A Hyperbolic Metric

The Poincare half-plane model for hyperbolic space puts the following metric on the plane:

d s 2 = 1 y 2 ( d x 2 + d y 2 ) . ds^2 = \frac{1}{y^2} (dx^2 + dy^2).

Compute the Ricci scalar R R for this metric in matrix form. Is this a vacuum solution to Einstein's equations?

Give your answer as an ( R , (R, Yes/No ) ) pair.

2 ; No -2 ; \text{ No} 1 y 2 ; Yes \frac1{y^2}; \text{ Yes} 0 ; No 0 ; \text{ No} 2 ; Yes -2 ; \text{ Yes}

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1 solution

Matt DeCross
May 10, 2016

The Ricci tensor for this metric is (skipping the many steps involved in obtaining the Ricci tensor, which are tedious):

R μ ν = ( 1 y 2 0 0 1 y 2 ) . R_{\mu \nu} = \begin{pmatrix} -\frac{1}{y^2} & 0 \\ 0 & -\frac{1}{y^2} \end{pmatrix}.

The Ricci scalar is thus R = g μ ν R μ ν = 2 R = g^{\mu \nu} R_{\mu \nu} = -2 . The hyperbolic half-space is one of constant negative curvature.

Computing the Einstein tensor, one finds:

G μ ν = R μ ν 1 2 R g μ ν = 0. G_{\mu \nu} = R_{\mu \nu} - \frac12 R g_{\mu \nu} = 0.

Thus, this metric is a solution for the vacuum Einstein equations. This seems strange because this is a space of constant negative curvature, which would seem to require some sort of matter/energy. However, the reason why it is allowed is that this is just a two-dimensional spatial metric, which turns out to be a degenerate case for the Einstein equations.

How was i supposed to know that R= g^( mu nu) R_( mu nu)? This should be in the article. I've never studied covariance and contravariance. The definition of the ricci scalar in tension from the ricci tensor was unclear

Bryce Cannon - 1 year, 1 month ago

So basically it's a solution because you say so, no need to show your work...? The question was to find it, and you skipped that part

David Löfqvist - 11 months ago

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