Finding local flat space of the Poincare half-disk

Click For Summary
SUMMARY

The discussion focuses on finding local flat space coordinates for the metric \( ds^2 = \frac{dx^2 + dy^2}{y^2} \). Participants analyze the metric components \( g_{yy} = \frac{1}{y^2} \) and \( g_{xx} = \frac{1}{x^2} \), and explore the process of expanding the metric around the point \( (0, y_*) \). The objective is to transform the metric into an identity matrix by eliminating the first-order coefficient \( A \) through a coordinate transformation defined by \( x^{\mu} = k^\mu_\nu x^{'\nu} + L^\mu_{\nu\lambda} x^{\nu} x^{\lambda} + ... \). The discussion highlights the need to solve for \( k^\mu_\nu \) and \( L^\mu_{\nu\lambda} \) to achieve the desired transformation.

PREREQUISITES
  • Understanding of differential geometry and metric tensors
  • Familiarity with coordinate transformations in Riemannian geometry
  • Knowledge of Taylor series expansions in multiple dimensions
  • Experience with mathematical notation and tensor calculus
NEXT STEPS
  • Study the process of metric expansion in Riemannian geometry
  • Learn about coordinate transformations and their applications in general relativity
  • Explore the implications of the identity matrix in the context of metric tensors
  • Investigate the relationship between first-order and second-order terms in metric expansions
USEFUL FOR

Students and researchers in theoretical physics, particularly those studying general relativity and differential geometry, as well as mathematicians interested in the properties of metric tensors.

ozone
Messages
121
Reaction score
0
Ω

Homework Statement



Given the metric ds^2 = \frac{dx^2 + dy^2}{y^2} find a set of coordinates which yield local flat space. i.e. (g_{\mu\nu} = \delta_{\mu\nu} + second order terms).

My text outlined a process to go through to find the flat space coordinates, but the actual execution is slightly beyond me. I would really like to know how to complete this problem for my own understanding.. Let's dive into the math then:

Our given metric is g_{yy} = \frac{1}{y^2} , g_{xx}= \frac{1}{x^2}. Then without any loss of generality we may expand this metric about the point (0,y_{*}) the resulting expansion will leave us with new metric terms given as

g_{yy} = \frac{1}{y_{*}^2} - \frac{2}{y_*^3} (y-y_*) + \frac{6}{y^4_*} (y-y_*)^2, g_{xx} = \frac{1}{y_{*}^2}

we might write this in the form g_{\mu\nu}(x) = g_{\mu\nu}(0) + A_{\mu\nu,\lambda} x^\lambda +B_{\mu\nu,\lambda \sigma} x^\lambda x^\sigma

However we really don't need to worry about our second order coefficient, as our only aim right now is to take our constant term and turn it into the identity matrix, and to find a coordinate system which will remove our first order matrix coefficient A.

Then doing a coordinate transformation to x^{\mu} = k^\mu_\nu x^{'\nu} + L^\mu_{\nu\lambda} x^{\nu} x^{\lambda} + ...

We are now ready to solve for k^\mu_\nu and for reasons which aren't 100% clear to me (I believe it has to do with the definition of the metric tensor being the first order derivatives of x and the way it transforms) my book states that we wish to solve the equation g'_{\rho\sigma}(0) = k^\mu_\lambda k^\nu_\sigma g_{\mu\nu}(0). This seems logical to me and I can generally follow up to this point, I can solve that with ease(we want our primed 0th order term to be an identity matrix), but I did not know how to deduce the relationship we want to solve for L^\mu_{\nu\lambda}, furthermore my book made the cryptic statement that solving for k will change the resulting value of our coefficient L. Any help on solving for the with which we can L eliminate our coefficient A would be much appreciated
 
Physics news on Phys.org
Any luck with the answer?

Sorry for bringing this old post back. I am going through the exact same problem. I was wondering if you figured out the answer and could help me understand it. And also shouldn't gxx=gyy=1/y2?
P.S. Which book were you referring to?
 

Similar threads

  • · Replies 5 ·
Replies
5
Views
3K
Replies
0
Views
2K
Replies
1
Views
4K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 22 ·
Replies
22
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 5 ·
Replies
5
Views
5K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K