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2 votes
2 answers
94 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 ...
Sanjana's user avatar
  • 785
0 votes
1 answer
82 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: ...
emilio grandinetti's user avatar
-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 ...
Krešimir Bradvica's user avatar
4 votes
0 answers
89 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 ...
Daniel Grimmer's user avatar
1 vote
2 answers
150 views

What is the manifold topology of a spinning Cosmic String?

Given the following metric which is that of a rotating Cosmic String: $$g=-c^2 dt^2 + d\rho^2 + (\kappa^2 \rho^2 - a^2) d\phi^2 - 2ac d \phi dt + dz^2.$$ can one determine the manifold topology ...
Bastam Tajik's user avatar
  • 1,212
-1 votes
1 answer
131 views

Geometric Construction of Minkowski Space and Proper Time

In Minkowski spacetime, we define a tangent space at each point and using the metric, we calculate a real number that is the infinitesimal invariant interval between two points. This real number, ...
VVM's user avatar
  • 487
0 votes
1 answer
76 views

How to motivate that in presence of gravity the spacetime metric must be modified to $ds^2=g_{ab}(x)dx^adx^b$?

In the presence of a gravitational field, the spacetime metric, $$ds^2=\eta_{ab}dx^a dx^b,$$ should be changed to, $$ds^2=g_{ab}(x)dx^adx^b.$$ What are the convincing physical arguments that motivate ...
Solidification's user avatar
1 vote
1 answer
54 views

Does the Weyl tensor amount to tidal effects of gravity?

The Ricci tensor, for the spacetime surrounding the Earth, is zero, so the spacetime around the Earth is Ricci-flat. The Riemann tensor though is not zero since spacetime certainly is curved. This ...
Il Guercio's user avatar
2 votes
1 answer
123 views

Could the universe have a form of a $T^3$-torus?

Cosmological measurements suggest that we live in a flat universe. However, what might be less clear is its topology. So could the flat universe have the form of a $T^3$-torus, i.e. the torus whose ...
Frederic Thomas's user avatar
2 votes
1 answer
100 views

Reducing Tensor-rank by fixing an argument

Assume for example that you are given a (2,0) tensor $T^{\mu\nu}$ and you want to create a vector, i.e., a (1,0) tensor out of it. Is it possible to just fix an index of $T^{\mu\nu}$ while keeping the ...
Burgulence's user avatar
1 vote
0 answers
32 views

Example of lightlike curve that's not a geodesic in Lorentz spacetime [duplicate]

Let $(M,g)$ be a 4 dimensional Lorentz spacetime. A smooth curve $\alpha:\ I\to M$ is called lightlike if $\alpha'(s)\in TM_{\alpha(s)}$ is lightlike for all $s\in I$, which means $$g_{\alpha(s)}\big(\...
PermQi's user avatar
  • 143
3 votes
0 answers
87 views

Intuition for the interior Killing vector fields in Schwarzschild?

The Schwarzschild metric represents a stationary (and static), spherically-symmetric, spacetime. These characteristics are manifested by the four Killing vector fields: one for time translation and ...
Ben H's user avatar
  • 1,290
0 votes
0 answers
32 views

Still having trouble understanding gravitational lensing [duplicate]

The normal diagram used to explain gravitational lensing shows a two-dimensional plane that is deflected by a heavy weight. This is a two dimensional description that requires an extra dimension to ...
Michael Mcgarry's user avatar
1 vote
2 answers
82 views

What is Dirac's reasoning when saying parallel displacement creates vector field with vanishing covariant derivative?

Section 12 of Dirac's book "General Theory of Relativity" is called "The condition for flat space", and he is proving that a space is flat if and only if the curvature tensor $R_{\...
Lewis Kirby's user avatar
2 votes
0 answers
59 views

Examples of spacetimes that are asymptotically flat at future timelike infinity

There are interesting non-trivial examples of spacetimes which are asymptotically flat at null and spacelike infinities. For example, the Kerr family of black holes satisfies these conditions. However,...
Níckolas Alves's user avatar

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