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A theory that describes how matter interacts dynamically with the geometry of space and time. It was first published by Einstein in 1915 and is currently used to study the structure and evolution of the universe, as well as having practical applications like GPS.

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Why are these vectors perpendicular?

Assuming that $\mathbf F$ is the Faraday tensor, then it is antisymmetric by definition. Therefore, $$E_\lambda X^\lambda = F_{\lambda \mu}X^\mu X^\lambda$$ is the contraction of an antisymmetric obj …
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3 votes

Would time continue to flow forever in a curved spacetime?

No. Note that curved is not the same as closed. For instance, an infinite plane which is distorted so it has small hills and valleys would have curvature, but would not be closed like a sphere is.
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1 vote
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Normal vector of hypersurface in Schwarzshild spacetime

Your surface is defined implicitly by the equation $F(t,r,\theta,\phi) = B$. The natural object which defines the orientation of the surface is not a vector but rather a covector $n_\mu$, with compon …
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4 votes

How small is "vanishingly small" when working with the Schwarzschild metric?

Your question pertains to the 2D Euclidean metric in polar coordinates. Given that $$x = r \cos \phi \qquad y = r \sin\phi$$ It's easy to show that the distance between any two points $(r_1,\phi_1)$ …
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2 votes

Why do we use null geodesics?

Your question is based on a false premise. The equation $$ \frac{d^2x^\mu}{ds^2} + \Gamma^\mu_{ \ \ \alpha\beta} \frac{dx^\alpha}{ds} \frac{dx^\beta}{ds} = 0$$ is solved by any geodesic, whether it b …
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1 vote
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Why is a real manifold (used in GR) defined in the way it is?

The images of open sets can be open or closed tough. Not under homeomorphisms. The image $\psi(O)$ of an open set $O$ under a homeomorphism $\psi$ is also open. One can see this immediately by not …
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0 votes

Falling body geodesics seem counterintuitive

Here is an explicit calculation which might yield some insight. If we take the flat-earth approximation (which in Newtonian mechanics corresponds to $\vec F_g = - mg \hat z$), then an observer standin …
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2 votes

Einstein Summation Problem

If we wanted all possible combinations, it would be a bit silly to use the same letter for both indices. According to the Einstein summation convention, repeated indices are summed over. That is, $$a^ …
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2 votes
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Determinant of metric tensor in Cartesian Coordinates constant in vacuum

$\mathrm{det}(g)$ is not coordinate-independent - it is a scalar density of weight $+2$ (or $-2$, depending on your convention) which generically changes across spacetime. In Minkowski space equipped …
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4 votes
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Isometry between Minkowski space and Tangent space

Two (metric) manifolds $(M,g_M)$ and $(N,g_N)$ are isometric if there exists a diffeomorphism $\varphi:M\rightarrow N$ such that $g_M = \varphi^*g_N$. On the other hand, two pre-Hilbert spaces $(V, \l …
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6 votes

Carroll's interpretation of 1-forms

EDIT: I agree with Kostya that there is likely a typo in Carroll's book, and that the equality of first (not second) derivatives is what's required. I haven't thought about this for long, though, so …
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7 votes
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Why does this derivation of the Einstein Field Equations only work with the Trace-Reversed f...

I will use signature (+---). In the weak-field limit in which $\mathbf g \simeq \boldsymbol \eta + \mathbf h$, the components of the Ricci tensor are given by $$R_{\mu\nu} = -\frac{1}{2}\left(\square …
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2 votes
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Torsion tensor definition doubt

If your confusion is with the apparently missing factor of $1/2$, note that $$\nabla_{[a}\nabla_{b]} \equiv \frac{1}{2}(\nabla_a\nabla_b-\nabla_b\nabla_a)$$ Symmetrization and antisymmetrization brack …
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17 votes
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"And God said ... and the universe was ..." What does this equation mean?

$\gamma:\mathbb R\rightarrow M$ is a curve whose image lies in the spacetime $M$, so $\gamma(t)$ is the event at parameter value $t$ along the curve. $\gamma'(t) \in T_{\gamma(t)}M$ is the tangent v …
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2 votes

Could gravitational waves be matter waves?

The energy being radiated away by gravitational waves is provided by the orbital energy (kinetic + gravitational potential) of the merging bodies. Conceptually, it is basically the same as the electr …
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