Schwartz's Quantum field theory (12.9)

In summary, Schwartz's Quantum Field Theory (12.9) provides a comprehensive framework for understanding quantum fields and their interactions. It covers key concepts such as the quantization of fields, the role of symmetries, and the formulation of scattering theory. The text emphasizes rigorous mathematical foundations, including the use of operator algebras and perturbative techniques, to describe particle dynamics and the underlying principles of quantum mechanics. It also addresses advanced topics like renormalization and the implications of relativistic invariance in field theory.
  • #1
Plantation
14
1
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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  • #2
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
$$\langle \Omega |[\hat{a}(\vec{p},s), \hat{a}^{\dagger}(\vec{p}',s')]|\Omega = \langle \Omega |\hat{a}(\vec{p},s) \hat{a}^{\dagger}(\vec{p}',s') \Omega= \frac{1}{\sqrt{2 \omega_{\vec{p}}}} \frac{1}{\sqrt{2 \omega_{\vec{p}'}}} 2 \omega_{\vec{p}} (2 \pi)^3 \delta^{(3)}(\vec{p}-\vec{p}') \delta_{ss'}=(2 \pi)^3 \delta^{(3)}(\vec{p}-\vec{p}') \delta_{ss'}.$$
 
  • #3
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?) ?
 
  • #4
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}##.
 
  • #5
Ah, the confusion one gets when implicitly implying Dieac delta's and then forgetting about them :P
 
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FAQ: Schwartz's Quantum field theory (12.9)

What is the main focus of Schwartz's Quantum Field Theory Chapter 12.9?

Schwartz's Quantum Field Theory Chapter 12.9 primarily focuses on the renormalization group and the concept of running couplings. It delves into how coupling constants change with energy scales and the implications for quantum field theory calculations.

How does Schwartz explain the concept of running couplings in Chapter 12.9?

Schwartz explains running couplings by discussing how physical parameters, such as coupling constants, are not fixed but vary with the energy scale at which they are measured. This is described using the renormalization group equations, which show how these parameters evolve with energy.

What mathematical tools are introduced in Chapter 12.9 for understanding the renormalization group?

Chapter 12.9 introduces several mathematical tools, including differential equations and beta functions, which describe how the coupling constants change with the energy scale. These tools are essential for performing calculations in quantum field theory and understanding the behavior of physical systems at different scales.

Why is the concept of the renormalization group important in quantum field theory?

The renormalization group is important because it provides a systematic way to handle infinities that arise in quantum field theory calculations. It allows physicists to understand how physical quantities change with energy and leads to more accurate predictions about the behavior of particles and fields at different scales.

Can you provide an example of a physical phenomenon that is explained using the concepts from Chapter 12.9?

An example of a physical phenomenon explained using the concepts from Chapter 12.9 is asymptotic freedom in quantum chromodynamics (QCD). This phenomenon describes how the strong force between quarks becomes weaker at higher energy scales, which can be understood by studying the running of the QCD coupling constant using the renormalization group equations.

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