Klein-Gordon equation and factorization

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Discussion Overview

The discussion revolves around the factorization of the Klein-Gordon equation as it pertains to a Dirac field of a neutrino. Participants explore the implications of different orderings in the factorization and the resulting equations, particularly in the context of high relativistic limits and approximations of energy-momentum relations.

Discussion Character

  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant presents a derivation involving the Klein-Gordon equation and its factorization, questioning the implications of changing the order of factors.
  • Another participant asserts that the Klein-Gordon operator acting on a plane wave yields a result proportional to \( m^2 \), suggesting that the order of operations should not affect the outcome.
  • A different viewpoint suggests that if the mass is neglected in the high relativistic limit, the resulting equations become consistent, but confusion arises regarding the importance of operator order when mass is considered.
  • Participants discuss the appropriateness of approximating \( E \) as \( k \) and the implications of neglecting higher-order terms in the context of the derived equations.
  • One participant raises a concern about the validity of approximations when calculating differences, suggesting that the same reasoning may not apply uniformly across different operations.
  • There is a discussion about the correct decomposition of the d'Alembert operator and the criteria for choosing a specific factorization method.

Areas of Agreement / Disagreement

Participants express differing views on the significance of operator order in the factorization of the Klein-Gordon equation, with no consensus reached on the implications of these differences. The discussion remains unresolved regarding the best approach to factorization and the treatment of mass in the relativistic limit.

Contextual Notes

Participants note that the treatment of mass and the choice of approximations can lead to different equations, highlighting the need for careful consideration of assumptions in the derivation process.

parton
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Hi!

I read a text were some kind of "Schroedinger-equation" for a neutrino field is being derived. But there is a particular step I do not understand.

Consider a Dirac field \psi(t, \vec{x}) of a neutrino, satisfying the Klein-Gordon equation:
\left( \partial_{t}^{2} + \vec{k}^{2} + m^{2} \right) \psi_{\vec{k}}(t) = 0
where the field was expanded in plane waves \psi(t,\vec{x}) = \psi_{0} e^{i (\vec{k} \cdot \vec{x} - E \cdot t)} and the spatial derivatives were already computed.

Furthermore, we assume the high relativistic limes where k = \vert \vec{k} \vert \gg m

Now we can linearzie the equation above using
\partial_{t}^{2} + \vec{k}^{2} = (-i \partial_{t} + k) (i \partial_{t} + k)
Applying only the 2nd factor onto the field \psi(t,\vec{x})
will lead to
\left \lbrace (-\partial_{t} + k) (E + k) + m^{2} \right \rbrace \psi(t,\vec{x}) = 0

Now the following approximaton of the energy-momentum relation is used:
E = \sqrt{\vec{k}^{2} + m^{2}} \simeq k
If we use this approximation in the equation above, we have
\left \lbrace (-\partial_{t} + k) (2 k) + m^{2} \right \rbrace \psi(t,\vec{x}) = 0
which is actually the equation I need.

But my problem is, what happens if I exchange the order in the factorization above:

\partial_{t}^{2} + \vec{k}^{2} = (i \partial_{t} + k) (-i \partial_{t} + k)

Going through the same steps as above I end up with
\left \lbrace (\partial_{t} + k) (k - k) + m^{2} \right \rbrace \psi(t,\vec{x}) = 0
so finally I have
m^{2} \psi(t,\vec{x}) = 0
which does not make sense.

So my question is why is it possible to make the linarization
\partial_{t}^{2} + \vec{k}^{2} = (-i \partial_{t} + k) (i \partial_{t} + k)
and why do I have to pay attention to the order of the factors?

I hope somebody could help me.
 
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I didn't read carefully enough to spot where you made the mistake, but I'll tell you the answer; the Klein-Gordan operator acting on a plane wave returns m^2 times the plane wave, even in the relativistic limit. Therefore, no matter what order you do things, you should expect a cancellation between two big numbers (k^2 + m^2) and (-k^2) such that you get the small number m^2.
 
Thanks for your answer.
the Klein-Gordan operator acting on a plane wave returns m^2 times the plane wave, even in the relativistic limit.
I think you mean the d'Alembert operator (the Klein-Gordan operator applied on a free field should return 0).

The equation
m^{2} \psi(t,x) = 0
makes no sense. But I just recognized that if the relativistic limit corresponds to the massless limit, this equation would make sense if we set m=0.

And the other equation (if we exchange the order of the operators) would be
(-\partial_{t} + k) \psi(t,\vec{x}) = 0
So if the mass is vanishing in the high relativistic limit there is no contradiction anymore and the order of the operators does not matter.

But nevertheless I am confused. As long as I do not neglect the mass the order is important and depending on it, I find two different equations.

Maybe the "derivation" of the equation
\left \lbrace (-\partial_{t} + k) (2 k) + m^{2} \right \rbrace \psi(t,\vec{x}) = 0
should be considered as some kind of heuristic reasoning to find this "Schroedinger"-equation.
If we write it in the form
\partial_{t} \psi(t, \vec{x}) = \left( k + \dfrac{m^{2}}{2k} \right) \psi(t,\vec{x})
we see that the RHS is just the expansion of the energy in the relativistic limit:
E = \sqrt{k^{2} + m^{2}} \simeq k + \dfrac{m^{2}}{2k}
But this is confusing me, because above I used another approximation:
E \simeq k
So if originally E ~ k is used and therefore, higher order terms
\mathcal{O} \left(\dfrac{m^{2}}{2k} \right)
are neglected why are this higher order terms not neglected in the "Schroedinger" equation too?
 
Code:
Isn't the basic issue here that, whilst it may be reasonable to approximate k ≈ E when calculating the factor (E + k), doing this is much less so when calculating
(-i\partial_{t} + k) = (k - E)
For example, it is often reasonable to say that 1,000,000 + 1,000,001 ≈ 2,000,000, but much less so to suggest that 1,000,001 - 1,000,000 ≈ 0.

If, instead, we use the approximation
E - k \simeq \dfrac{m^{2}}{2k}
then the equation becomes
\left \lbrace (i\partial_{t} + k) (\dfrac{-m^{2}}{2k}) + m^{2} \right \rbrace \psi(t,\vec{x}) = 0
which (unless I've got something wrong here) reduces to
(-i\partial_{t} + k)\ \psi(t,\vec{x}) = 0
and doesn't really help here. Actually, I don't really see why the same result should follow regardless of which factor we decide to operate with on the wavefunction first.

(Also, haven't you left out an i that should be before the ∂t in some of your equations?)
 
(Also, haven't you left out an i that should be before the ∂t in some of your equations?)

Yes, you are right.

Actually, I don't really see why the same result should follow regardless of which factor we decide to operate with on the wavefunction first.

I am just confused by the decomposition
\partial_{t}^{2} + \vec{k}^{2} = (-i \partial_{t} + k) (i \partial_{t} + k)
If the order is important then how do I know how to decompose the d'Alembert operator in the right way?

How do I know that i should write
\partial_{t}^{2} + \vec{k}^{2} = (-i \partial_{t} + k) (i \partial_{t} + k)
and not
\partial_{t}^{2} + \vec{k}^{2} = (i \partial_{t} + k) (-i \partial_{t} + k)
?

Or should I argue that I am intersted in the "difference" between energy and momentum and therefore, need to consider
\partial_{t}^{2} + \vec{k}^{2} = (-i \partial_{t} + k) (i \partial_{t} + k)
 

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