hv, and h --> 0, then E --> 0, which is essentially a continuous energy spectrum and quantization and discreteness goes away. Hence classical physics.
That's definitely one way of looking at it. More accurately, you would say delta_E = hv, and so as h->0, delta_E = dE, and you get a continuous energy spectrum that would require us to consider things like intensity of the wave which we've since largely discarded.
 
Yeah, I really meant to say dE. :smile:
 

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