Constraint on conformal transformation (Ketov)

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SUMMARY

The discussion centers on a differential equation related to conformal transformations as presented in the book "Conformal Field Theory" by Ketov. The author identifies a discrepancy in the signs of terms derived from the transformation equations, specifically in the expression for the metric tensor under the transformation. The solution involves correcting a sign error by substituting \(\omega\) with \(-\omega\) and taking the trace of both sides, thereby aligning the results with those in Ketov's text.

PREREQUISITES
  • Understanding of Conformal Field Theory (CFT)
  • Familiarity with differential geometry and metric tensors
  • Knowledge of the chain rule in calculus
  • Experience with Taylor expansions in mathematical physics
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  • Study the derivation of conformal transformations in "Conformal Field Theory" by Ketov
  • Learn about the implications of sign errors in differential equations
  • Research the role of trace operations in tensor calculus
  • Explore advanced topics in differential geometry related to metric modifications
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This discussion is beneficial for theoretical physicists, graduate students in mathematical physics, and researchers focusing on conformal field theories and their applications in quantum field theory.

maverick280857
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Hi,

First of all, I'm not sure if this thread belongs to the BSM forum because the question I'm posing here is a simple CFT question which could well be posed in the forum on GR or Particle Physics/QFT. I will defer to the judgment of the moderator to put this in the right place if it already isn't.

So, while working through the book on Conformal Field Theory by Ketov, I came across a differential equation that must be satisfied by the conformal parameter \xi defined through

x^\mu \rightarrow {\tilde{x}}^\mu = x^\mu + \xi^\mu

Now,

\tilde{g}_{\mu\nu}(\tilde{x}) = \frac{\partial x^\lambda}{\partial \tilde{x}^\mu}\frac{\partial x^\rho}{\partial \tilde{x}^\nu}g_{\lambda\rho}(x)

For the infinitesimal transformation in question,

\frac{\partial x^\mu}{\partial \tilde{x}^\rho} = \delta^{\mu}_{\rho} - \frac{\partial x^\lambda}{\partial \tilde{x}^\rho}\frac{\partial \xi^{\mu}}{\partial x^\lambda}

using the chain rule in the second term. Now, to lowest order in \xi, this becomes

\frac{\partial x^\mu}{\partial \tilde{x}^\rho} = \delta^{\mu}_{\rho} - \partial_{\rho}\xi^\mu

But this means,

\tilde{g}_{\mu\nu}(\tilde{x}) = g_{\mu\nu}(x) - g_{\mu\rho}(x)\partial_\nu\xi^\rho - g_{\nu\lambda}\partial_\mu \xi^\lambda

which, with the identification \Omega(x) = e^{\omega(x)} and \tilde{g}(\tilde{x}) = \Omega(x)g_{\mu\nu}(x), yields

(1 + \omega)g_{\mu\nu} = g_{\mu\nu} - \partial_\nu \xi_\mu - \partial_\mu \xi_\nu

The right hand side has the wrong signs for the second and third terms, when compared to the result given in Ketov's book. Now this looks like a fairly straightforward application of the chain rule and Taylor expansion, to me. Is there something I'm missing?

Thanks in advance!
 
Physics news on Phys.org
Solved. There is a sign error but this can be fixed by replacing \omega with -\omega and taking the trace of both sides.
 

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