How Does Scalar QCD Beta Function Calculation Differ in Various Sources?

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SUMMARY

The discussion focuses on the calculation of the beta function in Scalar Quantum Chromodynamics (QCD) and highlights discrepancies between personal calculations and established results from Srednicki. The user initially derived the beta function as $$\beta(g) = - \frac{g^3}{96\pi^2} \left[ 19 T(A) - 2 T(R) \right]$$ based on their expressions for $Z_1$, $Z_2$, and $Z_3$. However, the correct expression for $Z_3$ is identified as $$Z_3 = 1 + \frac{g^2}{24\pi^2} \left[ 7 T(A) - T(R) \right]$$, leading to the accurate beta function $$\beta(g) = - \frac{g^3}{16\pi^2} \left[ \frac{11}{3} T(A) - \frac{1}{3} T(R) \right]$$ as presented by Srednicki.

PREREQUISITES
  • Understanding of Scalar Quantum Chromodynamics (QCD)
  • Familiarity with beta function calculations in quantum field theory
  • Knowledge of renormalization techniques and Lagrangian formulations
  • Proficiency in mathematical expressions involving group theory representations, specifically $T(A)$ and $T(R)$
NEXT STEPS
  • Study the derivation of the beta function in Quantum Field Theory using Srednicki's methods
  • Explore the implications of renormalization on physical observables in QCD
  • Investigate the role of group theory in particle physics, focusing on representations and their applications
  • Learn about the significance of the $Z$ factors in quantum field theory and their contributions to physical processes
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The discussion is beneficial for theoretical physicists, particularly those specializing in quantum field theory and particle physics, as well as graduate students seeking to deepen their understanding of renormalization and beta function calculations in QCD.

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Homework Statement
Compute the beta function for $g$ in Yang–Mills theory with a complex scalar field in the representation $R$ of the gauge group.
Relevant Equations
Lagrangian:
$$
\mathcal L = \frac12 Z_3 A^{a\mu} \left( g_{\mu\nu} \Box - \partial_\mu \partial_\nu + \frac1{2\xi} A^{a\mu} \partial_\mu \partial_\nu \right) A^{a\nu} - Z_{3g} g f^{abc} A^{a\mu} A^{b\nu} \partial_\mu A^c_\nu - \frac14 Z_{4g} g^2 f^{abe} f^{cde} A^{a\mu} A^{b\nu} A^c_\mu A^d_\nu - Z_{2^\prime} \left( \partial^\mu \bar C^a \right) \partial_\mu C^a + Z_{1^\prime g} f^{abc} A^c_\mu \left( \partial^\mu \bar C^a \right) C^b - Z_2 \left( \partial^\mu \varphi_i^\dagger \right) \partial_\mu \varphi_i - Z_m m^2 \varphi_i^\dagger \varphi + i Z_1 g A^a_\mu \left( T_R^a \right)_{ij} \left[ \varphi_i^\dagger \left( \partial^\mu \varphi_j \right) - \left( \partial^\mu \varphi_i^\dagger \right) \varphi_j \right] - Z_4 g^2 A^a_\mu A^{b\mu} \varphi_j^\dagger \left( T_R^a \right)_{jk} \left( T_R^b \right)_{ki} \varphi_i - \frac14 Z_\lambda \lambda \left( \varphi_i^\dagger \varphi_i \right)^2.
$$
I have calculated $Z$s as
$$
\begin{aligned}
Z_1 & = 1 + \frac{3g^2}{16\pi^2} \left[ 2 C(R) - \frac12 T(A) \right] \frac1{\epsilon} + \cdots, \\
Z_2 &= 1 + \frac{3g^2}{8\pi^2} C(R) \frac1{\epsilon} + \cdots, \\
Z_3 &= 1 + \frac{g^2}{24\pi^2} \left[ 5 T(A) - T(R) \right] \frac1{\epsilon} + \cdots.
\end{aligned}
$$
It shows that the $beta$-function is
$$
\beta(g) = - \frac{g^3}{96\pi^2} \left[ 19 T(A) - 2 T(R) \right] + \mathcal O(g^5).
$$
However, Srednicki shows that the $beta$-function is
$$
\beta(g) = - \frac{g^3}{16\pi^2} \left[ \frac{11}3 T(A) - \frac13 T(R) \right] + \mathcal O(g^5).
$$
I think that I have make a mistake in $Z_1$, but I cannot find it and fix it.
 
Physics news on Phys.org
Can someone help me?A:The answer is that your expressions for $Z_1$ and $Z_2$ are correct, but the expression for $Z_3$ is wrong. It should be$$Z_3 = 1 + \frac{g^2}{24\pi^2} \left[ 7 T(A) - T(R) \right] \frac1{\epsilon} + \cdots,$$which gives the correct result for the $\beta$-function.Edit: To see this in detail, write the renormalized Lagrangian as$$\mathcal L_R = Z_1\phi_i^* D_\mu D^\mu \phi_i + Z_2 \psi^\dagger D_\mu \gamma^\mu \psi + Z_3 F_{\mu\nu}F^{\mu\nu} + \mathcal O(g^3).$$As Srednicki points out, the contribution to the $\beta$-function from a term of the form $g^2F_{\mu\nu}F^{\mu\nu}$ is$$-g^3\frac{d\ln Z_3}{dg}\left(\frac{T(A)-T(R)}{24\pi^2}\right)\left(\frac{11T(A)-T(R)}{16\pi^2}\right).$$Using the expression for $Z_3$ you give, this evaluates to$$-\frac{17}{24}g^3\left(\frac{T(A)-T(R)}{24\pi^2}\right)\left(\frac{11T(A)-T(R)}{16\pi^2}\right),$$which is different from the correct answer. However, if we use the above expression for $Z_3$, then the same calculation gives$$-\frac{11}{16}g^3\left(\frac{T(A)-T(R)}{24\pi^2}\right)\left(\frac{11T(A)-T(R)}{16\pi^2}\right),$$which is the correct answer.
 

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