Understanding the Math behind meson decay computations

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Discussion Overview

The discussion revolves around the computation of the meson-decay amplitude as presented in Tong's notes. Participants are exploring the mathematical details involved in the decay process, specifically focusing on the justification for certain terms vanishing in the amplitude calculation. The scope includes theoretical aspects of quantum field theory and the application of Dyson's formula.

Discussion Character

  • Homework-related
  • Mathematical reasoning
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Participants are examining the expression for the meson-decay amplitude, specifically the term involving the annihilation operator and its overlap with the final state.
  • One participant questions why the term involving ##a_{\vec k} e^{ipx}## vanishes, referencing Tong's justification of 'zero overlap' with the final state.
  • Another participant clarifies that 'no overlap' means the inner product between the states is zero, leading to the conclusion that certain terms do not contribute to the amplitude.
  • There is a discussion about the necessity of annihilation operators to match the number of creation operators for a non-zero result in the amplitude calculation.
  • Participants express uncertainty about the mathematical justification for why specific terms vanish and seek hints or guidance to understand the reasoning better.

Areas of Agreement / Disagreement

Participants generally agree on the mathematical framework being used but express differing levels of understanding regarding specific terms and their contributions to the amplitude. The discussion remains unresolved regarding the complete justification of why certain terms vanish.

Contextual Notes

Participants are working with specific equations and operators from quantum field theory, and there are references to commutation relations that may be relevant to the discussion but are not fully explored. The discussion reflects a process of clarification and refinement of understanding rather than a definitive conclusion.

Who May Find This Useful

This discussion may be useful for students and researchers interested in quantum field theory, particularly those studying meson decay processes and the mathematical techniques involved in calculating decay amplitudes.

JD_PM
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Homework Statement:: I am studying how to compute the meson-decay amplitude worked out in Tong's notes (pages 55 and 56; I attached the PDF).
Relevant Equations:: $$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \phi (x) |i>$$

The initial and final states are given by

$$|i > = \sqrt{2 E_{\vec p}} a_{\vec p}^{\dagger} |0>$$

$$|f > = \sqrt{4 E_{\vec q_1}E_{\vec q_2}} b_{\vec q_1}^{\dagger}c_{\vec q_2}^{\dagger} |0>$$

Using Dyson formula's expansion we get that

$$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \phi (x) |i>$$

We first expand out ##\phi \sim a + a^{\dagger}## using the following formula

Captura de pantalla (1021).png

Doing so we get

$$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} a_{\vec k} a_{\vec p}^{\dagger} e^{-ikx} |0> = -ig<f|\int d^4 x \psi^{\dagger} (x) \psi (x) e^{-ipx} |0>$$

I do not understand why the ##a_{\vec k}e^{ipx}## term vanishes.

Tong justifies it as follows: when ##a^{\dagger}## hits |i> we get a two meson state, which has 'zero overlap' with ##<f|## and 'and there’s nothing in the ##\psi## and ##\psi^{\dagger}## operators that lie between them to change this fact'.

What does he mean with 'zero overlap' with ##<f|##?

He uses the same argument to justify the final solution:
Captura de pantalla (1020).png


With this thread I am aimed at understanding and getting the provided solution.

Thank you.

PS: The amplitude can be computed by formula (3.26), The unitary matrix is given by formula (3.23), where the ##H_{int}## is given by (3.25)
 

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JD_PM said:
Homework Statement:: I am studying how to compute the meson-decay amplitude worked out in Tong's notes (pages 55 and 56; I attached the PDF).
Relevant Equations:: $$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \phi (x) |i>$$

The initial and final states are given by

$$|i > = \sqrt{2 E_{\vec p}} a_{\vec p}^{\dagger} |0>$$

$$|f > = \sqrt{4 E_{\vec q_1}E_{\vec q_2}} b_{\vec q_1}^{\dagger}c_{\vec q_2}^{\dagger} |0>$$

Using Dyson formula's expansion we get that

$$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \phi (x) |i>$$

We first expand out ##\phi \sim a + a^{\dagger}## using the following formula

View attachment 260586
Doing so we get

$$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} a_{\vec k} a_{\vec p}^{\dagger} e^{-ikx} |0> = -ig<f|\int d^4 x \psi^{\dagger} (x) \psi (x) e^{-ipx} |0>$$

I do not understand why the ##a_{\vec k}e^{ipx}## term vanishes.

Tong justifies it as follows: when ##a^{\dagger}## hits |i> we get a two meson state, which has 'zero overlap' with ##<f|## and 'and there’s nothing in the ##\psi## and ##\psi^{\dagger}## operators that lie between them to change this fact'.

