P&S Chapter 2: Derivation of the KG Hamiltonian

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    Derivation Hamiltonian
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Discussion Overview

The discussion revolves around the derivation of the Hamiltonian for a real scalar field as presented in Peskin & Schröder. Participants explore the steps involved in arriving at the Hamiltonian expression, addressing potential errors and clarifying notation. The conversation includes technical calculations, conceptual clarifications, and challenges related to the derivation process.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant expresses uncertainty about their derivation of the Hamiltonian and seeks confirmation of their steps, specifically regarding the transition from one form of the Hamiltonian to another.
  • Another participant suggests splitting the integral into two parts and changing variables to simplify the calculation, indicating that this approach should yield the correct result.
  • Concerns are raised about the notation used in the exponential function and the implications of treating momentum as either 3-vectors or 4-vectors, which could affect the interpretation of the Hamiltonian.
  • A participant mentions the reality condition imposed on the field and how it leads to specific relationships between the operators, questioning the resulting Hamiltonian expression derived from these conditions.
  • There is a discussion about the significance of the term involving the commutation relation of the operators and how it affects the final form of the Hamiltonian.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the correctness of the derivation steps or the implications of the notation used. Multiple competing views and interpretations of the calculations and their significance remain present throughout the discussion.

Contextual Notes

Participants highlight the potential confusion arising from the notation and the assumptions made during the derivation process. There are unresolved questions regarding the treatment of the operators and the implications of the reality condition on the Hamiltonian.

hellfire
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I am not familiar with calculations such as the following one, and I want to be sure I do the right steps before going on with Peskin & Schröder. I want to derive step by step the Hamiltonian of the real scalar field. I have no problem to arrive at the first part of (2.31) in page 21:

H = \int dx^3 \int \frac {d^3p d^3p^{\prime}}{(2 \pi)^6} e^{i (p + p \prime) x} \left( - \frac{\sqrt{\omega_p \omega_{p \prime}}}{4} (a_{p} - a^{\dagger}_{-p}) (a_{p \prime} - a^{\dagger}_{-p \prime}) + \frac{-p p^{\prime} + m^2}{4 \sqrt{\omega_p \omega_{p \prime} }} (a_{p} + a^{\dagger}_{-p}) (a_{p \prime} + a^{\dagger}_{-p \prime}) \right)

This shall be equal to:

H = \int \frac{d^3p}{(2 \pi)^3} \omega_p \left(a^{\dagger}_{p} a_p + \frac{1}{2}[a_p, a^{\dagger}_{p}] \right)

So, I figured out I can make use of:

\int dx^3 e^{i (p + p \prime) x} = (2 \pi)^3 \delta^{(3)} (p + p^{\prime})

and

\int \delta(p + p^{\prime}) F(p^{\prime}) dp^{\prime} = F(- p)

and I can set p\prime = - p and \omega_p = \omega_p^{\prime} considering that p^2 + m^2 = \omega^2_p, remove dp' and I arrive at:

H = \int \frac {d^3p}{(2 \pi)^3} \frac{\omega_p}{4}} \left(- a_p a_{-p} + a_p a^{\dagger}_{p} + a^{\dagger}_{-p} a_{-p} - a^{\dagger}_{-p} a^{\dagger}_{p} + a_p a_{-p} + a_p a^{\dagger}_{p} + a^{\dagger}_{-p} a_{-p} + a^{\dagger}_{-p} a^{\dagger}_{p} \right)

which simplifies to

H = \int \frac {d^3p}{(2 \pi)^3} \frac{\omega_p}{2}} \left(a_p a^{\dagger}_{p} + a^{\dagger}_{-p} a_{-p} \right)

This seams to lead to the required result if a_p = a_{-p}, but this is not the case, isn't it? So, I may have made some error. Comments are appreciated... (I hope I made no typo...)
 
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hellfire said:
which simplifies to

H = \int \frac {d^3p}{(2 \pi)^3} \frac{\omega_p}{2}} \left(a_p a^{\dagger}_{p} + a^{\dagger}_{-p} a_{-p} \right)

This seams to lead to the required result if a_p = a_{-p}, but this is not the case, isn't it? So, I may have made some error. Comments are appreciated... (I hope I made no typo...)

