A Riemannian Geometry: GR & Importance Summary

binbagsss
Messages
1,291
Reaction score
12
Hi

I've done a masters taught module in GR and from what I've learned these are two of some of the most important significance of needing a Riemannian Geometry:

1) If we consider the Lagrangian of a freely-falling particle given by ##L= \int ds \sqrt{g_{uv}\dot{dx^u}\dot{dx^v}} ## and find the equations of motion, by the principle of least action this is the shortest path and so must be the definition of a geodesic.

The alternate way to define a geodesic is that the tangent vector of is parallel transported along itself :

##V^u \nabla_u V^a =0 ##

Then via the fundamental theorem of Riemannian geometry,( given a manifold equipped with a non-degenerate, symmetric, differentiable metric there exists a unique torsion-free connection such that ##\nabla_a g_bc =0 ##), we can show that these two definitions of a geodesic are important

2) Due to the fundamental theorem of Riemannian geometry, equipped with a metric on the space-time, we can express important objects such as the Christoffel symbol and Riemman tensor in terms of the metric, and so the metric effectively encodes all the information about the space-time

Are there other important roles played by Riemannian geometry?

I find the first one pretty interesting- is it Palatini formalism that looks at when the geometry is non-Riemmanian and so the geodesics would not be the same?

Thanks in advance.
 
Physics news on Phys.org
So I have read that in Palatini formalism, where the metric and connection are treated independently, if one is to assume any torsion-free connection then metric compatibility comes out by varying the action, is torsion free connection or a non-symmetric connection most widely explored in Palatini formalism?

Also, metric compatibility in GR means we can add the cosmological constant term whilst conserving the energy-momentum tensor still. In a palatini formalism where one does not assume torsion-free, are there any discussions on this or the fact the geodesics defined above do not agree, and a physical interpretation, that anyone could link me to? thanks
 
Yup, I read a paper on this a few months ago, here it is: https://arxiv.org/abs/1606.08756v5

I can recommend some other papers on the topic, but I think the book I mentioned above does go into this discussion as well in the appendix.To add into your question, I always see torsion free being explored because you can add torsion by just using a Dirac field as your source (which should have torsion). Also, if you want torsion and non-symmetry, you would be getting into a third theory which is Weyl's gravity.
 
  • Like
Likes binbagsss
OK, so this has bugged me for a while about the equivalence principle and the black hole information paradox. If black holes "evaporate" via Hawking radiation, then they cannot exist forever. So, from my external perspective, watching the person fall in, they slow down, freeze, and redshift to "nothing," but never cross the event horizon. Does the equivalence principle say my perspective is valid? If it does, is it possible that that person really never crossed the event horizon? The...
From $$0 = \delta(g^{\alpha\mu}g_{\mu\nu}) = g^{\alpha\mu} \delta g_{\mu\nu} + g_{\mu\nu} \delta g^{\alpha\mu}$$ we have $$g^{\alpha\mu} \delta g_{\mu\nu} = -g_{\mu\nu} \delta g^{\alpha\mu} \,\, . $$ Multiply both sides by ##g_{\alpha\beta}## to get $$\delta g_{\beta\nu} = -g_{\alpha\beta} g_{\mu\nu} \delta g^{\alpha\mu} \qquad(*)$$ (This is Dirac's eq. (26.9) in "GTR".) On the other hand, the variation ##\delta g^{\alpha\mu} = \bar{g}^{\alpha\mu} - g^{\alpha\mu}## should be a tensor...
ASSUMPTIONS 1. Two identical clocks A and B in the same inertial frame are stationary relative to each other a fixed distance L apart. Time passes at the same rate for both. 2. Both clocks are able to send/receive light signals and to write/read the send/receive times into signals. 3. The speed of light is anisotropic. METHOD 1. At time t[A1] and time t[B1], clock A sends a light signal to clock B. The clock B time is unknown to A. 2. Clock B receives the signal from A at time t[B2] and...
Back
Top