Lightlike geodesic in AdS5xS5, plane wave background

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Homework Help Overview

The discussion revolves around understanding the behavior of a lightlike particle in the context of the AdS_5×S^5 metric, particularly how it relates to a plane wave background. The original poster references specific lecture notes and seeks clarification on the metric's transformation under certain coordinate changes as the radius approaches infinity.

Discussion Character

  • Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to derive the metric in a limit and questions the emergence of mixed terms in the expansion related to the coordinates. Other participants suggest examining the quadratic terms in the expansions of trigonometric functions and express the need for precision in the comparison of terms.

Discussion Status

Participants are actively engaging with the mathematical details of the problem, with some providing guidance on how to approach the comparison of terms. There is an ongoing exploration of the implications of the coordinate transformations and the resulting metric forms.

Contextual Notes

There is a focus on the limit as R approaches infinity, and the discussion highlights potential assumptions or simplifications that may affect the interpretation of the terms involved in the metric expansion.

physicus
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Homework Statement



My question is about a step in the lecture notes [http://arxiv.org/abs/hep-th/0307101] on page 6, and it is probably quite trivial:

I want to see why a lightlike particle in AdS_5\times S^5 sees the metric as plane wave background. The metric is
ds^2=R^2(-dt^2 \cosh^2\rho+d\rho^2+\sinh^2\rho \,d\Omega_3^2+d\psi^2\cos^2\theta+d\theta^2+\sin^2\theta\,\Omega_3'^2)

In order to study the metric close to a lightlike geodesic we make the follwoing change of coordinates:
{x}^+=\frac{1}{2\mu}(t+\psi), {x}^-=\frac{\mu R^2}{2}(t-\psi), \rho=\frac{r}{R}, \theta=\frac{y}{R}

I am supposed to get in the R\to\infty limit
ds^2=R^2(-\mu^2(dx^+)^2+\mu^2(dx^+)^2)+(-2dx^+dx^--\mu^2r^2(dx^+)^2+dr^2+r^2d\Omega_3^2 -2dx^+dx^--\mu^2y^2(dx^+)^2+dy^2+y^2d\Omega'{}_3^2)+\mathcal{O}(R^{-2})

This is not the final result, but from there on I know how to continue.

Homework Equations



\cosh x=1+\frac{1}{2}x^2+\mathcal{O}(x^4), \cos x=1-\frac{1}{2}x^2+\mathcal{O}(x^4)
\Rightarrow \cosh^2 x = 1+x^2+\mathcal{O}(x^4), \cosh^2 x = 1-x^2+\mathcal{O}(x^4)

The Attempt at a Solution



I can expand in \rho, \theta, since they will be small in the R \to \infty limit:
ds^2=R^2(-dt^2 \cosh^2\rho+d\rho^2+\sinh^2\rho \,d\Omega_3^2+d\psi^2\cos^2\theta+d\theta^2+\sin^2\theta\,\Omega'{}_3^2)
=R^2(-dt^2(1+\rho^2)+d\rho^2+\rho^2d\Omega_3^2+d\psi^2(1-\theta^2)+d\theta^2+\theta^2d\Omega'{}_3^2)+\mathcal{O}(R^{-2})
=R^2(-dt^2+d\psi^2)+(-dt^2r^2+dr^2+r^2d\Omega_3^2-d\psi^2y^2+dy^2+y^2d\Omega'{}_3^2=+\mathcal{O}(R^{-2})

Now I use:
dx^+dx^-=\frac{1}{2\mu}(dt+d\psi)\frac{\mu R^2}{2}(dt-d\psi)=\frac{R^2}{4}(dt^2-d\psi^2)
So the first term above is R^2(-dt^2+d\psi^2)=-4dx^+dx^-.

However, I do not know where all the (dx^+)^2 in the solution are coming from, since
(dx^+)^2=\frac{1}{4\mu^2}(dt^2+2dt\,d\psi+d\psi^2)
Where do these mixed dt\,d\psi terms come from?
 
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They come from quadratic terms in the expansion of cos and cosh that are finite in the scaling limit.
 
Thank you, but could you be a bit more precise, please. From comparing the given result and what I got so far I should be able to show:
-dt^2r^2-d\psi^2y^2=R^2(-\mu^2(dx^+)^2+\mu^2(dx^+)^2)-\mu^2r^2(dx^+)^2-\mu^2y^2(dx^+)^2
The left hand sinde are those quadratic terms from the expansion of \cos and \cosh. Since the first part of the right hand side is 0 anyways, I don't mind to much that I don't get that one, but I still don't see the equality:
-\mu^2r^2(dx^+)^2-\mu^2y^2(dx^+)^2=-\frac{r^2+y^2}{4}(dt^2+2dt\,d\psi+d\psi^2)
Why is this equal to -r^2dt^2-y^2d\psi^2?
 
physicus said:
Thank you, but could you be a bit more precise, please. From comparing the given result and what I got so far I should be able to show:
-dt^2r^2-d\psi^2y^2=R^2(-\mu^2(dx^+)^2+\mu^2(dx^+)^2)-\mu^2r^2(dx^+)^2-\mu^2y^2(dx^+)^2
The left hand sinde are those quadratic terms from the expansion of \cos and \cosh. Since the first part of the right hand side is 0 anyways, I don't mind to much that I don't get that one, but I still don't see the equality:
-\mu^2r^2(dx^+)^2-\mu^2y^2(dx^+)^2=-\frac{r^2+y^2}{4}(dt^2+2dt\,d\psi+d\psi^2)
Why is this equal to -r^2dt^2-y^2d\psi^2?

You are making the mistake of working backwards from the answer, when there are terms that get dropped in the limit. You can't obtain these original terms from just the finite part, hence your confusion. Express ##t,\psi## in terms of ##x^\pm## and just write down what

$$-dt^2r^2-d\psi^2y^2$$

works out to be.
 
Perfect, thanks!
 

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