I didn't follow your calculation, but assuming you correctly got up here, I don't see the difficulty: split the integral of the sum into a sum of 2 integrals, and then change variables p => -p in the second term. Now put them together again and you're done, no ?

cheers,
Patrick.
 
hellfire said:
I am not familiar with calculations such as the following one, and I want to be sure I do the right steps before going on with Peskin & Schröder. I want to derive step by step the Hamiltonian of the real scalar field. I have no problem to arrive at the first part of (2.31) in page 21:

H = \int dx^3 \int \frac {d^3p d^3p^{\prime}}{(2 \pi)^6} e^{i (p + p \prime) x} \left( - \frac{\sqrt{\omega_p \omega_{p \prime}}}{4} (a_{p} - a^{\dagger}_{-p}) (a_{p \prime} - a^{\dagger}_{-p \prime}) + \frac{-p p^{\prime} + m^2}{4 \sqrt{\omega_p \omega_{p \prime} }} (a_{p} + a^{\dagger}_{-p}) (a_{p \prime} + a^{\dagger}_{-p \prime}) \right)

This shall be equal to:

H = \int \frac{d^3p}{(2 \pi)^3} \omega_p \left(a^{\dagger}_{p} a_p + \frac{1}{2}[a_p, a^{\dagger}_{p}] \right)

This is the Klein-Gordon Hamiltonian. The second term is the infinite background energy that you discard by convincing yourself that you can only measure energy differences and that this term doesn't contribute to that difference since it is present in both cases. Read the paragraph after this equation on page 21 continueing onto page 22.
Cheers
 
What i hated about this exercise,thing which made to stay away till now,is that the notation is pretty confusing.In the exponential:
e^{i(p+p')x}

is a tensor contraction of 2 3vectors or 2 4vectors.
What's the functional dependence of the operators a and a dagger...??That's the most annoying part.

Daniel.

P.S.What's the commutation relation between the operators (why is that (2pi)^{3} left in the final integral)...?There must be a weird scaling of the amplitudes.
 
vanesch said:
I didn't follow your calculation, but assuming you correctly got up here, I don't see the difficulty: split the integral of the sum into a sum of 2 integrals, and then change variables p => -p in the second term. Now put them together again and you're done, no ?
Yes, this would lead to the required result. Can I do that for only one of the integrals and then sum both?

(To clarify the notation: the p and p' are 3-vectors here).
 
ADVICE:Do both integrals and try to "catch" the trick.It's an useful exercise.Many more such integrals will be present...

Daniel.
 
hellfire said:
Yes, this would lead to the required result. Can I do that for only one of the integrals and then sum both?

(To clarify the notation: the p and p' are 3-vectors here).

Sure, why not ?

Try to calculate integral dx (f(x) + f(-x)) OVER ALL X.

You can write the first term as integral dx f(x) (duh!)
and the second one as integral dx f(-x) (duh2!)

In this second one, you do u = -x.
Because the integral is still over all x, this is: integral du f(u)
(you switched sign in du, and then inverted the integration limits again)

So now we have: integral dx f(x) + integral du f(u)

dummy change of variable in the last one u -> x:

integral dx 2 f(x)

Note that in YOUR problem there is something non-trivial:
that is that omega_p must be equal to omega_(-p)

But that's so because omega(p) = sqrt( p^2 + m^2)

cheers,
Patrick.
 
dextercioby said:
What i hated about this exercise,thing which made to stay away till now,is that the notation is pretty confusing.In the exponential:
e^{i(p+p')x}

If I remember well from P&S, all p-s here are 3-vectors, because we are still in the Schroedinger picture, so our hamiltonian is time-less.
The subtle part is indeed that you can keep exactly the same notation, but consider this time, p and x to be 4-vectors, and suddenly you're in the Heisenberg picture !

A long time ago I tried to capture this in a summary of chapter 2 of P&S:
http://perso.wanadoo.fr/patrick.vanesch/Summary_Chapter_2_PS.html

cheers,
Patrick
 
It is clear now, thank you!
 
  • #10
vanesch said:
Sure, why not ?

Try to calculate integral dx (f(x) + f(-x)) OVER ALL X.

You can write the first term as integral dx f(x) (duh!)
and the second one as integral dx f(-x) (duh2!)

In this second one, you do u = -x.
Because the integral is still over all x, this is: integral du f(u)
(you switched sign in du, and then inverted the integration limits again)

So now we have: integral dx f(x) + integral du f(u)

dummy change of variable in the last one u -> x:

integral dx 2 f(x)

Note that in YOUR problem there is something non-trivial:
that is that omega_p must be equal to omega_(-p)

But that's so because omega(p) = sqrt( p^2 + m^2)

cheers,
Patrick.

