Me not falling through the ground and Pauli's Exclusion Principle

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Discussion Overview

The discussion revolves around the reasons why individuals do not fall through the ground, specifically examining the roles of classical electrostatics and Pauli's Exclusion Principle (PEP). Participants explore both theoretical and conceptual aspects of this phenomenon, considering various states of matter such as solids and liquids.

Discussion Character

  • Conceptual clarification
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants suggest that classical electrostatic repulsion is sufficient to explain why individuals do not fall through the ground.
  • Others argue that Pauli's Exclusion Principle becomes relevant in high-density scenarios, such as neutron stars, where it helps prevent collapse due to gravitational forces.
  • A participant notes that while electrostatic repulsion is a good initial explanation, understanding molecular arrangements requires consideration of PEP.
  • Another participant challenges the assertion that PEP is only relevant at high densities, stating that exchange interactions are significant even in typical molecules and can influence the stability of matter.
  • One contribution references historical work by Dyson and Lenard, suggesting that PEP is crucial for the stability of solids, while also raising questions about the applicability of this principle to liquids.
  • A later reply emphasizes that the behavior of liquids, such as water, also involves interactions that prevent them from passing through solid objects.

Areas of Agreement / Disagreement

Participants express differing views on the necessity of Pauli's Exclusion Principle versus classical electrostatics, with no consensus reached on the primary explanation for the phenomenon. The discussion remains unresolved regarding the contexts in which each principle applies.

Contextual Notes

Some claims depend on specific definitions of stability and density, and the discussion includes unresolved questions about the interactions in different states of matter, such as solids versus liquids.

Swimmingly!
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I explained to myself that I don't fall through the ground due to electrons repelling. Using classical electrostatic repulsion.
Once in a while I hear it explained through Pauli's exclusion principle (PEP).

  • Do we need PEP to explain this, or is classical electrostatics enough?
 
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Classical electrostatics accounts for almost every feature of the interactions between macroscopic bodies. Occasionally, the interaction can be modeled with Van der Waals forces, http://en.wikipedia.org/wiki/Van_der_Waals_force#Van_der_Waals_forces_between_macroscopic_objects.

In order for the exclusion principle to be relevant, the object must be at an huge density. One such example is the neutron star, http://en.wikipedia.org/wiki/Neutron_star. There the intense gravitational interaction is balanced by an effective repulsion between nucleons that serves to prevent further collapse of the stellar core. For larger bodies of mass, even the PEP effect cannot prevent further collapse to a black hole.
 
Hi Swimmingly!
It depends on how far you want to go
electrostatic repulsion is a good answer, but eventually if you want to work out the details of how did molecules even get to setup into this kind of mesh, so as to get the full picture, then Pauli's exlusion principle would kick in.
 
fzero said:
In order for the exclusion principle to be relevant, the object must be at an huge density.
That is not true. In typical molecules, the energetic effect of the "exchange interaction" is only one order of magnitude less, and sometimes not even that much less, than the direct Coulomb repulsion. That can be seen from Hartree-Fock or Kohn-Sham calculations, where you get a direct number for this "exchange energy". While "one order of magnitude less" might sound small, those energy scales are *astronomical* on chemical scales, easily being 10000 times as large as typical energy differences you get in molecular reactions (and let's not even talk about conformations or intermolecular, or weak interactions, which are much smaller but still account for a great deal of everyday physics).

In short: Without taking the antisymmetry of the wave function properly into account (and thus accounting for exchange interactions), there is no way you would even get something remotely describing real matter in any sensible way.

So to OP: It's both, electrostatics and exchange. The latter is, however, not a real force, but a kind of fake interaction which can be used to describe the effects arising from combining the regular Coulomb interaction with antisymmetry constraints of Fermionic wave functions.
 
yes, in order for the electrostatic repulsion to be effective the ground must be a stable solid, and a major reason for that is the Pauli Exclusion Principle as deduced by Dyson and Lenard in 1967:

FJ Dyson and A Lenard: Stability of Matter, Parts I and II, J. Math. Phys., 8, 423-434 (1967)

the argument was subsequently improved, eg by Lieb in 1976, see section IV of http://www.pas.rochester.edu/~rajeev/phy246/lieb.pdf

and an updated paper available at Project Euclid:

The stability of Matter: from Atoms to Stars - Elliot Lieb 1990
 
Thank you all for the answer.

unusualname said:
yes, in order for the electrostatic repulsion to be effective the ground must be a stable solid, and a major reason for that is the Pauli Exclusion Principle as deduced by Dyson and Lenard in 1967:

Why must it be solid, I don't understand what context you're referring too?
My question applies to for example liquids too. Water doesn't run through my hand.
 
yeah, the reason water doesn't run through your hand is because it's a liquid, try running your hand through ice.
 

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