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TrickyDicky
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What exactly is the physical meaning of the fact that the covariant derivative of the metric tensor vanishes?
LAHLH said:We choose this property of metric compatibility as it's known when we specify our connection. One could I believe choose different connections to Christoffell for which you wouldn't have metric compatibility, but then these are non physical. The fact that you geodesics are not just curves that parallel transport their tangent vectors wrt connection, but that they are also paths of extremal distance in spacetime is owing to the Christoffell connection being the connection we chose. Metric compat means lots of nice properties too, such as preservation of angle between two parallel transported vectors, or equivalently that geodesics can't change their character from null/timelike/spacelike.
I'm sure someone else will be able to give deeper and maybe more physical reasons still though...
The vanishing of the covariant derivative of the metric—the condition of
metric compatibility—is sometimes introduced perfunctorily in texts on general
relativity, but Schr¨odinger was right to call it “momentous” (Schr¨odinger 1985,
106). It means that the local Lorentz frames associated with a space-time point
p (those for which, at p, the metric tensor takes the form diag(1,−1,−1,−1)
and the first derivatives of all its components vanish) are also local inertial
frames (relative to which the components of the connection vanish at p).10 If
the laws of physics of the non-gravitational interactions are assumed to take
their standard special relativistic form at p relative to such local Lorentz charts
(the local validity of special relativity), then metric compatibility implies that
gravity is not a force in the traditional sense—an agency causing deviation from
natural motion—, in so far as the worldlines of freely falling bodies are geodesics
of the connection.
The full physical implications of the non-metric compatible connection in
Weyl’s theory remain obscure in the absence of a full-blown theory of matter.
Weyl’s hints at a solution to the Einstein objection seem to involve a violation of
minimal coupling, i.e. a violation of the prohibition of curvature coupling in the
non-gravitational equations, and hence of the local validity of special relativity.
But it seems that the familiar insight into the special nature of the gravitational
interaction provided by the strong equivalence principle—the encapsulation of
the considerations given in the previous paragraph—is lost in the Weyl theory.
Right, that's what's been said.bcrowell said:A covariant derivative is a derivative from which we've removed any contribution that is purely a result of the choice of coordinates.
I'm not sure what you mean here, the second derivatives are the ones determined by the metric.bcrowell said:The first derivatives of the metric are the way they are purely as a result of the choice of coordinates.
TrickyDicky said:bcrowell said:The first derivatives of the metric are the way they are purely as a result of the choice of coordinates.
I'm not sure what you mean here, the second derivatives are the ones determined by the metric.
bcrowell said:Since a covariant derivative like [itex]\nabla_a g_{bc}[/itex] is supposed to exclude variation in g that occurs only because of the choice of coordinates, it has to be zero.
bcrowell said:I've never come across a clear explanation of what metric compatibility means (preferably both mathematically and physically), and why we care about it.
A Metric Covariant Derivative is a mathematical operation used in differential geometry to calculate the rate of change of a vector field on a curved manifold. It takes into account the curvature of the manifold by using the metric tensor, which describes the distance between points on the manifold.
While an ordinary derivative is defined on a flat Euclidean space, a Metric Covariant Derivative is defined on a curved manifold. It takes into account the changes in the metric tensor and the curvature of the manifold, whereas an ordinary derivative does not.
The metric tensor plays a crucial role in the Metric Covariant Derivative as it describes the distance between points on the manifold. It allows the derivative to take into account the curvature of the manifold, making it a more accurate measure of the rate of change of a vector field.
The Metric Covariant Derivative is used in many fields, including physics, engineering, and computer graphics. It is used to calculate the motion of objects on curved surfaces, such as planets in orbit or the trajectory of a spaceship. It is also used in fluid dynamics and general relativity.
The Metric Covariant Derivative is calculated using the Levi-Civita connection, which is a way of connecting tangent spaces at different points on a manifold. It involves taking the partial derivatives of the vector field and the metric tensor, and then using them to calculate the rate of change of the vector field in the direction of a given basis vector.