What does he mean with 'zero overlap' with ##<f|##?

He uses the same argument to justify the final solution:View attachment 260583

With this thread I am aimed at understanding and getting the provided solution.

Thank you.

PS: The amplitude can be computed by formula (3.26), The unitary matrix is given by formula (3.23), where the ##H_{int}## is given by (3.25)
When people say there is "no overlap" between two states, they mean that ##\langle a | b \rangle = 0 ##. So here he is saying that when the state will be applied to ##\langle f|##, the result will be zero.
 
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JD_PM said:
Homework Statement:: I am studying how to compute the meson-decay amplitude worked out in Tong's notes (pages 55 and 56; I attached the PDF).
Relevant Equations:: $$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \phi (x) |i>$$

The initial and final states are given by

$$|i > = \sqrt{2 E_{\vec p}} a_{\vec p}^{\dagger} |0>$$

$$|f > = \sqrt{4 E_{\vec q_1}E_{\vec q_2}} b_{\vec q_1}^{\dagger}c_{\vec q_2}^{\dagger} |0>$$

Using Dyson formula's expansion we get that

$$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \phi (x) |i>$$

We first expand out ##\phi \sim a + a^{\dagger}## using the following formula

View attachment 260586
Doing so we get

$$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} a_{\vec k} a_{\vec p}^{\dagger} e^{-ikx} |0> = -ig<f|\int d^4 x \psi^{\dagger} (x) \psi (x) e^{-ipx} |0>$$

I do not understand why the ##a_{\vec k}e^{ipx}## term vanishes.
To help a bit more, first let me add this. First, note that you meant that ##a_{\vec k}^{\dagger} \, e^{ipx}## vanishes. Write this term and look at all the annihilation and creation operators sandwiched between the vacuum states. What do you observe?
 
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nrqed said:
To help a bit more, first let me add this. First, note that you meant that ##a_{\vec k}^{\dagger} \, e^{ipx}## vanishes. Write this term and look at all the annihilation and creation operators sandwiched between the vacuum states. What do you observe?

Yes you are right, I meant to ask 'why does ##a_{\vec k}^{\dagger} \, e^{ipx}## vanish?'

Let's write it explicitly and see why it does. We have:

$$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} \Big(a_{\vec k}e^{-ikx}+a_{\vec k}^{\dagger}e^{ikx} \Big) a_{\vec p}^{\dagger}|0>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} \Big(a_{\vec k}a_{\vec p}^{\dagger}e^{-ikx}|0>+a_{\vec k}^{\dagger}a_{\vec p}^{\dagger}e^{ikx}|0> \Big)$$

Mmm but I still do not see why the following term is zero

$$ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} a_{\vec k}^{\dagger}a_{\vec p}^{\dagger}e^{ikx}|0>=0$$
 
JD_PM said:
Yes you are right, I meant to ask 'why does ##a_{\vec k}^{\dagger} \, e^{ipx}## vanish?'

Let's write it explicitly and see why it does. We have:

$$<f|S|i>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} \Big(a_{\vec k}e^{-ikx}+a_{\vec k}^{\dagger}e^{ikx} \Big) a_{\vec p}^{\dagger}|0>=-ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} \Big(a_{\vec k}a_{\vec p}^{\dagger}e^{-ikx}|0>+a_{\vec k}^{\dagger}a_{\vec p}^{\dagger}e^{ikx}|0> \Big)$$

Mmm but I still do not see why the following term is zero

$$ig<f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} a_{\vec k}^{\dagger}a_{\vec p}^{\dagger}e^{ikx}|0>=0$$
Two ##\phi## particles are created out of the vacuum. Do theyget annihilated before you apply the vacuum bra?
 
nrqed said:
Two ##\phi## particles are created out of the vacuum. Do they get annihilated before you apply the vacuum bra?

I'd say yes but I do not know why... could you please give me a hint? :)
 
JD_PM said:
I'd say yes but I do not know why... could you please give me a hint? :)
Sure. If you have two creation operators acting on the vacuum, you need two annihilation operators for the same particle type in order to have a non zero result. So you need two operators ##a_p, a_p'## somewhere in your expression to compensate for the two creation operators. Do you have these?
 
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nrqed said:
Sure. If you have two creation operators acting on the vacuum, you need two annihilation operators for the same particle type in order to have a non zero result. So you need two operators ##a_p, a_p'## somewhere in your expression to compensate for the two creation operators. Do you have these?

Oh so the reason is that, as there are no ##a_p, a_p'## compensating ##a_p^{\dagger}, a_p'^{\dagger}##, then that term has to be zero. Alright thanks!

