1. May 3, 2014

### exmarine

In Dirac's book on GRT, he says the following, p. 45: "In curved space the conservation of energy and momentum is only approximate. The error is to be ascribed to the gravitational field working on the matter and having itself some energy and momentum."

Yet when I work my way from the Schwarzschild metric to the geodesic equations, one of them produces the conservation of angular momentum. There is no approximation that I am aware of.

What am I missing? Was Dirac wrong? Can anyone explain? Thanks.

2. May 3, 2014

### HomogenousCow

I think he was referring to arbitrary metrics. A general metric without angular symmetry will not conserve angular momentum along the geodesic.

3. May 3, 2014

### WannabeNewton

Say instead we were talking about the EM field. Then $T_{\mu\nu} = T^{\text{charges}}_{\mu\nu} + T^{\text{EM}}_{\mu\nu}$ hence $\nabla^{\mu}T_{\mu\nu} = 0$ already takes into account the energy-momentum of the EM field when talking about the local conservation of energy-momentum of the charge distribution interacting with this EM field. It is immediate from this why there comes a difficulty when wanting to take into account the energy-momentum of the gravitational field interacting with a given matter distribution in speaking of the local conservation of energy-momentum because we cannot write down the local energy-density of the gravitational field; $\nabla^{\mu}T_{\mu\nu} = 0$ does not account for this! In fact in GR we can only talk about the energy-momentum of the gravitational field using global quantities (such as the Komar energy/angular momentum, ADM energy-momentum etc.) or pseudo-tensorial quantities (such as the LL pseudo-tensor).

So Dirac's statement is much deeper and much more general than that of an axially symmetric space-time possessing an axial Killing field conserving angular momentum.

Last edited: May 3, 2014
4. May 3, 2014

### bcrowell

Staff Emeritus
There are two different things here:

(1) Conservation of angular momentum for a test particle moving in a fixed background metric.

(2) Conservation of angular momentum for the field theory in general, including the angular momentum contained in the gravitational fields itself.