This is a old thread, but I think there is a better answer. P&S use the notation p, -p because it is usefull. If you make many changes of variables because of that, it become more complicated than the notation with only p, and you surely solve the problem in a way P&S would'nt.
In the following, I try another way to solve the problem, but it seems to give the bad result. I would like if you can help me with that.

Take \phi given by eq. (2.27), impose \phi^*(x)=\phi(x) (reality condition), and then we get easily the conditions a_{-p}=a_{p}^\dag and a_{-p}^\dag=a_{p}. Reporting this result in the last equation of the first post of hellfire, one find
H=\int \frac{d^{3}p}{\left( 2\pi \right) ^{3}}\omega _{\bf{p}}a_{\bf{p}}a_{\bf{p}}^{\dag }​

But this is not the good result, since we have
a_{\bf{p}}a_{\bf{p}}^\dag = [a_{\bf{p}},a_{\bf{p}}^\dag]+a_{\bf{p}}^\dag a_{\bf{p}}​
which give
H=\int \frac{d^{3}p}{\left( 2\pi \right) ^{3}}\omega _{\bf{p}}\left([a_{\bf{p}},a_{\bf{p}}^\dag]+a_{\bf{p}}^\dag a_{\bf{p}}\right)​

So, the result is similar, but without the 1/2 factor which should appear in the good result :

H=\int \frac{d^{3}p}{\left( 2\pi \right) ^{3}}\omega _{\bf{p}}\left(\frac{1}{2}[a_{\bf{p}},a_{\bf{p}}^\dag]+a_{\bf{p}}^\dag a_{\bf{p}}\right)​

Could someone help me to fix the problem in my calculation?

Thanks a lot,

Tipi
 
  • #11
Tipi said:
Take \phi given by eq. (2.27), impose \phi^*(x)=\phi(x) (reality condition), and then we get easily the conditions a_{-p}=a_{p}^\dag and a_{-p}^\dag=a_{p}.
Here is the calculation, since I found the problem in it.

We have (eq (2.27-28), p.21 of P&S)

$\phi \left( \bf{x}\right) =\int \frac{d^{3}p}{\left( 2\pi \right) ^{3}}e^{i\bf{p\cdot \bf{x}}}\phi \left( \bf{p}\right) $

$\pi \left( \bf{x}\right) =\int \frac{d^{3}p}{\left( 2\pi \right) ^{3}}e^{i\bf{p\cdot \bf{x}}}\pi \left( \bf{p}\right) $​

where

$\phi \left( \bf{p}\right) =\frac{1}{\sqrt{2\omega _{\bf{p}}}}\left( a_{\bf{p}}+a_{-\bf{p}}^{\dag }\right) \,\,\,\, (1)$

$\pi \left( \bf{p}\right) =-i\sqrt{\frac{\omega _{\bf{p}}}{2}}\left( a_{\bf{p}}-a_{-\bf{p}}^{\dag }\right)\,\,\,\,(2) $​

From (1), we have
a_{\bf{p}}=\sqrt{2\omega _{\bf{p}}}\phi \left( \bf{p}\right) -a_{-\bf{p}}^{\dag }\,\,\,\,(1')​

and from (2), we have
a_{-\bf{p}}^{\dag }=a_{\bf{p}}-i\sqrt{\frac{2}{\omega _{\bf{p}}}}\pi \left( \bf{p}\right)\,\,\,\,(2')​

The substitution of (2') in (1') gives
a_{\bf{p}}=\sqrt{\frac{\omega _{\bf{p}}}{2}}\phi \left( \bf{p}\right) +i\sqrt{\frac{1}{2\omega _{\bf{p}}}}\pi \left( \bf{p}\right)​

If \phi(x) and \pi(x) are real, then, we must have \phi^\dag(p)=\phi(-p) and \pi^\dag(p)=\pi(-p). So, we have

a_{\bf{p}}^{\dag }=\sqrt{\frac{\omega _{\bf{p}}}{2}}\phi \left( -\bf{p}\right) -i\sqrt{\frac{1}{2\omega _{\bf{p}}}}\pi \left( -\bf{p}\right)\,\,\,\,(*)​

and we DON'T HAVE a_{\bf{p}}^{\dag }=a_{-\bf{p}}. That was the mistakes. So it seems that the method proposed by Vanesh is better...

Sorry for that. It should be fine to find such an identity between the "a" operators... but so far I didn't find one. Damn ;)

Tipi
 
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