How could we prove that statement though? Through commutation relations?

I am going to try again and see if I get the final answer (it will be tricky though o_O)

Captura de pantalla (1020).png
 
JD_PM said:
Oh so the reason is that, as there are no ##a_p, a_p'## compensating ##a_p^{\dagger}, a_p'^{\dagger}##, then that term has to be zero. Alright thanks!

How could we prove that statement though? Through commutation relations?

I am going to try again and see if I get the final answer (it will be tricky though o_O)

It follows from the fact that states with different number of particles (of each type) are orthogonal. For example, if ##| \alpha \rangle ## is a state containing two particles of type ##\phi##, in other words if it is proportional to

$$ |\alpha \rangle \propto a_k^\dagger a^\dagger_{k'} |0 \rangle $$

then we automatically have

$$ \langle 0 | \alpha \rangle = 0. $$

Good luck with the rest of your calculation. If you get stuck on something, don't hesitate to ask!
 
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  • #10
Please let me show all my work and then add some comments.

So we were dealing with the leading order in g

$$\langle f|S|i\rangle=-ig \langle f| \int d^4 x \psi^{\dagger} (x) \psi (x) \phi (x) |i \rangle \ \ \ \ (1)$$

I'll go step by step

1) We plug the mode expansion for ##\phi## and the given definition for ##|i\rangle## into (1) to get

##\langle f|S|i \rangle =-ig \langle f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} \Big(a_{\vec k}a_{\vec p}^{\dagger}e^{-ikx}|0 \rangle +a_{\vec k}^{\dagger}a_{\vec p}^{\dagger}e^{ikx}|0 \rangle \Big)##

Thanks to your explanation at #9 I see that we have ##\langle 0 |a_{\vec k}^{\dagger}a_{\vec p}^{\dagger}| 0 \rangle=0##. So we end up with

$$\langle f|S|i\rangle=-ig \langle f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} a_{\vec k}a_{\vec p}^{\dagger}e^{-ikx}|0\rangle \ \ \ \ (2)$$

2) Use the commutation relation ##[a_{\vec k}, a_{\vec p}^{\dagger}] = \delta^3 (\vec p - \vec k)##

Based on the commutation relation we know that ##a_{\vec k}a_{\vec p}^{\dagger}=\delta^3 (\vec p - \vec k)+a_{\vec p}^{\dagger}a_{\vec k}##. Plugging it into (2) we get

$$\langle f|S|i\rangle=-ig \langle f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} \Big( \delta^3 (\vec p - \vec k)+a_{\vec p}^{\dagger}a_{\vec k} \Big)e^{-ikx}|0\rangle $$

We know that, by definition, we have ##a_{\vec k}|0\rangle = 0##. Thus (2) of course becomes

$$\langle f|S|i\rangle=-ig \langle f| \int d^4 x \psi^{\dagger} (x) \psi (x) \int \frac{d^3 k \sqrt{2E_{\vec p}}}{(2 \pi)^3 \sqrt{2E_{\vec k}}} \delta^3 (\vec p - \vec k) e^{-ikx}|0\rangle$$

Based on the famous sifting property of the Dirac delta function (i.e. ##\int f(t) \delta (t-T) dt = f(T)##), we compute the following integral

$$\int \frac{d^3 k}{\sqrt{2E_{\vec k}}} \delta^3 (\vec p - \vec k) e^{-ikx} = \frac{(2\pi)^3}{\sqrt{2E_{\vec p}}} e^{-ipx}$$

Thus we end up with

$$\langle f|S|i\rangle=-ig \langle f| \int d^4 x \psi^{\dagger} (x) \psi (x) e^{-ipx}|0\rangle \ \ \ \ (3)$$

3) Recall the mode expansion of the complex field

$$\psi = \int \frac{d^3 k_1}{(2 \pi)^3} \frac{1}{\sqrt{2E_{\vec k_1}}}\Big( b_{\vec k_1}e^{i k_1 x}+c_{\vec k_1}^{\dagger}e^{-i k_1 x}\Big)$$

$$\psi^{\dagger} = \int \frac{d^3 k_2}{(2 \pi)^3} \frac{1}{\sqrt{2E_{\vec k_2}}}\Big( b_{\vec k_2}^{\dagger}e^{-i k_2 x}+c_{\vec k_2}e^{i k_2 x}\Big)$$

4) Plug the mode expansion for ##\psi##, ##\psi^{\dagger}## and ##\langle f|= \langle 0| \sqrt{4 E_{\vec q_1} E_{\vec q_2}}c_{\vec q_2} b_{\vec q_1}## into (3)

