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0 votes
0 answers
17 views

Hawking and Ellis Lemma 4.3.1 Proof

I have a few questions about Hawking and Ellis' proof of this lemma (pages 92-93): Write the $(2, 0)$ stress-energy tensor in coordinates as $\mathbf{T} = T^{ab} \partial_a \otimes \partial_b$ and ...
2 votes
1 answer
109 views

Boundary conditions on transition maps on general relativity

On the initial courses of topology and differential geometry, we learn again and again about charts, and atlas, and transition maps. I feel that transition maps are a very powerful idea, because they ...
4 votes
1 answer
402 views

What is the geometry of light cones if space is curved/non-Euclidean?

In light cone diagrams, the plane corresponding to the present is always the Euclidean one, but what if space is curved? Now, I've also seen diagrams where spacetime is supposed to be regarded as ...
2 votes
0 answers
60 views

Under what circumstances can a 4D singularity occur in General Relativity?

I've tried to find on the literature about 4D (single point) singularities, but most of the theorems about singularities pertain to either space-like or time-like singularities, which always have some ...
1 vote
1 answer
207 views

Spin connection raise and lower flat indices

The spin connection $\omega^a_{b\nu}$ is used to define the covariant derivative of a spinor in curved spacetime. I want to explicitly calculate the covariant derivative: $$\nabla_\nu\Psi=(\partial_\...
1 vote
1 answer
707 views

Finding the correct Christoffel-symbols in a 2+1D space-time

I'm trying to calculate the Christoffel Symbols in a 2+1D space-time with the following metric: $$ds^2 = N^2(\vec r)c^2dt^2-\phi(\vec r)(dx^1)^2-\phi(\vec r)(dx^2)^2$$ To find the Christoffel ymbols ...
0 votes
1 answer
360 views

Angular Deficit of a Conical Singularity

I'm currently studying the Bonnor solution starting with this paper on Black Diholes. The metric is given by : $$ ds^2 = \left(1-\frac{2Mr}\Sigma\right)^2 \left[-dt^2 + \frac{\Sigma^4}{(\Delta + (M^2 +...
2 votes
2 answers
96 views

Are $i^\pm$ and $i^0$ codimension 1 surfaces?

Standard textbooks like Carroll's say that spatial and temporal infinities in Minkowski space Penrose diagram are points. But on the footnote in pg. 3 of some draft notes on Celestial holography by ...
-1 votes
2 answers
1k views

Does the expansion of the Universe into a higher dimensional space imply that 4D objects are real?

It is my understanding that objects in the Universe are not just getting farther apart but space itself is expanding and so in some real sense, higher-dimensional geometry is "real" -- if so, on a ...
0 votes
1 answer
83 views

What objects are solutions to the Einstein Field Equations?

The usual way the solutions of the Einstien Field Equations are introduced is by saying they are (pseudo-) riemannian metrics that satiafy the diff equations for a given EM Tensor. My question is: ...
98 votes
9 answers
23k views

What is a manifold? [closed]

For complete dummies when it comes to space-time, what is a manifold and how can space-time be modelled using these concepts?
4 votes
0 answers
92 views

Is the causal structure completely determined by the Weyl tensor alone?

By causal/conformal structure I mean the context of Malament's 1977 theorem. If I understand correctly this means that any two spacetimes which agree about all of the future-directed continuous ...
2 votes
2 answers
260 views

Is a stationary spacetime automatically globally hyperbolic?

Is a stationary spacetime automatically globally hyperbolic? Can one construct a Cauchy-Surface by the existence of a global timelike Killing Vector field?
2 votes
1 answer
3k views

Ricci scalar curvature in FLRW flat universe

I have a simple question about the relation between the Ricci scalar curvature and the $k$ constant in the Friedmann–Lemaître–Robertson–Walker solution. Assuming $k=0$, such that the space can be ...
-1 votes
1 answer
53 views

If an area in 2D cannot be curved and finite is the same regarding the space of our pressumed 3D universe?

Is the sentence in the title right that our universe is infinite? And if so does it mean that stars are not evenly distributed along our universe but they all move from a populated centre to a fairly ...

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