Schwartz's Quantum field theory (12.9)

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The discussion centers on a calculation from Schwartz's Quantum Field Theory regarding the commutation relations for identical particles, particularly bosons. The key point is the derivation of the equality involving creation operators, which leads to the conclusion that the commutators vanish for bosons, as expressed in equation (12.8). Participants express confusion over the normalization conventions used in the definitions of momentum-spin eigenstates and creation operators, questioning the validity of Schwartz's normalization. Clarifications indicate that the normalization is indeed consistent and serves to ensure Lorentz invariance, while also confirming that it suffices to evaluate the commutation relations for the vacuum state to establish the broader result. The discussion emphasizes the importance of understanding these conventions in quantum field theory calculations.
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Homework Statement
$$[a_{\vec{p_1} s_1 n}, a^{\dagger}_{\vec{p_2}s_2 n}]= (2 \pi)^3 \delta^{3}(\vec{p_1}-\vec{p_2}) \delta_{s_1, s_2} . $$
Relevant Equations
$$ \langle \vec{p_1} | \vec{p_2} \rangle = 2 \omega_1 ( 2\pi)^3 \delta^{3}(\vec{p_1}-\vec{p_2}) $$
I am reading the Schwartz's quantum field theory, p.207 and stuck at some calculation.

In the page, he states that for identical particles,

$$ | \cdots s_1 \vec{p_1}n \cdots s_2 \vec{p_2} n \rangle = \alpha | \cdots s_2 \vec{p_2}n \cdots s_1 \vec{p_1}n \cdots \rangle, \tag{12.5}$$

where ##\alpha = e^{i\phi}## for some real ##\phi##.

From this, he argues that for boson case we obtain

$$a^{\dagger}_{\vec{p_1} s_1 n} a^{\dagger}_{\vec{p_2}s_2 n} | \psi \rangle = a^{\dagger}_{\vec{p_2}s_2 n} a^{\dagger}_{\vec{p_1} s_1 n} | \psi \rangle \tag{12.7}$$ for all ##|\psi\rangle## (I don't know why this is true from (12.5)) so that

$$ [a^{\dagger}_{\vec{p_1} s_1 n}, a^{\dagger}_{\vec{p_2}s_2 n}] = [a_{\vec{p_1} s_1 n}, a_{\vec{p_2}s_2 n}] =0 \tag{12.8}$$

And he saids that since ## \langle \vec{p_1} | \vec{p_2} \rangle = 2 \omega_1 ( 2\pi)^3 \delta^{3}(\vec{p_1}-\vec{p_2}) ##, we can use same argument to show that

$$[a_{\vec{p_1} s_1 n}, a^{\dagger}_{\vec{p_2}s_2 n}]= (2 \pi)^3 \delta^{3}(\vec{p_1}-\vec{p_2}) \delta_{s_1, s_2} . \tag{12.9} $$

Q. And why this is true? How can we use the formula for ##\langle \vec{p_1} | \vec{p_2} \rangle## ? What should I catch?
 
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He has a somewhat confusing normalization convention (in fact almost any author uses another more or less confusing convention; at the end it doesn't matter). He defines the momentum-spin eigenstates as normalized as
$$\langle \vec{p},s |\vec{p}',s' \rangle=(2 \pi)^3 \delta^{(3)} 2 \omega_{\vec{p}} (\vec{p}-\vec{p}') \delta_{s s'}$$
and the corresponding creation operator by
$$\hat{a}^{\dagger}(\vec{p},s) |\Omega \rangle=\frac{1}{\sqrt{2 \omega_{\vec{p}}}} |\vec{p},\vec{s} \rangle.$$
Adjoining this gives
$$\langle \Omega|\hat{a}(\vec{p},s) = \frac{1}{\sqrt{2 \omega_{\vec{p}}}} \langle \vec{p},s|.$$
From this you get for bosons
$$\langle \Omega |[\hat{a}(\vec{p},s), \hat{a}^{\dagger}(\vec{p}',s')]|\Omega = \langle \Omega |\hat{a}(\vec{p},s) \hat{a}^{\dagger}(\vec{p}',s') \Omega= \frac{1}{\sqrt{2 \omega_{\vec{p}}}} \frac{1}{\sqrt{2 \omega_{\vec{p}'}}} 2 \omega_{\vec{p}} (2 \pi)^3 \delta^{(3)}(\vec{p}-\vec{p}') \delta_{ss'}=(2 \pi)^3 \delta^{(3)}(\vec{p}-\vec{p}') \delta_{ss'}.$$
 