##\langle f|S|i\rangle=-ig \langle 0|\iiint d^4 x \frac{d^3 k_2 d^3 k_1}{(2 \pi)^6} \frac{\sqrt{4 E_{\vec q_1} E_{\vec q_2}}}{\sqrt{4 E_{\vec k_2} E_{\vec k_1}}}c_{\vec q_2} b_{\vec q_1}\Big( b_{\vec k_2}^{\dagger}e^{-i k_2 x}+c_{\vec k_2}e^{i k_2 x}\Big) \Big( b_{\vec k_1}e^{i k_1 x}+c_{\vec k_1}^{\dagger}e^{-i k_1 x}\Big) e^{-ipx}|0\rangle \ \ \ \ (4)##

The only non-zero term is ##\langle 0| c_{\vec q_2} b_{\vec q_1} b_{\vec k_2}^{\dagger} c_{\vec k_1}^{\dagger} | 0 \rangle##. Thus (4) becomes

$$\langle f|S|i\rangle=-ig \langle 0|\iiint d^4 x \frac{d^3 k_2 d^3 k_1}{(2 \pi)^6} \frac{\sqrt{4 E_{\vec q_1} E_{\vec q_2}}}{\sqrt{4 E_{\vec k_2} E_{\vec k_1}}}c_{\vec q_2} b_{\vec q_1} b_{\vec k_2}^{\dagger}c_{\vec k_1}^{\dagger}|0\rangle e^{-i(k_2+k_1+p)x} \ \ \ \ (5)$$

5) Use the commutation relation ##[b_{\vec q_1}, b_{\vec k_2}^{\dagger}] = \delta^3 (\vec k_2 - \vec q_1)##

Based on the commutation relation we know that ##b_{\vec q_1} b_{\vec k_2}^{\dagger}=\delta^3 (\vec k_2 - \vec q_1)+b_{\vec k_2}^{\dagger}b_{\vec q_1}##. Plugging it into (5) we get

$$\langle f|S|i\rangle=-ig \langle 0|\iiint d^4 x \frac{d^3 k_2 d^3 k_1}{(2 \pi)^6} \frac{\sqrt{4 E_{\vec q_1} E_{\vec q_2}}}{\sqrt{4 E_{\vec k_2} E_{\vec k_1}}} \delta^3 (\vec k_2 - \vec q_1) c_{\vec q_2} c_{\vec k_1}^{\dagger}|0\rangle e^{-i(k_2+k_1+p)x}$$

Where I've used the fact that ##b_{\vec q_1} |0\rangle =0##

Based on the famous sifting property of the Dirac delta function (i.e. ##\int f(t) \delta (t-T) dt = f(T)##), we compute the following integral

$$\int \frac{d^3 k_2}{\sqrt{2E_{\vec k_2}}} \delta^3 (\vec k_2 - \vec q_1) e^{-i k_2 x} = \frac{(2\pi)^3}{\sqrt{2E_{\vec q_1}}} e^{i q_1 x}$$

6) Use the commutation relation ##[c_{\vec q_2}, c_{\vec k_1}^{\dagger}] = \delta^3 (\vec k_1 - \vec q_2)##

Based on the commutation relation we know that ##c_{\vec q_2} c_{\vec k_1}^{\dagger}=\delta^3 (\vec k_1 - \vec q_2)+c_{\vec k_1}^{\dagger}c_{\vec q_2}##.

At this point we proceed the same way as 5): we use the fact that ##c_{\vec q_2}|0\rangle=0## and we solve the integral

$$\int \frac{d^3 k_1}{\sqrt{2E_{\vec k_1}}} \delta^3 (\vec k_1 - \vec q_2) e^{-i k_1 x} = \frac{(2\pi)^3}{\sqrt{2E_{\vec q_2}}} e^{i q_2 x}$$

7) Use 5) and 6) to solve equation (5)

$$\langle f|S|i\rangle=-ig \langle 0|\int d^4 x e^{i(q_1+q_2-p)x}|0\rangle = -ig (2\pi)^4 \delta^4 (q_1+q_2-p)$$
 
  • #11
I think I got it right but, to be honest, it feels like I cheated; I already knew the answer and based on it I got the the following integral:

$$\int \frac{d^3 k_2}{\sqrt{2E_{\vec k_2}}} \delta^3 (\vec k_2 - \vec q_1) e^{-i k_2 x} = \frac{(2\pi)^3}{\sqrt{2E_{\vec q_1}}} e^{i q_1 x}$$

Particularly, I do not see why the sign of the exponent changes after solving the integral.
 

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