Pauli Exclusion Principle: Quantum Coherence & Range

Click For Summary
SUMMARY

The Pauli Exclusion Principle is crucial in various states of matter, particularly in atoms, metals, and white dwarfs. John Thompson emphasizes that the principle requires antisymmetrization of the wavefunction, which remains significant as systems cool down to their ground states. In these conditions, quantum effects dominate over thermal motion, impacting electron configurations and stability. The principle's relevance diminishes at higher temperatures, where fermions occupy higher energy states, reducing the observable effects of exclusion.

PREREQUISITES
  • Understanding of quantum mechanics principles
  • Familiarity with wavefunction antisymmetrization
  • Knowledge of fermions and their behavior at different temperatures
  • Basic concepts of atomic structure and electron configurations
NEXT STEPS
  • Explore the implications of wavefunction antisymmetrization in quantum systems
  • Study the behavior of fermions at varying temperatures and their impact on matter
  • Investigate the role of quantum coherence in electron interactions
  • Learn about the transition from white dwarfs to stars and the effects of temperature on electron states
USEFUL FOR

Physicists, chemists, and students of quantum mechanics seeking to deepen their understanding of the Pauli Exclusion Principle and its applications in various physical systems.

john t
Messages
33
Reaction score
3
Over what range is the Pauli Exclusion Principle important? As a chemist I take it as an atom, but that seems an arbitrary stipulation. For instance, in metals how far apart must 2 electrons be to have the same 4 quantum numbers? I have seen that it has to do more with quantum coherence field than a certain space range. What determines the extent of the quantum coherence?

John Thompson
 
  • Like
Likes   Reactions: Mileto Graziano
Physics news on Phys.org
john t said:
Over what range is the Pauli Exclusion Principle important?

Forever. You always have to antisymmetrize the wavefunction. Whether or not that makes a noticeable difference to anything you observe depends on how much you can notice.
 
Pauli exclusion is important in any matter that has radiated down to its ground state (such that there aren't many more transitions left to happen, if any.) These systems include:
  • Blocks of metal, whose electrons occupy something fairly close to one giant pile of degeneracy.
  • Atoms, like you mentioned.
  • White dwarfs.
In all of these cases, the system has lost enough energy that it is not predominately the motion of the material that keeps it from collapsing. (A gas, I think, would be mainly held up by motion and not by quantum effects; PV=nRT comes from the mechanics of the atoms bouncing around.)

All fermions will end up in situations where exclusion is important if you cool them down enough. If you heat them up enough, they fly up into the high states and populate them so sparsely that exclusion stops being important. Examples of those things would be turning metal into plasma, ionizing electrons away from atoms, and going from white dwarfs to living stars which are kept very hot by fusion.
 
  • Like
Likes   Reactions: Imager and Mileto Graziano

Similar threads

  • · Replies 5 ·
Replies
5
Views
1K
  • · Replies 17 ·
Replies
17
Views
3K
  • · Replies 15 ·
Replies
15
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K