What Happens When Two Up-Up Fermions Collide?

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Discussion Overview

The discussion revolves around the implications of colliding two up-up fermions, particularly in the context of quantum mechanics and the Pauli exclusion principle. Participants explore the nature of Pauli repulsion and its potential measurability, as well as the practical outcomes of such collisions in particle accelerators and astrophysical contexts.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Valleyman questions what happens when two up-up fermions collide, noting the implications of the Pauli exclusion principle and the concept of Pauli repulsion force.
  • One participant suggests that the interpretation of quantum mechanics affects the understanding of Pauli repulsion, proposing that if the wave function is seen as a real field, then the repulsion is a real force.
  • Another participant argues that if the wave function represents knowledge or information, then Pauli repulsion may not be considered a real force.
  • A participant mentions that in neutron stars, Pauli repulsion prevents collapse, but in larger stars, gravitational forces can overcome this repulsion, leading to black hole formation.
  • It is noted that the symmetric spin state of fermions results in an antisymmetric spatial wavefunction, which keeps the particles farther apart, but does not constitute a force.
  • One participant claims that collisions of fermions occur in particle accelerators, suggesting that sufficient energy can lead to interactions that release energy, similar to processes in black holes.

Areas of Agreement / Disagreement

Participants express differing views on the nature of Pauli repulsion and its status as a measurable force. There is no consensus on whether it is a real force or an emergent property, and the discussion remains unresolved regarding the implications of these collisions.

Contextual Notes

Participants reference different interpretations of quantum mechanics and the implications for understanding forces in particle physics. The discussion includes assumptions about the nature of wave functions and the conditions under which fermions interact.

valleyman
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This morning I've been thinking about a simple problem whose I can't find out a satisfying solution. We all know that two "close" fermions can't exist in a up-up or down-down spin configuration because of vanishing state function as expressed by the exclusion principle.
But what does *practically* happen when I try to collide two up-up fermions, maybe with an accelerator? I've encountered several times the vague concept of a "Pauli repulsion force" in studies about atomic structure but is it a misurable force - i.e. real - or just an emergent property of the system itself? Or am I missing something obvious?

Thanks in advance,
Valleyman
 
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valleyman said:
This morning I've been thinking about a simple problem whose I can't find out a satisfying solution. We all know that two "close" fermions can't exist in a up-up or down-down spin configuration because of vanishing state function as expressed by the exclusion principle.
But what does *practically* happen when I try to collide two up-up fermions, maybe with an accelerator? I've encountered several times the vague concept of a "Pauli repulsion force" in studies about atomic structure but is it a misurable force - i.e. real - or just an emergent property of the system itself? Or am I missing something obvious?

Thanks in advance,
Valleyman


The answer to this depends on what interpretation of QM you subscribe to, in particular whether you believe that the wave function represents a real objectively existing wave field (as in de Broglie-Bohm theory). If you do think this, then that does generally imply that Pauli repulsion is a real force.

If you think that the wave function represents 'knowledge' or 'information', then - realizing that it is very difficult for knowledge to push things around - your answer would be 'Splutter. Don't be ridiculous. How dare you ask such a stupid question. Of course it isn't a real force. Pauli proved this mathematically with some terribly complicated bit of quantum field theory that your tiny brain can never understand.'

On the other hand, I found http://www.tcm.phy.cam.ac.uk/~mdt26/PWT/lectures/towler_pauli.pdf" quite useful in sorting out my thinking on this.
 
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i know that pulsars and neutron stars don't collapse because Pauli repulsion force but in bigger stars the gravitational force is stronger than Pauli repulsion force so the star collapses to forma a black hole so i guess its real. its what i know
 
alphali said:
i know that pulsars and neutron stars don't collapse because Pauli repulsion force but in bigger stars the gravitational force is stronger than Pauli repulsion force so the star collapses to forma a black hole so i guess its real. its what i know

Pauli repulsion force/degeneracy pressure in stars was discussed extensively in https://www.physicsforums.com/showthread.php?t=364464".
 
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But what does *practically* happen when I try to collide two up-up fermions, maybe with an accelerator?
All that happens is that since the spin part of the wavefunction is symmetric, then the space part must be antiysmmetric. So L=1, 3, ... This is not a "force", but does mean the particles remain farther apart.
 
i think it happens all the time in particle accelerators when they collide proton-proton beams.its like in the neutron star and black hole, if u have enough energy they will collide (in particle accelerator)and release energy and in case of a black hole the star is made of fermions and it collapses to form a black hole so all the particles are in one place but that only happens if the gravitational energy is enough to overcome exclusion principle.
 

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