vanhees71 said:
He has a somewhat confusing normalization convention (in fact almost any author uses another more or less confusing convention; at the end it doesn't matter). He defines the momentum-spin eigenstates as normalized as
$$\langle \vec{p},s |\vec{p}',s' \rangle=(2 \pi)^3 2 \omega_{\vec{p}} \delta^{(3)} (\vec{p}-\vec{p}') \delta_{s s'}$$
and the corresponding creation operator by
$$\hat{a}^{\dagger}(\vec{p},s) |\Omega \rangle=\frac{1}{\sqrt{2 \omega_{\vec{p}}}} |\vec{p},\vec{s} \rangle.$$
Adjoining this gives
$$\langle \Omega|\hat{a}(\vec{p},s) = \frac{1}{\sqrt{2 \omega_{\vec{p}}}} \langle \vec{p},s|.$$
From this you get for bosons
$$\langle \Omega |[\hat{a}(\vec{p},s), \hat{a}^{\dagger}(\vec{p}',s')]|\Omega \rangle = \langle \Omega |\hat{a}(\vec{p},s) \hat{a}^{\dagger}(\vec{p}',s') | \Omega \rangle= \frac{1}{\sqrt{2 \omega_{\vec{p}}}} \frac{1}{\sqrt{2 \omega_{\vec{p}'}}} 2 \omega_{\vec{p}} (2 \pi)^3 \delta^{(3)}(\vec{p}-\vec{p}') \delta_{ss'}=(2 \pi)^3 \delta^{(3)}(\vec{p}-\vec{p}') \delta_{ss'}.$$

Thanks.

Question 1 : Why the final equality is true? ; i.e., why ##\frac{1}{\sqrt{2 \omega_{\vec{p}}}} \frac{1}{\sqrt{2 \omega_{\vec{p}'}}} 2 \omega_{\vec{p}} =1 ## ? Perhaps,

$$\langle \vec{p},s |\vec{p}',s' \rangle=(2 \pi)^3 2 \sqrt{\omega_{\vec{p}}} \sqrt{\omega_{\vec{p'}}} \delta^{(3)} (\vec{p}-\vec{p}') \delta_{s s'}$$

is more correct normalization condition ? ; i.e., the author (Schwartz) made mistake ?

Question 2 : Is it really enough to show only $$\langle \Omega |[\hat{a}(\vec{p},s), \hat{a}^{\dagger}(\vec{p}',s')]|\Omega \rangle = (2 \pi)^3 \delta^{(3)}(\vec{p}-\vec{p}') \delta_{ss'} $$ to show the (12.9) : $$[a_{\vec{p_1} s_1 n}, a^{\dagger}_{\vec{p_2}s_2 n}]= (2 \pi)^3 \delta^{3}(\vec{p_1}-\vec{p_2}) \delta_{s_1, s_2} . $$ in my question, without having to show the statement for all ##|\psi\rangle## instead of ##\Omega## (ground state?) ?
 
Ad 1: It's together with the ##\delta## distribution, because ##\delta^{(3)}(\vec{p}-\vec{p}')=0## for ##\vec{p} \neq \vec{p}'##. The final result indeed is
$$\langle \vec{p},s|\vec{p}',s' \rangle=(2 \pi)^3 2 \omega_{\vec{p}} \delta^{(3)}(\vec{p}-\vec{p}') \delta_{ss'}.$$
The advantage of this normalization convention is that this scalar product between momentum-spin eigenstates gives a Lorentz scalar.

Ad 2: It's enough, because from the canonical equal-time commutation relations, which you postulate, e.g., in the canonical-quantization argument of field quantization, it's clear that ##[\hat{a}_{\vec{p}_1 s_2 n},\hat{a}_{\vec{p}_2 s_2 n}] \propto \hat{1}##.
 
Ah, the confusion one gets when implicitly implying Dieac delta's and then forgetting about them :P
 
I want to find the solution to the integral ##\theta = \int_0^{\theta}\frac{du}{\sqrt{(c-u^2 +2u^3)}}## I can see that ##\frac{d^2u}{d\theta^2} = A +Bu+Cu^2## is a Weierstrass elliptic function, which can be generated from ##\Large(\normalsize\frac{du}{d\theta}\Large)\normalsize^2 = c-u^2 +2u^3## (A = 0, B=-1, C=3) So does this make my integral an elliptic integral? I haven't been able to find a table of integrals anywhere which contains an integral of this form so I'm a bit stuck. TerryW

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