Graduate Getting particle/antiparticle solutions from the Dirac Equation

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SUMMARY

The discussion focuses on deriving particle and antiparticle solutions from the Dirac Equation, specifically using Griffiths and Srednicki's approaches. The key equations discussed include the factorization of the Dirac operator and the introduction of solutions in the form of wave functions, represented as \( \varphi(x) = u(\mathbf{p}) e^{ipx} + v(\mathbf{p}) e^{-ipx} \). The participants clarify the derivation of equation (37.28) from (37.23) and emphasize the importance of linear independence of the exponential terms in the solutions. The derivation concludes with the conditions \( (\not\!p + m)u(\mathbf{p}) = 0 \) and \( (-\not\!p + m)v(\mathbf{p}) = 0 \).

PREREQUISITES
  • Understanding of the Dirac Equation and its significance in quantum mechanics.
  • Familiarity with gamma matrices and their role in relativistic wave equations.
  • Knowledge of the Klein-Gordon equation and its implications for wave functions.
  • Basic proficiency in quantum field theory concepts, particularly particle-antiparticle solutions.
NEXT STEPS
  • Study Griffiths' "Introduction to Quantum Mechanics" for a detailed derivation of the Dirac Equation.
  • Explore Srednicki's "Quantum Field Theory" to understand the conventions used in particle physics.
  • Learn about the implications of linear independence in quantum mechanics, particularly in wave function solutions.
  • Investigate the role of the Klein-Gordon equation in deriving solutions for relativistic particles.
USEFUL FOR

Physicists, graduate students in quantum mechanics, and researchers interested in quantum field theory and the mathematical foundations of particle physics.

peguerosdc
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TL;DR
How to motivate positive and negative energy solutions as a superposition of two solutions?
Hi!

I am studying Dirac's equation and I already have understood the derivation. Following Griffiths, from factoring Einstein's energy relation with the gamma matrices:

##
(\gamma^\mu p_\mu + m)(\gamma^\mu p_\mu - m) = 0
##

You take any of the two factors, apply quantization and you arrive to Dirac's equation. Griffiths takes for example the second one:

##
(\gamma^\mu p_\mu - m) \varphi = 0
##

Comparing this with Srednicki's, they look the same just that he renames ## \gamma^\mu p_\mu = i\not\!\partial ##, inverts signs and arrives to this expression for Dirac's equation (equation 37.23):

##
(-i\not\!\partial + m) \varphi = 0
##

Now, Srednicki motivates finding two solutions (one with +E and one with -E) by showing that the wave function must obey the Klein-Gordon equation, so he proposes the solution as (eq 37.27):

##
\varphi (x) = u(\mathbf p) e^{ipx} + v(\mathbf p) e^{-ipx}
##

where u is the positive energy solution and v the negative energy solution.

So far, so good. Now, where I need help is understanding the next step. He says:
Plugging eq. (37.27) into the eq. (37.23) we get eq (37.28):
$$
(\not\!p + m)u(\mathbf p) e^{ipx} + (-\not\!p + m)v(\mathbf p) e^{-ipx} = 0
$$
Thus we require (37.29):
$$
(\not\! p + m)u(\mathbf p) = 0
\qquad
(-\not\!p + m)v(\mathbf p) = 0
$$
I don't understand why plugging eq. 37.27 into 37.23 yields equation 37.28. It looks like we are taking one different factor for each solution (that's why I introduced my question with Griffiths' derivation), but I don't understand the reasoning behind it.

Thanks!
 
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I do not go into detail but the formula seems to say ##e^{ipx}## and ##e^{-ipx}## are linear independent.
 
anuttarasammyak said:
I do not go into detail but the formula seems to say ##e^{ipx}## and ##e^{-ipx}## are linear independent.
Thanks for the reply! Yes, I think that's why 37.28 implies 37.29, but my question is more how to get to equation 37.28.
Following Srednicki, if you just plug 37.27 into 37.23, you get:

$$
\begin{align*}
(-\not\!p + m) ( u(\mathbf p) e^{ipx} + v(\mathbf p) e^{-ipx} ) &= 0 \\
(-\not\!p + m)u(\mathbf p) e^{ipx} + (-\not\!p + m)v(\mathbf p) e^{-ipx} &= 0
\end{align*}
$$

