Is there an alternative form of the zero point energy?

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Discussion Overview

The discussion revolves around the concept of zero point energy, particularly in the context of free electrons and the challenges of defining it without a quantized space interval (L). Participants explore alternative formulations, renormalization techniques, and implications of including or excluding gravity in these considerations.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants question whether a ground state energy for free electrons can be proposed without a defined interval L.
  • There is a suggestion that taking limits of the non-alternative form of zero point energy might not be problematic.
  • One participant argues that using a different basis for wavefunctions will ultimately lead to the standard zero point energy formula, though renormalization may allow for the addition of a constant.
  • Concerns are raised about the implications of setting the eigenenergy to zero, with one participant suggesting it may lead to unrealistic initial conditions.
  • Participants discuss the role of gravity in setting the zero point energy, indicating that it may need to align with the cosmological constant if gravity is included.
  • There is mention of the Quantum Hall effect and its relation to zero point energy, with questions about how cosmological constants might affect it.
  • Some participants reflect on the vacuum state in quantum field theory (QFT) and its complexities, particularly regarding initial conditions for wavefunction studies.
  • Questions arise about the nature of annihilation operators and their effect on average values in quantum states.

Areas of Agreement / Disagreement

Participants express a range of views on the formulation and implications of zero point energy, with no consensus reached on the alternative forms or the necessity of interval L. The discussion remains unresolved with multiple competing perspectives presented.

Contextual Notes

Limitations include the dependence on the definitions of zero point energy and the interval L, as well as the unresolved implications of including gravity in the discussion.

Who May Find This Useful

Researchers and students interested in quantum mechanics, quantum field theory, and the implications of zero point energy in various physical contexts may find this discussion relevant.

SeM
Hi, is there an alternative form of the zero point energy for free electrons, where there is no space interval L to be quantized in? The zero point energy for electrons in an atom can be simplified to a variant where Z^2 is present in the nominator, however, these are not free electrons.

Can a ground state energy for a free electron be proposed at all without L?
 
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Is taking the limit(s) of the non-alternative form such a bad idea ?
 
I don't think so... You can try using a different basis for the wavefunctions, but the zero point energy will end being equivalent to the standard formula... You can renormalize it adding a constant that has the same kind of divergence, and it won't mess up anything more on your theory, so... It's a good thing to do.

It's ok my answer?
 
Iliody said:
I don't think so... You can try using a different basis for the wavefunctions, but the zero point energy will end being equivalent to the standard formula... You can renormalize it adding a constant that has the same kind of divergence, and it won't mess up anything more on your theory, so... It's a good thing to do.

It's ok my answer?
Hi, renormalizing is a necessity, but the problem is the interval L. For an electron traveling freely, that interval is pretty much infinity? Even worse, if that electron is oscillating in an area which is unknown for its dimensions, then how can one treat L? As a parameter?
 
BvU said:
Is taking the limit(s) of the non-alternative form such a bad idea ?
Not sure what you mean. Do you mean the limits of E_0 as L goes for from 0 to infinity?
 
SeM said:
...the problem is the interval L. For an electron traveling freely, that interval is pretty much infinity? ... oscillating in an area which is unknown for its dimensions, then how can one treat L?

You regularize first, restricting the base of first-quantized wavefunctions with which you make the base of second-quantized wavefunctions, being them normalized, then you diagonalize your Hamiltonian (plus a renormalizing constant that depends on the regularization), and then you look for the lower eigenval. That eigenval is the zero energy, and (my opinion) you can set it to zero by renormalization (when there are no symmetries in tour theory forbiding it).
Good look!

Pd: I am not sure about how common is that this is opinion is shared in the physics comunity, so it's maybe wrong that I put this answer here.
 
Iliody said:
You regularize first, restricting the base of first-quantized wavefunctions with which you make the base of second-quantized wavefunctions, being them normalized, then you diagonalize your Hamiltonian (plus a renormalizing constant that depends on the regularization), and then you look for the lower eigenval. That eigenval is the zero energy, and (my opinion) you can set it to zero by renormalization (when there are no symmetries in tour theory forbiding it).
Good look!

Pd: I am not sure about how common is that this is opinion is shared in the physics comunity, so it's maybe wrong that I put this answer here.
Thanks , I think setting the eigenenergy to zero gives a somewhat unrealistic initial condition. However, I would like to thank you for your comments in any case!
 
If de don't include gravity in our discussion, it's ok to ser it to any value, if you include gravity, you need to set it to the cosmological constant. I never did perturbative QG calculations (they can be done to one loop if we don't put matter loop corrections in gravity-gravity scattering), so I don't know how many quantities depende on the cosmo-constant.
 
Iliody said:
If de don't include gravity in our discussion, it's ok to ser it to any value, if you include gravity, you need to set it to the cosmological constant. I never did perturbative QG calculations (they can be done to one loop if we don't put matter loop corrections in gravity-gravity scattering), so I don't know how many quantities depende on the cosmo-constant.
This is a particle in a Quantum Hall. cosmological constants- would they affect it? Which cosmological constant do you mean?
 
  • #10
SeM said:
This is a particle in a Quantum Hall.
Sorry, I thinked that you were talking about other kind of system. I don't remember anything about Quantum Hall... And I remembered now that my affirmations were limited to QFT correlation functions without boundaries (infinite volume limit). There are observables like presure that depend on the zero point energy in a nontrivial way (even in that case, the thing that I said about zero energy renormalization-regularization).
 
  • #11
Iliody said:
Sorry, I thinked that you were talking about other kind of system. I don't remember anything about Quantum Hall... And I remembered now that my affirmations were limited to QFT correlation functions without boundaries (infinite volume limit). There are observables like presure that depend on the zero point energy in a nontrivial way (even in that case, the thing that I said about zero energy renormalization-regularization).
Hi, QFT may have indeed some important common themes with the Quantum Hall. However, is there a "starting" point, or some initial condition one uses in QFT for wavefunction study?

Cheers
 
  • #12
SeM said:
Is there a "starting" point, or some initial condition one uses in QFT for wavefunction study?

Mmm... It's usually taken a vacuum state at the infinite past & at the infinite future, and you change that state inserting operators add particle exitations (first-quantized non-interacting wavefunctions) of the different fields. That has a lot of troubles, in some sense.
 
  • #13
Iliody said:
Mmm... It's usually taken a vacuum state at the infinite past & at the infinite future, and you change that state inserting operators add particle exitations (first-quantized non-interacting wavefunctions) of the different fields. That has a lot of troubles, in some sense.
how does this vacuum state look like in terms of function/value/expression?
 
  • #14
SeM said:
how does this vacuum state look like in terms of function/value/expression?
It's the state annihilated by all field anihillation operators, that are Fourier modes of the field operators.
 
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  • #15
Thanks! How do the annihilation operators prevent an infinitesimal value of the averages? Do they converge to some minimal value?
 

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