Diffeomorphism invariance of the Polyakov action

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Discussion Overview

The discussion revolves around the diffeomorphism invariance of the Polyakov action in the context of string theory. Participants explore the mathematical formulation of the action, the implications of diffeomorphism transformations on the world-sheet metric, and the properties of certain scalar quantities derived from the action.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant presents the Polyakov action and expresses confusion regarding the derivation of the Einstein variation of the world-sheet metric under diffeomorphism transformations.
  • Another participant suggests expanding the left-hand side of the equation to clarify the terms involved in the variation.
  • There is a query about the definition of an "Einstein scalar" and whether the expression \( h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu \) transforms as a scalar function.
  • Concerns are raised about the placement of parentheses in the expression for the variation of \( \sqrt{-h} \), indicating uncertainty about the mathematical formulation.
  • A later reply proposes a general fact about operators satisfying the Leibniz rule, which may help in proving the relations discussed.

Areas of Agreement / Disagreement

Participants express varying degrees of understanding and agreement on the properties of the Polyakov action and the transformations involved, but no consensus is reached on the specific mathematical details or definitions, indicating ongoing debate and exploration of the topic.

Contextual Notes

Participants note the need for careful handling of mathematical expressions and the implications of diffeomorphism invariance, but specific assumptions and definitions remain unresolved.

maverick280857
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[SOLVED] Diffeomorphism invariance of the Polyakov action

Hi,

I'm struggling with something that is quite elementary. I know that the Polyakov action is diffeomorphism invariant and Weyl invariant. Denoting the world-sheet coordinates \sigma^0 = \sigma and \sigma^1 = t and the independent world-sheet metric by h_{\alpha\beta}(\sigma), the Polyakov action can be written as

S_{P} = -\frac{T}{2}\int d^{2}\sigma \, \sqrt{-h}h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu

where T is the string tension and \alpha, \beta run over 0 and 1 (labeling \sigma and t).

Now, if I define

\delta_{E}h_{\alpha\beta}(\sigma) = h_{\alpha\beta}'(\sigma) - h_{\alpha\beta}(\sigma)

as the Einstein variation of the independent world-sheet metric, where the primed coordinates denote the transformed world-sheet coordinates under a diffeomorphism defined by

{\sigma'}^{\gamma} = \sigma^\gamma - \xi^\gamma(\sigma)

then I would like to show that

\delta_E h_{\alpha\beta} = \partial_\alpha \xi^\gamma h_{\gamma\beta} + \partial_\beta \xi^\gamma h_{\alpha\gamma} + \xi^\gamma \partial_\gamma h_{\alpha\beta}

This is supposed to follow from chain rule, but I do not quite get all the terms.

My working

h'_{\gamma\delta}(\sigma') = h_{\alpha\beta}(\sigma)\frac{d\sigma^\alpha}{d{\sigma'}^\gamma}\frac{d{\sigma}^\beta}{d{\sigma'}^\delta}

Now by definition,

\sigma^\alpha = {\sigma'}^\alpha + \xi^\alpha(\sigma)

So,

\frac{d\sigma^\alpha}{d{\sigma'}^\beta} = \delta^\alpha_\beta + \frac{d\sigma^\delta}{d{\sigma'}^\beta}\frac{d{\xi}^\alpha(\sigma)}{d {\sigma}^{\delta}}

But this seems to give only the first two terms of \delta_E h and not the third one, which is the usual derivative (change along gradient) term that I'd expect to get.

Any suggestions will be greatly appreciated.

Thanks!
 
Last edited:
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Solved. Thanks anyway!
 
maverick280857 said:
Hi,
h'_{\gamma\delta}(\sigma') = h_{\alpha\beta}(\sigma)\frac{d\sigma^\alpha}{d{\sigma'}^\gamma}\frac{d{\sigma}^\beta}{d{\sigma'}^\delta}

Thanks!

Expand the left-hand-side as well
h^{'}_{ \mu \nu } ( \sigma^{'} ) = h^{'}_{ \mu \nu } ( \sigma - \xi ) \approx h^{'}_{ \mu \nu } ( \sigma ) - \xi^{ \rho } \partial_{ \rho } h^{'}_{ \mu \nu } ( \sigma ) .
But infinitesimally
\xi^{ \rho } \partial_{ \rho } h^{'}_{ \mu \nu } ( \sigma ) \approx \xi^{ \rho } \partial_{ \rho } h_{ \mu \nu } ( \sigma ) .
 
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Thanks samalkhaiat, yes, I got that.

I would also like to show that

(a) \delta_E(h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu) = \xi^\rho \partial_\rho(h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu) because "h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu is an Einstein scalar". What is an Einstein scalar?

My guess is that h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu transforms as a scalar function.

(b) \delta_E(\sqrt{-h}) = \partial_\rho(\xi^\rho \sqrt{-h})

This one worries me a little because of the placement of parenthesis...any ideas?

How does one prove these relations?
 
Last edited:
maverick280857 said:
Thanks samalkhaiat, yes, I got that.

I would also like to show that

(a) \delta_E(h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu) = \xi^\rho \partial_\rho(h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu) because "h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu is an Einstein scalar". What is an Einstein scalar?

My guess is that h^{\alpha\beta}\partial_\alpha X^\mu \partial_\beta X_\mu transforms as a scalar function.
That is correct.

(b) \delta_E(\sqrt{-h}) = \partial_\rho(\xi^\rho \sqrt{-h})

This one worries me a little because of the placement of parenthesis...any ideas?

How does one prove these relations?
Use the following fact. For any operator \hat{ \delta }, satisfying the Leibnz rule such as ( \partial , \delta ), the following can be proven
\frac{ \hat{ \delta }( \sqrt{ - g } ) }{ \sqrt{ - g } } = \frac{1}{2} g^{ \mu \nu } \hat{ \delta } g_{ \mu \nu } .

Sam
 

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