Which doesn't look like 37.28 as some signs are wrong. I was thinking about plugging 37.27 into the first equation in my post to get something like:
$$
\begin{align*}
(\not\!p + m)(\not\!p - m) \varphi &= 0 \\
(\not\!p + m)(\not\!p - m)u(\mathbf p) e^{ipx} + (\not\!p + m)(\not\!p - m)v(\mathbf p) e^{-ipx} &= 0
\end{align*}
$$
But then I don't know how I could get 37.28 from that.
 
peguerosdc said:
Thanks for the reply! Yes, I think that's why 37.28 implies 37.29, but my question is more how to get to equation 37.28.
Following Srednicki, if you just plug 37.27 into 37.23, you get:

$$
\begin{align*}
(-\not\!p + m) ( u(\mathbf p) e^{ipx} + v(\mathbf p) e^{-ipx} ) &= 0 \\
(-\not\!p + m)u(\mathbf p) e^{ipx} + (-\not\!p + m)v(\mathbf p) e^{-ipx} &= 0
\end{align*}
$$

Which doesn't look like 37.28 as some signs are wrong. I was thinking about plugging 37.27 into the first equation in my post to get something like:
$$
\begin{align*}
(\not\!p + m)(\not\!p - m) \varphi &= 0 \\
(\not\!p + m)(\not\!p - m)u(\mathbf p) e^{ipx} + (\not\!p + m)(\not\!p - m)v(\mathbf p) e^{-ipx} &= 0
\end{align*}
$$
But then I don't know how I could get 37.28 from that.
As per the book, you must get a different factor when you differentiate ##e^{ipx}## and ##e^{-ipx}##. One must have a factor of ##-1## compared to the other.
 
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PeroK said:
As per the book, you must get a different factor when you differentiate ##e^{ipx}## and ##e^{-ipx}##. One must have a factor of ##-1## compared to the other.
Oh, right! I knew this was most likely a dumb question. Thanks!
 
peguerosdc said:
Oh, right! I knew this was most likely a dumb question. Thanks!
Let's look at this anyway. We are looking for ##\varphi(x)## to satisfy:
$$(-i \not\!\partial + m)\varphi(x) = (-i \gamma^{\mu}\partial_{\mu}+m)\varphi(x) = (-i \gamma^{\mu}\frac{\partial}{\partial x^{\mu}}+m)\varphi(x) = 0$$ where
$$\varphi(x) = u(p)e^{ipx} + v(p)^{-ipx} = u(p)e^{ip_{\nu}x^{\nu}} + v(p)e^{-ip_{\nu}x^{\nu}}$$
Note that this is a different convention from Griffiths with ##u(p)## for antiparticles. In any case:
$$\frac{\partial}{\partial x^{\mu}}e^{ip_{\nu}x^{\nu}} = ip_{\mu}e^{ip_{\nu}x^{\nu}}= ip_{\mu}e^{ipx} \ \ \text{and} \ \ \frac{\partial}{\partial x^{\mu}}e^{-ip_{\nu}x^{\nu}} = -ip_{\mu}e^{-ip_{\nu}x^{\nu}} = -ip_{\mu}e^{-ipx}$$
So that:
$$(-i \not\!\partial + m)\varphi(x) = -i\gamma^{\mu}u(p) (ip_{\mu}e^{ipx}) -i\gamma^{\mu}v(p)(-ip_{\mu}e^{-ipx}) + mu(p)e^{ipx} + mv(p)e^{-ipx}$$ $$ = (\gamma^{\mu}p_{\mu}+ m)u(p)e^{ipx} + (-\gamma^{\mu}p_{\mu}+ m)v(p)e^{-ipx}$$
Setting this to zero and using the linear independence of ##e^{ipx}, e^{-ipx}## gives:
$$(\gamma^{\mu}p_{\mu}+ m)u(p) = 0 \ \ \text{and} \ \ (-\gamma^{\mu}p_{\mu}+ m)v(p) = 0$$
 
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PeroK said:
Note that this is a different convention from Griffiths with ##u(p)## for antiparticles.
Yeah, I almost missed that and actually I think that's the convention followed in every book, so it's worth noting it for future readers that check this thread.

Thank you for showing the full derivation! Definitely helpful.
 
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