Can the Uncertainty Principle Explain High Electron Energies in the Nucleus?

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SUMMARY

The discussion centers on applying the uncertainty principle to determine the kinetic energy of an electron hypothetically located within a nucleus, specifically at a radius of approximately 10^-15 m. The initial calculations using the uncertainty relation (Δx)(Δp) ≥ ħ led to an unphysical result for velocity, exceeding the speed of light. The correct approach involves recognizing that for ultra-relativistic particles, the energy can be approximated as E ≈ pc, leading to a calculated kinetic energy of approximately 500 MeV for the electron, which aligns with the conclusion that electrons cannot exist in the nucleus.

PREREQUISITES
  • Understanding of the Heisenberg Uncertainty Principle (Δx)(Δp) ≥ ħ
  • Familiarity with special relativity, particularly the energy-momentum relation E² = (pc)² + (mc²)²
  • Knowledge of relativistic kinetic energy calculations, K = (γ - 1)mc²
  • Basic concepts of particle physics, including the Compton wavelength
NEXT STEPS
  • Study the implications of the Heisenberg Uncertainty Principle in quantum mechanics
  • Learn about ultra-relativistic particles and their energy-momentum relationships
  • Explore the concept of Compton wavelength and its relevance in particle physics
  • Investigate the role of kinetic energy in nuclear physics and the behavior of electrons in atomic structures
USEFUL FOR

This discussion is beneficial for physics students, educators, and anyone interested in quantum mechanics and nuclear physics, particularly those exploring the implications of the uncertainty principle on particle behavior within atomic nuclei.

Kazuya
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Hi, I'm a first year physics student at the University of Oregon and I was hoping that someone here might be able to help me with a problem I've been having.

A question on my assignment asks me to "Use the uncertainty principle to show that if an electron were present in the nucleus (r = approximately 10^-15 m), its kinetic energy (use relativity) would be hundreds of MeV. (Since such electron energies are not observed, we conclude that electrons are not present in the nucleus). [Hint: a particle can have energy as large as its uncertainty.]

Firstly, I decided to use the form of uncertainty principle (delta x)(delta p) is approximately larger than h-bar. I used (10^-15 m) as (delta x) and split (delta p) into m(delta v). I than used the rest mass of an electron (9.11x10^-31 kg) as m and attempted to solve for (delta v). [Using h-bar = 1.055x10^-34 J*s]. Unfortunately, this gave me an answer of (delta v) is approximately larger than (1.15x10^11 m/s)... which of course is much larger than c (3.00x10^8 m/s).

Already I knew there was a problem... when attempting to find K = (gamma - 1)mc^2, gamma becomes something like (382i)^-1/2. This is a definite problem because we haven't begun using non-real numbers (i) in this course yet.

Does anyone see an obvious problem with what I'm doing? Should I be using (delta E)(delta t) approximately larger than h-bar for the uncertainty principle? For my special relativity equation should I use E^2 =(p^2)(c^2) + (m^2)(c^4)?

I've spent several hours on this problem trying every imaginable route and have even come to the conclusion (incorrectly, of course) that [1+ (m^2)(c^2)] is approximately larger than 1/(2pi)^2! Any help is greatly appreciated.
 
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Originally posted by Kazuya
Hi, I'm a first year physics student at the University of Oregon and I was hoping that someone here might be able to help me with a problem I've been having.

A question on my assignment asks me to "Use the uncertainty principle to show that if an electron were present in the nucleus (r = approximately 10^-15 m), its kinetic energy (use relativity) would be hundreds of MeV. (Since such electron energies are not observed, we conclude that electrons are not present in the nucleus). [Hint: a particle can have energy as large as its uncertainty.]

Firstly, I decided to use the form of uncertainty principle (delta x)(delta p) is approximately larger than h-bar. I used (10^-15 m) as (delta x) and split (delta p) into m(delta v). I than used the rest mass of an electron (9.11x10^-31 kg) as m and attempted to solve for (delta v). [Using h-bar = 1.055x10^-34 J*s]. Unfortunately, this gave me an answer of (delta v) is approximately larger than (1.15x10^11 m/s)... which of course is much larger than c (3.00x10^8 m/s).

Already I knew there was a problem... when attempting to find K = (gamma - 1)mc^2, gamma becomes something like (382i)^-1/2. This is a definite problem because we haven't begun using non-real numbers (i) in this course yet.

Does anyone see an obvious problem with what I'm doing? Should I be using (delta E)(delta t) approximately larger than h-bar for the uncertainty principle? For my special relativity equation should I use E^2 =(p^2)(c^2) + (m^2)(c^4)?

I've spent several hours on this problem trying every imaginable route and have even come to the conclusion (incorrectly, of course) that [1+ (m^2)(c^2)] is approximately larger than 1/(2pi)^2! Any help is greatly appreciated.

You began well by saying that p is of the order of hbar/Δx.
Instead of finding the velocity of the electron just compare pc with mc^2. Why that? Remember that E = γmc^2 and p = γmv. So that p/E = v/c^2 and if the velocity is of the order of c, you get E is approximately equal to pc. When you put this result in the equation E^2 =(p^2)(c^2) + (m^2)(c^4), you see thatthis means that you can neglect mc^2 wrt pc. In fact there is a terminology for this. A particle is said to be ultra-relativistic if its velocity is so closed to c that it can be treated as a zero mass particle where E=pc.

In the case of ultra-relativistic, almost all the energy will be kinetic energy.

If you look at your example you have p = h/r so that Ek = hbar*c/r.
remember that the compton wavelength of the electron is given by λ = hbar/mc, you will find that Ek = λ/r*mc^2.
For the electron, &lambda is about 10^-12 m, r is about 10^-15 and mc^2 is 0.5 MeV. So you get Ek is about 500MeV.

Hope I could help
 
Awesome =) Thanks for the help!
 

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